0000000000592624

AUTHOR

Paolo Pagano

showing 114 related works from this author

Linking Small-scale Solar Wind Properties with Large-scale Coronal Source Regions through Joint Parker Solar Probe–Metis/Solar Orbiter Observations

2022

Abstract The solar wind measured in situ by Parker Solar Probe in the very inner heliosphere is studied in combination with the remote-sensing observation of the coronal source region provided by the METIS coronagraph aboard Solar Orbiter. The coronal outflows observed near the ecliptic by Metis on 2021 January 17 at 16:30 UT, between 3.5 and 6.3 R ⊙ above the eastern solar limb, can be associated with the streams sampled by PSP at 0.11 and 0.26 au from the Sun, in two time intervals almost 5 days apart. The two plasma flows come from two distinct source regions, characterized by different magnetic field polarity and intensity at the coronal base. It follows that both the global and local p…

Magnetohydrodynamics (694)Settore FIS/05 - Astronomia E AstrofisicaAstronomi astrofysik och kosmologiSpace and Planetary ScienceSolar corona (1483)Space plasmas (1544)Solar wind (1534)Interplanetary turbulence (830)Astronomy Astrophysics and CosmologyAstronomy and AstrophysicsAlfven waves (23)Heliosphere (711)
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Measuring the electron temperatures of coronal mass ejections with future space-based multi-channel coronagraphs: a numerical test

2018

Context. The determination from coronagraphic observations of physical parameters of the plasma embedded in coronal mass ejections (CMEs) is of crucial importance for our understanding of the origin and evolution of these phenomena. Aims. The aim of this work is to perform the first ever numerical simulations of a CME as it will be observed by future two-channel (visible light VL and UV Ly-α) coronagraphs, such as the Metis instrument on-board ESA-Solar Orbiter mission, or any other future coronagraphs with the same spectral band-passes. These simulations are then used to test and optimize the plasma diagnostic techniques to be applied to future observations of CMEs. Methods. The CME diagno…

010504 meteorology & atmospheric sciencesSun: coronal mass ejections (CMEs)Plasma parametersT-NDASContext (language use)Astrophysics01 natural sciencessymbols.namesakeMethods: data analysis0103 physical sciencesRadiative transferCoronal mass ejectionAstrophysics::Solar and Stellar AstrophysicsQB Astronomydata analysis [Methods]010303 astronomy & astrophysicsQCQB0105 earth and related environmental sciencesPhysicsUV radiation [Sun]numerical [Methods]Methods: numericalAstronomy and AstrophysicsPlasmaSun: UV radiationPolarization (waves)coronal mass ejections (CMEs) [Sun]Computational physicsQC PhysicsPlasmasSpace and Planetary SciencePhysics::Space PhysicssymbolsMagnetohydrodynamicsDoppler effectAstronomy & Astrophysics
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A fast multi-dimensional magnetohydrodynamic formulation of the transition region adaptive conduction (TRAC) method

2021

We have demonstrated that the Transition Region Adaptive Conduction (TRAC) method permits fast and accurate numerical solutions of the field-aligned hydrodynamic equations, successfully removing the influence of numerical resolution on the coronal density response to impulsive heating. This is achieved by adjusting the parallel thermal conductivity, radiative loss, and heating rates to broaden the transition region (TR), below a global cutoff temperature, so that the steep gradients are spatially resolved even when using coarse numerical grids. Implementing the original 1D formulation of TRAC in multi-dimensional magnetohydrodynamic (MHD) models would require tracing a large number of magne…

Sun: flaresMagnetohydrodynamics (MHD)010504 meteorology & atmospheric sciencescorona [Sun]Field lineNDASFOS: Physical scienceschromosphere [Sun]Astrophysics01 natural sciencestransition region [Sun]0103 physical sciencesRadiative transferQB AstronomyMagnetohydrodynamic driveflares hydrodynamics [Sun]Sun: transition region010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)QC0105 earth and related environmental sciencescomputer.programming_languageQBPhysicsSun: coronaSun: chromosphereAstronomy and AstrophysicsTRACCoronal loopThermal conductionComputational physicsMagnetic fieldQC PhysicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceHydrodynamicsMagnetohydrodynamicscomputerSettore FIS/06 - Fisica Per Il Sistema Terra E Il Mezzo Circumterrestre
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Measurement of charged jet production cross sections and nuclear modification in p–Pb collisions at sNN=5.02 TeV

2015

Charged jet production cross sections in p–Pb collisions at √sNN = 5.02 TeV measured with the ALICE detector at the LHC are presented. Using the anti-kT algorithm, jets have been reconstructed in the central rapidity region from charged particles with resolution parameters R = 0.2 and R = 0.4. The reconstructed jets have been corrected for detector effects and the underlying event background. To calculate the nuclear modification factor, RpPb, of charged jets in p–Pb collisions, a pp reference was constructed by scaling previously measured charged jet spectra at √s = 7 TeV. In the transverse momentum range 20 ≤ pT, ch jet ≤ 120 GeV/c, RpPb is found to be consistent with unity, indicating th…

PhysicsNuclear and High Energy PhysicsJet (fluid)Particle physicsRange (particle radiation)Large Hadron ColliderAstrophysics::High Energy Astrophysical PhenomenaNuclear matterSpectral lineCharged particleNuclear physicsHigh Energy Physics::ExperimentRapidityNuclear ExperimentScalingPhysics Letters B
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Understanding the Origins of Problem Geomagnetic Storms Associated with "Stealth" Coronal Mass Ejections.

2021

Geomagnetic storms are an important aspect of space weather and can result in significant impacts on space- and ground-based assets. The majority of strong storms are associated with the passage of interplanetary coronal mass ejections (ICMEs) in the near-Earth environment. In many cases, these ICMEs can be traced back unambiguously to a specific coronal mass ejection (CME) and solar activity on the frontside of the Sun. Hence, predicting the arrival of ICMEs at Earth from routine observations of CMEs and solar activity currently makes a major contribution to the forecasting of geomagnetic storms. However, it is clear that some ICMEs, which may also cause enhanced geomagnetic activity, cann…

010504 meteorology & atmospheric sciencesSpace weather01 natural scienceslaw.inventionDIMMINGSPhysics - Space PhysicslawRECONNECTIONCoronal mass ejectionQB Astronomy010303 astronomy & astrophysicsCoronagraphQCMISSIONQBSTREAMERSUN3rd-DASLow-coronal signaturesMagnetic StormsAstrophysics - Solar and Stellar AstrophysicsMagnetic stormsPhysical SciencesCURRENT SHEETSpace WeatherGeologyCoronal Mass EjectionsSettore FIS/06 - Fisica Per Il Sistema Terra E Il Mezzo CircumterrestreSpace weatherSOLAR-WIND HELIUMMAGNETIC CLOUDSFOS: Physical sciencesSolar cycle 24Astronomy & AstrophysicsArticleCurrent sheet0103 physical sciencesSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesGeomagnetic stormScience & TechnologyAstronomyAstronomy and AstrophysicsSpace Physics (physics.space-ph)EVOLUTIONEarth's magnetic fieldQC Physics13. Climate actionSpace and Planetary Science[SDU]Sciences of the Universe [physics]Low-Coronal SignaturesCoronal mass ejectionsMAGNETOHYDRODYNAMIC MODELSInterplanetary spaceflightSpace science reviews
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D -Meson Azimuthal Anisotropy in Midcentral Pb-Pb Collisions at sNN=5.02  TeV

2018

A.I. Alikhanyan National Science Laboratory (Yerevan Physics Institute) Foundation (ANSL), State Committee of Science and World Federation of Scientists (WFS), Armenia; Austrian Academy of Sciences and Nationalstiftung fur Forschung, Technologie und Entwicklung, Austria; Ministry of Communications and High Technologies, National Nuclear Research Center, Azerbaijan; Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq), Universidade Federal do Rio Grande do Sul (UFRGS), Financiadora de Estudos e Projetos (Finep), and Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP), Brazil; Ministry of Science and Technology of China (MSTC), National Natural Science Foundation of …

Particle physicsHigher education010308 nuclear & particles physicsbusiness.industry4. EducationAtomic energyIndustrial researchGeneral Physics and AstronomyLibrary science01 natural scienceslanguage.human_languageBildungResearch centrePolitical science0103 physical scienceslanguageSlovak010306 general physicsChinabusinessResearch centerPhysical Review Letters
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Hydrogen non-equilibrium ionisation effects in coronal mass ejections

2020

This research has received funding from the Science and Technology Facilities Council (UK) through the consolidated grant ST/N000609/1 and the European Research Council (ERC) under the European Union Horizon 2020 research and innovation program (grant agreement No. 647214). D.H.M. would like to thank both the UK STFC and the ERC (Synergy grant: WHOLE SUN, grant Agreement No. 810218) for financial support. D.H.M. and P.P. would like to thank STFC for IAA funding under grant number SMC1-XAS012. This work used the DiRAC@Durham facility man-aged by the Institute for Computational Cosmology on behalf of the STFC DiRAC HPC Facility (www.dirac.ac.uk. The equipment was funded by BEIS capital fundin…

Magnetohydrodynamics (MHD)010504 meteorology & atmospheric sciencesHydrogenSun: coronal mass ejections (CMEs)FOS: Physical scienceschemistry.chemical_elementAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciences7. Clean energycoronal mass ejections (CMEs) [un]Ionization0103 physical sciencesCoronal mass ejectionAstrophysics::Solar and Stellar AstrophysicsQB Astronomydata analysis [Methods]Sun: magnetic fields010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)QCQB0105 earth and related environmental sciencesPhysicsUV radiation [Sun]Sun: coronaAstronomy and Astrophysics3rd-DASPlasmaMagnetic fluxSolar windQC PhysicsAstrophysics - Solar and Stellar AstrophysicschemistrySpace and Planetary SciencePhysics::Space PhysicsPlasma diagnosticsMagnetohydrodynamicsAstronomy & Astrophysics
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Measurement of PromptD-Meson Production inp−PbCollisions atsNN=5.02  TeV

2014

The p_{T}-differential production cross sections of the prompt charmed mesons D^{0}, D^{+}, D^{*+}, and D_{s}^{+} and their charge conjugate in the rapidity interval -0.96<y_{cms}<0.04 were measured in p-Pb collisions at a center-of-mass energy sqrt[s_{NN}]=5.02 TeV with the ALICE detector at the LHC. The nuclear modification factor R_{pPb}, quantifying the D-meson yield in p-Pb collisions relative to the yield in pp collisions scaled by the number of binary nucleon-nucleon collisions, is compatible within the 15%-20% uncertainties with unity in the transverse momentum interval 1<p_{T}<24 GeV/c. No significant difference among the R_{pPb} of the four D-meson species is observed. The results…

PhysicsParticle physicsMeson010308 nuclear & particles physicsHadronGeneral Physics and Astronomy7. Clean energy01 natural sciencesNuclear physicsMomentum0103 physical sciencesD mesonHigh Energy Physics::ExperimentProduction (computer science)RapidityNuclear Experiment010306 general physicsEnergy (signal processing)BosonPhysical Review Letters
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J/ψ suppression at forward rapidity in Pb–Pb collisions at sNN=5.02 TeV

2017

The inclusive J/$\psi$ production has been studied in Pn-Pb and pp collisions at the centre-of-mass energy per nucleon pair $\sqrt{s_{\rm NN}}=5.02$ TeV, using the ALICE detector at the CERN LHC. The J/$\psi$ meson is reconstructed, in the centre-of-mass rapidity interval $2.5<y<4$ and in the transverse-momentum range $p_{\rm T}<12$ GeV/$c$, via its decay to a muon pair. In this Letter, we present results on the inclusive J/$\psi$ cross section in pp collisions at $\sqrt{s}=5.02$ TeV and on the nuclear modification factor $R_{\rm AA}$. The latter is presented as a function of the centrality of the collision and, for central collisions, as a function of the transverse momentum $p_{\rm T}$ of…

PhysicsNuclear and High Energy PhysicsParticle physicsMuonMeson010308 nuclear & particles physics01 natural sciencesNuclear physics0103 physical sciencesQuark–gluon plasmaHigh Energy Physics::ExperimentRapidityProduction (computer science)Impact parameterNuclear Experiment010306 general physicsNucleonEnergy (signal processing)Physics Letters B
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Production of Muons from Heavy Flavor Decays at Forward Rapidity inppand Pb-Pb Collisions atsNN=2.76  TeV

2012

The ALICE Collaboration has measured the inclusive production of muons from heavy-flavor decays at forward rapidity, 2.5 < y < 4, in pp and Pb-Pb collisions at root s(NN) = 2.76 TeV. The p(t)-differential inclusive cross section of muons from heavy-flavor decays in pp collisions is compared to perturbative QCD calculations. The nuclear modification factor is studied as a function of p(t) and collision centrality. A weak suppression is measured in peripheral collisions. In the most central collisions, a suppression of a factor of about 3-4 is observed in 6 < p(t) < 10 GeV/c. The suppression shows no significant p(t) dependence.

PhysicsParticle physicsMuon010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyGeneral Physics and AstronomyPerturbative QCDModification factor01 natural sciencesNuclear physics0103 physical sciencesHigh Energy Physics::ExperimentRapidityNuclear Experiment010306 general physicsFlavorPhysical Review Letters
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J/ψElliptic Flow in Pb-Pb Collisions atsNN=2.76  TeV

2013

We report on the first measurement of inclusive J/psi elliptic flow v(2) in heavy-ion collisions at the LHC. The measurement is performed with the ALICE detector in Pb-Pb collisions at root s(NN) = 2.76 TeV in the rapidity range 2.5 < y < 4.0. The dependence of the J/psi v(2) on the collision centrality and on the J/psi transverse momentum is studied in the range 0 <= p(T) < 10 GeV/c. For semicentral Pb-Pb collisions at root s(NN) = 2.76 TeV, an indication of nonzero v(2) is observed with a largest measured value of v(2) = 0.116 +/-0.046(stat) +/- 0.029(syst) for J/psi in the transverse momentum range 2 <= p(T) < 4 GeV/c. The elliptic flow measurement complements the previously reported ALI…

PhysicsParticle physicsLarge Hadron Collider010308 nuclear & particles physicsElliptic flowGeneral Physics and AstronomyModification factor01 natural sciencesDeconfinementCharm quarkNuclear physics0103 physical sciencesQuark–gluon plasmaTransverse momentumHigh Energy Physics::ExperimentRapidityNuclear Experiment010306 general physicsPhysical Review Letters
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Models and data analysis tools for the Solar Orbiter mission

2020

All authors: Rouillard, A. P.; Pinto, R. F.; Vourlidas, A.; De Groof, A.; Thompson, W. T.; Bemporad, A.; Dolei, S.; Indurain, M.; Buchlin, E.; Sasso, C.; Spadaro, D.; Dalmasse, K.; Hirzberger, J.; Zouganelis, I.; Strugarek, A.; Brun, A. S.; Alexandre, M.; Berghmans, D.; Raouafi, N. E.; Wiegelmann, T.; Pagano, P.; Arge, C. N.; Nieves-Chinchilla, T.; Lavarra, M.; Poirier, N.; Amari, T.; Aran, A.; Andretta, V.; Antonucci, E.; Anastasiadis, A.; Auchère, F.; Bellot Rubio, L.; Nicula, B.; Bonnin, X.; Bouchemit, M.; Budnik, E.; Caminade, S.; Cecconi, B.; Carlyle, J.; Cernuda, I.; Davila, J. M.; Etesi, L.; Espinosa Lara, F.; Fedorov, A.; Fineschi, S.; Fludra, A.; Génot, V.; Georgoulis, M. K.; Gilbe…

010504 meteorology & atmospheric sciencescorona [Sun]Solar windAstrophysics[SDU.ASTR] Sciences of the Universe [physics]/Astrophysics [astro-ph]7. Clean energy01 natural scienceslaw.inventionData acquisitionlawCoronal mass ejectiongeneral [Sun]QB AstronomyAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSun: magnetic fieldsQCComputingMilieux_MISCELLANEOUSQBPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]3rd-DASenergetic particlesSolar windCORONAL MASS EJECTIONSnumerical modelingmagnetic fields [Sun]solar windPhysics::Space PhysicsSystems engineeringAstrophysics::Earth and Planetary Astrophysicsatmosphere [Sun]fundamental parameters [Sun]Sun: generalFORCE-FREE FIELDSun: fundamental parametersSolar radiusContext (language use)STREAMER STRUCTUREOrbiter0103 physical sciencesOPTIMIZATION APPROACH[SDU.ASTR.SR] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]POLARIZATION MEASUREMENTSSun: Solar wind3-DIMENSIONAL STRUCTURE0105 earth and related environmental sciencesSpacecraftbusiness.industrySun: corona[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]solar coronaMAGNETIC-FLUX ROPESAstronomy and AstrophysicsSHOCKS DRIVEN115 Astronomy Space scienceSPECTRAL-LINESQC Physics13. Climate actionSpace and Planetary SciencebusinessHeliosphereSun: atmosphereELECTRON-DENSITY
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Elliptic flow of muons from heavy-flavour hadron decays at forward rapidity in Pb–Pb collisions at sNN=2.76 TeV

2016

The elliptic flow, $v_{2}$, of muons from heavy-flavour hadron decays at forward rapidity ($2.5 < y < 4$) is measured in Pb--Pb collisions at $\sqrt{s_{\rm NN}}$~=~2.76 TeV with the ALICE detector at the LHC. The scalar product, two- and four-particle $Q$ cumulants and Lee-Yang zeros methods are used. The dependence of the $v_2$ of muons from heavy-flavour hadron decays on the collision centrality, in the range 0--40\%, and on transverse momentum, $p_{\rm T}$, is studied in the interval $3 < p_{\rm T} < 10$~GeV/$c$. A positive $v_2$ is observed with the scalar product and two-particle $Q$ cumulants in semi-central collisions (10--20\% and 20--40\% centrality classes) for the $p_{\rm T}$ int…

PhysicsQuarkNuclear and High Energy PhysicsParticle physicsMuon010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyElliptic flowHadron01 natural sciencesHadronizationNuclear physicsPion0103 physical sciencesHigh Energy Physics::ExperimentRapidityImpact parameterNuclear Experiment010306 general physicsPhysics Letters B
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Pseudorapidity Density of Charged Particles inp+PbCollisions atsNN=5.02  TeV

2013

The charged-particle pseudorapidity density measured over four units of pseudorapidity in nonsingle-diffractive p + Pb collisions at a center-of-mass energy per nucleon pair root s(NN) = 5.02 TeV is presented. The average value at midrapidity is measured to be 16.81 +/- 0.71 (syst), which corresponds to 2.14 +/- 0.17 (syst) per participating nucleon, calculated with the Glauber model. This is 16% lower than in nonsingle-diffractive pp collisions interpolated to the same collision energy and 84% higher than in d + Au collisions at root s(NN) = 0.2 TeV. The measured pseudorapidity density in p + Pb collisions is compared to model predictions and provides new constraints on the description of …

PhysicsHigh energyParticle physics010308 nuclear & particles physicsModel predictionGeneral Physics and Astronomy01 natural sciencesCharged particleNuclear physicsPseudorapidity0103 physical sciencesHigh Energy Physics::ExperimentMultiplicity (chemistry)Nuclear Experiment010306 general physicsNucleonGlauberTellurium compoundsPhysical Review Letters
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Contribution of phase-mixing of Alfvén waves to coronal heating in multi-harmonic loop oscillations

2018

This research has received funding from the Science and Technology Facilities Council (UK) through the consolidated grant ST/N000609/1 and the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation program ( grant agreement No. 647214). This work is supported by the European Research Council under the SeismoSun Research Project No. 321141 (DJP). This project has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No 724326). This work used the DiRAC Data Centric system at Durham University, operated by the Institute for Computational Cosmology on behalf o…

Magnetohydrodynamics (MHD)corona [Sun]010504 meteorology & atmospheric sciencesAstrophysics7. Clean energy01 natural sciencesCoronal heatingQB AstronomyRESONANT ABSORPTIONAstrophysics::Solar and Stellar AstrophysicsQASun: magnetic fields010303 astronomy & astrophysicsQCQBSun: helioseismologymedia_commonPhysicsoscillations [Sun]European researchAstrophysics::Instrumentation and Methods for AstrophysicsKINK OSCILLATIONSmagnetic fields [Sun]MHD WAVESAstrophysics - Solar and Stellar AstrophysicsPhysical SciencesPhysics::Space Physicsatmosphere [Sun]INSTABILITYDirac (software)NDASTRACELibrary scienceAstronomy & AstrophysicsComputer Science::Digital Librariesmagnetohydrodynamics (MHD)0103 physical sciencesmedia_common.cataloged_instancewavesQA Mathematicshelioseismology [Sun]Sun: oscillationsEuropean unionPhase mixing0105 earth and related environmental sciencesScience & TechnologySun: coronaSEISMOLOGYAstronomy and AstrophysicsPhysics::History of PhysicsQC PhysicsSpace and Planetary ScienceWavesTRANSVERSE OSCILLATIONSAstronomy &amp; Astrophysics
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KS0andΛProduction in Pb-Pb Collisions atsNN=2.76  TeV

2013

The ALICE measurement of K^0_S and {\Lambda} production at mid-rapidity in Pb-Pb collisions at sqrt(sNN) = 2.76 TeV is presented. The transverse momentum (pT) spectra are shown for several collision centrality intervals and in the pT range from 0.4 GeV/c (0.6 GeV/c for {\Lambda}) to 12 GeV/c. The pT dependence of the {\Lambda}/K^0_S ratios exhibits maxima in the vicinity of 3 GeV/c, and the positions of the maxima shift towards higher pT with increasing collision centrality. The magnitude of these maxima increases by almost a factor of three between most peripheral and most central Pb-Pb collisions. This baryon excess at intermediate pT is not observed in pp interactions at sqrt(s) = 0.9 Te…

PhysicsParticle physicsLarge Hadron Collider010308 nuclear & particles physicsHadronGeneral Physics and AstronomyLambda01 natural sciencesSpectral lineHadronizationNuclear physicsBaryon0103 physical sciencesQuark–gluon plasmaHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsMaximaPhysical Review Letters
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Effect of gravitational stratification on the propagation of a CME

2013

Our aim is to study the role of gravitational stratification on the propagation of CMEs. In particular, we assess how it influences the speed and shape of CMEs and under what conditions the flux rope ejection becomes a CME or when it is quenched. We ran a set of MHD simulations that adopt an eruptive initial magnetic configuration that has already been shown to be suitable for a flux rope ejection. We varied the temperature of the backgroud corona and the intensity of the initial magnetic field to tune the gravitational stratification and the amount of ejected magnetic flux. We used an automatic technique to track the expansion and the propagation of the magnetic flux rope in the MHD simula…

Magnetohydrodynamics (MHD)010504 meteorology & atmospheric sciencescorona [Sun]Sun: coronal mass ejections (CMEs)Stratification (water)FOS: Physical sciencesAstrophysics01 natural sciencesmagnetohydrodynamics (MHD)Physics - Space Physics0103 physical sciencesGravitational stratificationCoronal mass ejectionQB AstronomyAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsFlux rope ejectionSolar and Stellar Astrophysics (astro-ph.SR)QB0105 earth and related environmental sciencesPhysicsCoronal mass ejections (CMEs)Sun: coronaAstronomy and AstrophysicsPlasmaCoronaMagnetic fluxSpace Physics (physics.space-ph)coronal mass ejections (CMEs) [Sun]Magnetic fieldAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsMagnetohydrodynamicsRope
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Flow dominance and factorization of transverse momentum correlations in Pb-Pb collisions at the LHC

2017

Physical review letters 118(16), 162302 (2017). doi:10.1103/PhysRevLett.118.162302

heavy ion: scattering:Kjerne- og elementærpartikkelfysikk: 431 [VDP]transverse momentum [correlation function]correlation [momentum]550Pb-PbPb-Pb collisionsGeneral Physics and Astronomyhiukkasfysiikkanucl-exPP01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)ALICEDEPENDENCEddc:550Nuclear Experiment (nucl-ex)ROOT-S(NN)=2.76 TEVNuclear ExperimentPERSPECTIVENuclear ExperimentPhysics and Astronomy (all); ALICE; LHCPhysicscorrelation function: transverse momentumPhysicsflow ; transverse ; momentum ; Pb-Pbtransverse momentum: correlationtwo-particleHanbury-Brown-Twiss effect:Mathematics and natural scienses: 400::Physics: 430::Nuclear and elementary particle physics: 431 [VDP]PRIRODNE ZNANOSTI. Fizika.transverseTransverse planeCorrelation function (statistical mechanics)CERN LHC Coll:Nuclear and elementary particle physics: 431 [VDP]flowPseudorapidityLHCParticle Physics - ExperimentdeconfinementParticle physicscollectiveVDP::Matematikk og naturvitenskap: 400::Fysikk: 430::Kjerne- og elementærpartikkelfysikk: 431FOS: Physical sciencesmomentumtriangulationPhysics and Astronomy(all)[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]114 Physical sciencesBethe ansatzMomentumNuclear physicsCENTRALITYPhysics and Astronomy (all)statistical analysisFactorizationscattering [heavy ion]Relativistic heavy-ion collisions0103 physical sciencesALICE / ALICE2760 GeV-cmsNuclear Physics - ExperimentRapiditystructurenumerical calculations010306 general physicsNuclear Physicstwo-particle transverse momentum differential correlation functionAnsatzleadDEPENDENCE PERSPECTIVE CENTRALITY PP.ta114VDP::Mathematics and natural scienses: 400::Physics: 430::Nuclear and elementary particle physics: 431hep-ex010308 nuclear & particles physics:Matematikk og naturvitenskap: 400::Fysikk: 430::Kjerne- og elementærpartikkelfysikk: 431 [VDP]momentum: correlationBethe ansatzROOT-S(NN)=2.76 TEV; DEPENDENCE; PERSPECTIVE; PPNATURAL SCIENCES. Physics.rapiditypile-uptransverse momentum: factorizationfactorization [transverse momentum]correlation [transverse momentum]experimental results
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Pseudorapidity dependence of the anisotropic flow of charged particles in Pb–Pb collisions at sNN=2.76 TeV

2016

We present measurements of the elliptic ($\mathrm{v}_2$), triangular ($\mathrm{v}_3$) and quadrangular ($\mathrm{v}_4$) anisotropic azimuthal flow over a wide range of pseudorapidities ($-3.5< \eta < 5$). The measurements are performed with Pb-Pb collisions at $\sqrt{s_{\text{NN}}} = 2.76$ TeV using the ALICE detector at the Large Hadron Collider (LHC). The flow harmonics are obtained using two- and four-particle correlations from nine different centrality intervals covering central to peripheral collisions. We find that the shape of $\mathrm{v}_n(\eta)$ is largely independent of centrality for the flow harmonics $n=2-4$, however the higher harmonics fall off more steeply with increasing $|…

PhysicsNuclear and High Energy PhysicsLarge Hadron Collider010308 nuclear & particles physicsElliptic flow01 natural sciencesCharged particleNuclear physicsPseudorapidityHarmonics0103 physical sciencesQuark–gluon plasmaHigh Energy Physics::ExperimentRapidityNuclear Experiment010306 general physicsScalingPhysics Letters B
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Contribution of mode coupling and phase-mixing of Alfv\'en waves to coronal heating

2017

This research has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No. 647214) and from the UK Science and Technology Facilities Council. This work used the DiRAC Data Centric system at Durham University, operated by the Institute for Computational Cosmology on behalf of the STFC DiRAC HPC Facility (www.dirac.ac.uk. This equipment was funded by a BIS National E-infrastructure capital grant ST/K00042X/1, STFC capital grant ST/K00087X/1, DiRAC Operations grant ST/K003267/1 and Durham University. Context. Phase-mixing of Alfvén waves in the solar corona has been identified as one possible candid…

Work (thermodynamics)Magnetohydrodynamics (MHD)corona [Sun]010504 meteorology & atmospheric sciencesNDASSun: Magnetic fieldsContext (language use)Astrophysics7. Clean energy01 natural sciences0103 physical sciencesThermalQB AstronomyAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsQCQB0105 earth and related environmental sciencesPhysicsSun: Coronabusiness.industrySun: Oscillationsoscillations [Sun]Astronomy and AstrophysicsCoronal loopMechanicsBoundary layerQC Physicsmagnetic fields [Sun]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceMode couplingPhysics::Space PhysicsWavesMagnetohydrodynamicsbusinessThermal energy
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MHD evolution of a fragment of a CME core in the outer solar corona

2007

Detailed hydrodynamic modeling explained several features of a fragment of the core of a Coronal Mass Ejection observed with SoHO/UVCS at 1.7 Ro on 12 December 1997, but some questions remained unsolved. We investigate the role of the magnetic fields in the thermal insulation and the expansion of an ejected fragment (cloud) traveling upwards in the outer corona. We perform MHD simulations including the effects of thermal conduction and radiative losses of a dense spherical or cylindrical cloud launched upwards in the outer corona, with various assumptions on the strength and topology of the ambient magnetic field; we also consider the case of a cylindrical cloud with an internal magnetic fi…

Physicsbusiness.industryAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsThermal conductionAstrophysicsCoronaMagnetic fieldSpace and Planetary ScienceThermal insulationBeta (plasma physics)Physics::Space PhysicsRadiative transferCoronal mass ejectionAstrophysics::Solar and Stellar AstrophysicsMagnetohydrodynamicsbusinessSun: coronal mass ejections (CMEs) – magnetohydrodynamics (MHD) – Sun: corona
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Azimuthal anisotropy ofD-meson production in Pb-Pb collisions atsNN=2.76TeV

2014

The production of the prompt charmed mesons D0, D+, and D*+ relative to the reaction plane was measured in Pb-Pb collisions at a center-of-mass energy per nucleon-nucleon collision of √sNN=2.76TeV with the ALICE detector at the CERN Large Hadron Collider. D mesons were reconstructed via their hadronic decays at central rapidity in the transverse-momentum (p_T) interval 2–16 GeV/c. The azimuthal anisotropy is quantified in terms of the second coefficient v2 in a Fourier expansion of the D-meson azimuthal distribution and in terms of the nuclear modification factor R_AA, measured in the direction of the reaction plane and orthogonal to it. The v2 coefficient was measured with three different …

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderMeson010308 nuclear & particles physicsPlane (geometry)Hadron01 natural sciences7. Clean energyNuclear physicsYield (chemistry)0103 physical sciencesD mesonHigh Energy Physics::ExperimentRapidityNuclear Experiment010306 general physicsAnisotropyPhysical Review C
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Charge separation relative to the reaction plane in Pb-Pb collisions atsNN=2.76  TeV

2013

Measurements of charge-dependent azimuthal correlations with the ALICE detector at the LHC are reported for Pb-Pb collisions at root s(NN) = 2.76 TeV. Two- and three-particle charge-dependent azimuthal correlations in the pseudorapidity range vertical bar eta vertical bar < 0.8 are presented as a function of the collision centrality, particle separation in pseudorapidity, and transverse momentum. A clear signal compatible with a charge-dependent separation relative to the reaction plane is observed, which shows little or no collision energy dependence when compared to measurements at RHIC energies. This provides a new insight for understanding the nature of the charge-dependent azimuthal co…

PhysicsParticle physicsRange (particle radiation)Large Hadron Collider010308 nuclear & particles physicsPlane (geometry)DetectorGeneral Physics and AstronomyCollision01 natural sciencesNuclear physicsAzimuthPseudorapidity0103 physical sciencesHigh Energy Physics::ExperimentImpact parameterNuclear Experiment010306 general physicsPhysical Review Letters
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Long-range angular correlations of π, K and p in p–Pb collisions at sNN=5.02 TeV

2013

Angular correlations between unidentified charged trigger particles and various species of charged associated particles (unidentified particles, pions, kaons, protons and antiprotons) are measured by the ALICE detector in p-Pb collisions at a nucleon-nucleon centre-of-mass energy of 5.02 TeV in the transverse-momentum range 0.3 < p(T) < 4 GeV/c. The correlations expressed as associated yield per trigger particle are obtained in the pseudorapidity range vertical bar n(lab)vertical bar < 0.8. Fourier coefficients are extracted from the long-range correlations projected onto the azimuthal angle difference and studied as a function of p(T) and in intervals of event multiplicity. In high-multipl…

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderProton010308 nuclear & particles physicsElliptic flowHadron01 natural sciencesNuclear physicsPionAntiprotonPseudorapidity0103 physical sciencesHigh Energy Physics::ExperimentMultiplicity (chemistry)Nuclear Experiment010306 general physicsPhysics Letters B
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ϕ-Meson production at forward rapidity in p–Pb collisions at sNN=5.02 TeV and in pp collisions at s=2.76 TeV

2017

The first study of $\phi$-meson production in p–Pb collisions at forward and backward rapidity, at a nucleon– nucleon centre-of-mass energy $\sqrt{S_{NN}}$= 5.02 TeV, has been performed with the ALICE apparatus at the LHC. The $\phi$-mesons have been identified in the dimuon decay channel in the transverse momentum ($p_T$) range 1 < $p_T$ < 7 GeV/c, both in the p-going (2.03 < y < 3.53) and the Pb-going (−4.46 < y < −2.96) directions — where $y$ stands for the rapidity in the nucleon–nucleon centre-of-mass — the integrated luminosity amounting to 5.01 ± 0.19 nb$^{−1}$ and 5.81 ± 0.20 nb$^{−1}$ , respectively, for the two data samples. Differential cross sections as a function of transverse …

PhysicsNuclear and High Energy PhysicsParticle physicsMeson010308 nuclear & particles physicsBranching fractionHadronStrangeness01 natural sciencesNuclear physics0103 physical sciencesHigh Energy Physics::ExperimentProduction (computer science)RapidityAbsorption (logic)Nuclear Experiment010306 general physicsNucleonPhysics Letters B
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J/ψSuppression at Forward Rapidity in Pb-Pb Collisions atsNN=2.76  TeV

2012

The ALICE experiment has measured the inclusive J/psi production in Pb-Pb collisions at root s(NN) = 2.76 TeV down to zero transverse momentum in the rapidity range 2.5 < y < 4. A suppression of the inclusive J/psi yield in Pb-Pb is observed with respect to the one measured in pp collisions scaled by the number of binary nucleon-nucleon collisions. The nuclear modification factor, integrated over the 0%-80% most central collisions, is 0.545 +/- 0.032(stat) +/- 0.083dsyst_ and does not exhibit a significant dependence on the collision centrality. These features appear significantly different from measurements at lower collision energies. Models including J/psi production from charm quarks in…

PhysicsParticle physicsRange (particle radiation)010308 nuclear & particles physicsGeneral Physics and AstronomyModification factor01 natural sciencesDeconfinementCharm quarkNuclear physicsYield (chemistry)0103 physical sciencesTransverse momentumHigh Energy Physics::ExperimentRapidityImpact parameterNuclear Experiment010306 general physicsPhysical Review Letters
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Anisotropic Flow of Charged Particles in Pb-Pb Collisions atsNN=5.02  TeV

2016

We report the first results of elliptic (v2), triangular (v3), and quadrangular (v4) flow of charged particles in Pb-Pb collisions at a center-of-mass energy per nucleon pair of √sNN=5.02  TeV with the ALICE detector at the CERN Large Hadron Collider. The measurements are performed in the central pseudorapidity region |η|<0.8 and for the transverse momentum range 0.2<pT<5  GeV/c. The anisotropic flow is measured using two-particle correlations with a pseudorapidity gap greater than one unit and with the multiparticle cumulant method. Compared to results from Pb-Pb collisions at √sNN=2.76  TeV, the anisotropic flow coefficients v2, v3, and v4 are found to increase by (3.0±0.6)%, (4.3±1.4)%, …

PhysicsRange (particle radiation)Large Hadron Collider010308 nuclear & particles physicsElliptic flowGeneral Physics and Astronomy01 natural sciences7. Clean energyCharged particleNuclear physicsPseudorapidity0103 physical sciencesQuark–gluon plasmaHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsNucleonAnisotropyPhysical Review Letters
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Measuring KS0K± interactions using Pb–Pb collisions at sNN=2.76 TeV

2019

We present the first measurements of femtoscopic correlations between the KS0 and K± particles in pp collisions at s=7 TeV measured by the ALICE experiment. The observed femtoscopic correlations are consistent with final-state interactions proceeding solely via the a0(980) resonance. The extracted kaon source radius and correlation strength parameters for KS0K− are found to be equal within the experimental uncertainties to those for KS0K+ . Results of the present study are compared with those from identical-kaon femtoscopic studies also performed with pp collisions at s=7 TeV by ALICE and with a KS0K± measurement in Pb–Pb collisions at sNN=2.76 TeV. Combined with the Pb–Pb results, our pp a…

Quantum chromodynamicsPhysicsCouplingNuclear and High Energy PhysicsLarge Hadron Collider010308 nuclear & particles physicsRadius01 natural sciencesResonance (particle physics)Particle identificationNuclear physicsDiquarkHadron physics0103 physical sciencesStatistical analysisTetraquark010306 general physicsPhysics Letters B
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Search for weakly decaying Λn‾ and ΛΛ exotic bound states in central Pb–Pb collisions at sNN=2.76 TeV

2016

We present results of a search for two hypothetical strange dibaryon states, i.e. the H-dibaryon and the possible (Lambda n) over bar bound state. The search is performed with the ALICE detector in central (0-10%) Pb-Pb collisions at root S-NN = 2.76 TeV, by invariant mass analysis in the decay modes (Lambda n) over bar (d) over bar pi(+) and H-dibaryon -> Lambda p pi(-). No evidence for these bound states is observed. Upper limits are determined at 99% confidence level for a wide range of lifetimes and for the full range of branching ratios. The results are compared to thermal, coalescence and hybrid UrQMD model expectations, which describe correctly the production of other loosely bound s…

PhysicsNuclear and High Energy PhysicsLarge Hadron Collider010308 nuclear & particles physicsBranching fractionNuclear TheoryBinding energyLambda01 natural sciencesParticle identificationNuclear physics0103 physical sciencesBound stateHigh Energy Physics::ExperimentInvariant massNuclear Experiment010306 general physicsHypertritonPhysics Letters B
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Pseudorapidity and transverse-momentum distributions of charged particles in proton–proton collisions at s=13 TeV

2016

The pseudorapidity (η) and transverse-momentum (pT) distributions of charged particles produced in proton-proton collisions are measured at the centre-of-mass energy s√ = 13 TeV. The pseudorapidity distribution in |η|< 1.8 is reported for inelastic events and for events with at least one charged particle in | η|< 1. The pseudorapidity density of charged particles produced in the pseudorapidity region |η|< 0.5 is 5.31 ± 0.18 and 6.46 ± 0.19 for the two event classes, respectively. The transverse-momentum distribution of charged particles is measured in the range 0.15 < pT < 20 GeV/c and |η|< 0.8 for events with at least one charged particle in |η|< 1. The correlation between transverse momen…

PhysicsNuclear and High Energy PhysicsParticle physicsTime projection chamber010308 nuclear & particles physicsHadronPartonStrangeness01 natural sciences7. Clean energyCharged particleHadronizationNuclear physicsPseudorapidity0103 physical sciencesHigh Energy Physics::ExperimentMultiplicity (chemistry)Nuclear Experiment010306 general physicsPhysics Letters B
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Measurement of electrons from semileptonic heavy-flavor hadron decays inppcollisions ats=2.76  TeV

2015

The pT-differential production cross section of electrons from semileptonic decays of heavy-flavor hadrons has been measured at midrapidity in proton-proton collisions at s=2.76TeV in the transverse momentum range 0.5<pT<12GeV/c with the ALICE detector at the LHC. The analysis was performed using minimum bias events and events triggered by the electromagnetic calorimeter. Predictions from perturbative QCD calculations agree with the data within the theoretical and experimental uncertainties.

Quantum chromodynamicsPhysicsSemileptonic decayNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderPhysics::Instrumentation and Detectors010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyHadronPerturbative QCD7. Clean energy01 natural sciencesNuclear physicsParticle decay0103 physical sciencesQuark–gluon plasmaHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsQCD matterPhysical Review D
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Production of charged pions, kaons and protons at large transverse momenta in pp and Pb–Pb collisions at sNN=2.76 TeV

2014

Transverse momentum spectra of pi(+/-), K-+/- and p((p) over bar) up to p(T) = 20 GeV/c at mid-rapidity in pp, peripheral (60-80%) and central (0-5%) Pb-Pb collisions at v root s(NN) = 2.76 TeV have been measured using the ALICE detector at the Large Hadron Collider. The proton-to-pion and the kaon-to-pionratios both show a distinct peak at p(T) approximate to 3 GeV/c in central Pb-Pb collisions. Below the peak, p(T) 10 GeV/c particle ratios in pp and Pb-Pb collisions are in agreement and the nuclear modification factors for pi(+/-), K-+/- and p((p) over bar) indicate that, within the systematic and statistical uncertainties, the suppression is the same. This suggests that the chemical comp…

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderJet (particle physics)Charged particleSpectral lineBaryonNuclear physicsTransverse planePionHigh Energy Physics::ExperimentNuclear ExperimentBar (unit)Physics Letters B
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J/ψ production as a function of charged particle multiplicity in pp collisions at s =7 TeV

2012

The ALICE Collaboration reports the measurement of the relative J/psi yield as a function of charged particle pseudorapidity density dN(ch)/d eta in pp collisions at root s = 7 TeV at the LHC. J/psi particles are detected for p(t) > 0, in the rapidity interval vertical bar y vertical bar 0. In the highest multiplicity interval with (dN(ch)/d eta)(bin)) = 24.1, corresponding to four times the minimum bias multiplicity density, an enhancement relative to the minimum bias J/psi yield by a factor of about 5 at 2.5 < y <4 (8 at vertical bar y vertical bar < 0.9) is observed. (C) 2012 CERN. Published by Elsevier B.V. All rights reserved.

PhysicsNuclear and High Energy PhysicsAntiparticle010308 nuclear & particles physicsElementary particle01 natural sciences7. Clean energyCharged particleNuclear physicsPseudorapidityAntimatter0103 physical sciencesHigh Energy Physics::ExperimentRapidityMultiplicity (chemistry)Nuclear Experiment010306 general physicsLeptonPhysics Letters B
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Alignment of the ALICE Inner Tracking System with cosmic-ray tracks

2010

ALICE (A Large Ion Collider Experiment) is the LHC (Large Hadron Collider) experiment devoted to investigating the strongly interacting matter created in nucleus-nucleus collisions at the LHC energies. The ALICE ITS, Inner Tracking System, consists of six cylindrical layers of silicon detectors with three different technologies; in the outward direction: two layers of pixel detectors, two layers each of drift, and strip detectors. The number of parameters to be determined in the spatial alignment of the 2198 sensor modules of the ITS is about 13,000. The target alignment precision is well below 10 micron in some cases (pixels). The sources of alignment information include survey measurement…

Physics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsperspectiveHigh Energy PhisicsDetector alignment and calibration methods (lasers sources particle-beams); Particle tracking detectors (Solid-state detectors); Instrumentation; Mathematical Physics01 natural sciences7. Clean energylaw.inventionHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)lawParticle tracking detectors[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Tracking detectors; High Energy Phisics; Heavy Ion PhysicsDetectors and Experimental TechniquesDetector alignment and calibration methodsNuclear ExperimentInstrumentationphysics.ins-detMathematical PhysicsdetectorsPhysicsLarge Hadron ColliderSolenoidal vector fieldPhysicsDetectorInstrumentation and Detectors (physics.ins-det)particle-beams)collisionsParticle tracking detectors (Solid-state detectors) ; Detector alignment and calibration methods (lasers ; sources ; particle-beams)collaboration; collisions; detector alignment and calibration methods (lasers; sources; particle-beams); detectors; particle tracking detectors (solid-state detectors); performance; perspective; quark-gluon plasmaColliding beam accelerators collisions Pb-Pb collisionsParticle tracking detectors (Solid-state detectors); Detector alignment and calibration methods (lasers sources particle-beams); QUARK-GLUON PLASMAperformancesourcesquark-gluon plasmaDetector alignment and calibration methodFOS: Physical sciencesCosmic ray114 Physical sciencesNuclear physicsTracking detectorsOpticsparticle tracking detectors (solid-state detectors)0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsColliderPixel010308 nuclear & particles physicsbusiness.industryhep-exHeavy Ion Physicsdetector alignment and calibration methods (laserscollaborationQuark–gluon plasmaDetector alignment and calibration methods; Particle tracking detectorsALICE (propellant)business
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Light vector meson production in pp collisions at s=7 TeV

2012

The ALICE experiment has measured low-mass dimuon production in pp collisions at root s = 7 TeV in the dimuon rapidity region 2.5 < y < 4. The observed dimuon mass spectrum is described as a superposition of resonance decays (eta, rho, omega, eta', phi) into muons and semi-leptonic decays of charmed mesons. The measured production cross sections for omega and phi are sigma(omega)(1 < p(t) < 5 GeV/c. 2.5 < y < 4) = 5.28 +/- 0.54(stat) +/- 0.49(syst) mb and sigma(phi)(1 < p(t) < 5 GeV/c. 2.5 < y < 4) = 0.940 +/- 0.084(stat) +/- 0.076(syst) mb. The differential cross sections d(2)sigma/dy dp(t) are extracted as a function of p(t) for omega and phi. The ratio between the rho and omega cross sec…

PhysicsParticle physicsNuclear and High Energy PhysicsMuonMeson010308 nuclear & particles physicsPhysicsHadronElementary particle01 natural sciencesOmegaNuclear physicsParticle decayLight vector meson0103 physical sciencesALICE; LHC; CERN; vector meson; pp; 7 TeVHigh Energy Physics::ExperimentRapidityVector mesonNuclear Experiment010306 general physicsPhysics Letters B
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Multi-particle azimuthal correlations in p-Pb and Pb-Pb collisions at the CERN Large Hadron Collider

2014

Measurements of multi-particle azimuthal correlations (cumulants) for charged particles in p-Pb and Pb-Pb collisions are presented. They help address the question of whether there is evidence for global, flow-like, azimuthal correlations in the p-Pb system. Comparisons are made to measurements from the larger Pb-Pb system, where such evidence is established. In particular, the second harmonic two-particle cumulants are found to decrease with multiplicity, characteristic of a dominance of few-particle correlations in p-Pb collisions. However, when a $|\Delta \eta|$ gap is placed to suppress such correlations, the two-particle cumulants begin to rise at high-multiplicity, indicating the prese…

Pb-Pb collisionsazimuthal correlationsPb-Pb and p-Pb collisions at the LHCPpb CollisionsHigh multiplicityppQUARK-GLUON PLASMAALICEp-Pb collisionsRoot-S(Nn)=5.02 Tevcharged particlesPbPbNuclear Experiment (nucl-ex)Nuclear ExperimentPhysicsLarge Hadron Colliderazimuthal correlations; p-Pb collisions; Pb-Pb collisionsFlowPhysicsLong-RangeCharged particle3. Good health:Mathematics and natural scienses: 400::Physics: 430::Nuclear and elementary particle physics: 431 [VDP]AzimuthPRIRODNE ZNANOSTI. Fizika.LHCThird harmonicLHC; ALICE; pp; PbPb; Azimuthal correlationsParticle Physics - ExperimentParticle physicsNuclear and High Energy PhysicsVDP::Matematikk og naturvitenskap: 400::Fysikk: 430::Kjerne- og elementærpartikkelfysikk: 431FOS: Physical sciencesEccentricities[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Nuclear physicsNuclear Physics - ExperimentDependenceCumulantNUCLEUS-NUCLEUS COLLISIONS; QUARK-GLUON PLASMA; ANGULAR-CORRELATIONSTransverse-Momentumta114VDP::Mathematics and natural scienses: 400::Physics: 430::Nuclear and elementary particle physics: 431NUCLEUS-NUCLEUS COLLISIONS:Matematikk og naturvitenskap: 400::Fysikk: 430::Kjerne- og elementærpartikkelfysikk: 431 [VDP]ALICE experimentMultiplicity (mathematics)ANGULAR-CORRELATIONSNATURAL SCIENCES. Physics.Quark–gluon plasma
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Net-charge fluctuations in Pb-Pb collisions at sqrt[sNN]=2.76TeV.

2013

We report the first measurement of the net-charge fluctuations in Pb-Pb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV, measured with the ALICE detector at the CERN Large Hadron Collider. The dynamical fluctuations per unit entropy are observed to decrease when going from peripheral to central collisions. An additional reduction in the amount of fluctuations is seen in comparison to the results from lower energies. We examine the dependence of fluctuations on the pseudo-rapidity interval, which may account for the dilution of fluctuations during the evolution of the system. We find that the ALICE data points are between the theoretically predicted values for a hadron gas and a Quark-Gluon Plasma.…

Particle physicsNuclear TheoryPhysics::Instrumentation and DetectorsHadroncharge fluctuation ; Pb-Pb ; heavy ion ; ALICEGeneral Physics and Astronomy01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsPhysics and Astronomy (all)0103 physical sciencesNuclear Physics - Experiment010306 general physicsNuclear ExperimentNuclear CollisionsNuclear theoryPhysicsLarge Hadron Collider010308 nuclear & particles physicsPhysicsHigh Energy Physics::PhenomenologyDetectorPlasmaHigh Energy Physics - PhenomenologyQuark–gluon plasmaHigh Energy Physics::ExperimentParticle Physics - Experiment
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Spin asymmetry A1d and the spin-dependent structure function g1d of the deuteron at low values of x and Q2

2007

Abstract We present a precise measurement of the deuteron longitudinal spin asymmetry A 1 d and of the deuteron spin-dependent structure function g 1 d at Q 2 1 ( GeV / c ) 2 and 4 × 10 −5 x 2.5 × 10 −2 based on the data collected by the COMPASS experiment at CERN during the years 2002 and 2003. The statistical precision is tenfold better than that of the previous measurement in this region. The measured A 1 d and g 1 d are found to be consistent with zero in the whole range of x.

PhysicsNuclear and High Energy PhysicsRange (particle radiation)Large Hadron Collider010308 nuclear & particles physicsmedia_common.quotation_subjectStructure functionZero (complex analysis)01 natural sciencesAsymmetryNuclear physicsDeuterium0103 physical sciencesCOMPASS experiment010306 general physicsSpin-½media_commonPhysics Letters B
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Anisotropic flow of charged hadrons, pions and (anti-)protons measured at high transverse momentum in Pb–Pb collisions at sNN=2.76 TeV

2013

The elliptic, v(2), triangular, v(3), and quadrangular, v(4), azimuthal anisotropic flow coefficients are measured for unidentified charged particles, pions, and (anti-)protons in Pb-Pb collisions at root S-NN = 2.76 TeV with the ALICE detector at the Large Hadron Collider. Results obtained with the event plane and four-particle cumulant methods are reported for the pseudo-rapidity range vertical bar eta vertical bar 8 GeV/c. The small p(T) dependence of the difference between elliptic flow results obtained from the event plane and four-particle cumulant methods suggests a common origin of flow fluctuations up to p(T) = 8 GeV/c. The magnitude of the (anti-)proton elliptic and triangular flo…

PhysicsNuclear and High Energy PhysicsParticle physicsMesonProton010308 nuclear & particles physicsElliptic flowHadron01 natural sciencesCharged particleNuclear physicsBaryonPionAntiproton0103 physical sciencesHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsPhysics Letters B
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Reconnection nanojets in the solar corona

2020

P.A. acknowledges STFC support from grant numbers ST/R004285/2 and ST/T000384/1 and support from the International Space Science Institute, Bern, Switzerland to the International Teams on ‘Implications for coronal heating and magnetic fields from coronal rain observations and modeling’ and ‘Observed Multi-Scale Variability of Coronal Loops as a Probe of Coronal Heating’. This project has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement no. 647214). P.T. was also supported by contracts 8100002705 and SP02H1701R from Lockheed-Martin to the Smithsonian Astrophysical Observatory (SAO), and NASA c…

Physics010504 meteorology & atmospheric sciencesMagnetic energyDASAstronomy and AstrophysicsMagnetic reconnectionAstrophysics01 natural sciencesNanoflaresMagnetic fieldQC PhysicsPhysics::Space Physics0103 physical sciencesCoronal heatingQB AstronomyAstrophysics::Solar and Stellar Astrophysicssolar corona coronal heating magnetic reconnection010303 astronomy & astrophysicsQCQB0105 earth and related environmental sciences
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Two-pion Bose-Einstein correlations inppcollisions ats=900  GeV

2010

We report on the measurement of two-pion correlation functions from pp collisions at root s = 900 GeV performed by the ALICE experiment at the Large Hadron Collider. Our analysis shows an increase of the Hanbury Brown-Twiss radius with increasing event multiplicity, in line with other measurements done in particle- and nuclear collisions. Conversely, the strong decrease of the radius with increasing transverse momentum, as observed at the Relativistic Heavy Ion Collider and at Tevatron, is not manifest in our data.

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderMeson010308 nuclear & particles physicsNuclear TheoryHadronTevatronParticle acceleratorBose–Einstein correlations01 natural scienceslaw.inventionNuclear physicsPionlaw0103 physical sciencesHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsRelativistic Heavy Ion ColliderPhysical Review D
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In Situ Generation of Transverse Magnetohydrodynamic Waves from Colliding Flows in the Solar Corona

2018

This research has received funding from the UK Science and Technology Facilities Council (Consolidated Grant ST/K000950/1) and the European Union Horizon 2020 Research and Innovation Programme (grant agreement No. 647214). V.M.N. acknowledges the support of the BK21 plus program through the National Research Foundation funded by the Ministry of Education of Korea. Transverse magnetohydrodynamic (MHD) waves permeate the solar atmosphere and are a candidate for coronal heating. However, the origin of these waves is still unclear. In this Letter, we analyze coordinated observations from Hinode/Solar Optical Telescope (SOT) and Interface Region Imaging Spectrograph (IRIS) of a prominence/corona…

Magnetohydrodynamics (MHD)010504 meteorology & atmospheric sciencesF300NDASEnergy fluxF500magnetohydrodynamics (MHD)01 natural sciencesSolar prominenceSun: activity0103 physical sciencesQB AstronomyAstrophysics::Solar and Stellar AstrophysicsCoronal rainwavesactivity [Sun]Magnetohydrodynamic drive010303 astronomy & astrophysicsQCQB0105 earth and related environmental sciencesPhysicsSun: coronaoscillations [Sun]Sun:oscillationsAstronomy and AstrophysicsPlasmaSun: filaments prominencesMagnetic fieldComputational physicsTransverse planeQC PhysicsSpace and Planetary SciencePhysics::Space PhysicsWavesfilaments prominences [Sun]MagnetohydrodynamicsThe Astrophysical Journal
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Charged kaon femtoscopic correlations inppcollisions ats=7  TeV

2013

Correlations of two charged identical kaons (KchKch) are measured in pp collisions at root s = 7 TeV by the ALICE experiment at the Large Hadron Collider (LHC). One-dimensional (KKch)-K-ch correlation functions are constructed in three multiplicity and four transverse momentum ranges. The (KKch)-K-ch femtoscopic source parameters R and lambda are extracted. The (KKch)-K-ch correlations show a slight increase of femtoscopic radii with increasing multiplicity and a slight decrease of radii with increasing transverse momentum. These trends are similar to the ones observed for pi pi and K-s(0) K-s(0) correlations in pp and heavy-ion collisions. However at high multiplicities, there is an indica…

Nuclear and High Energy PhysicsParticle physicsCOLISÕES DE ÍONS PESADOS RELATIVÍSTICOSLambda01 natural sciencesDECAYSNuclear physicsINTERFEROMETRYPion0103 physical sciences010306 general physicsNuclear ExperimentPhysicsBOSE-EINSTEIN CORRELATIONS; COULOMB CORRECTIONS; INTERFEROMETRY; INTERFERENCE; DECAYS; Z(0)COULOMB CORRECTIONSINTERFERENCELarge Hadron Collider010308 nuclear & particles physicsPhysicsMultiplicity (mathematics)Bose–Einstein correlationsZ(0)BOSE-EINSTEIN CORRELATIONSTransverse momentumHigh Energy Physics::Experimentkaon ; correlation ; ALICEPhysical Review D
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Forward-central two-particle correlations in p–Pb collisions at sNN=5.02 TeV

2016

Two-particle angular correlations between trigger particles in the forward pseudorapidity range (2.5 < |η| < 4.0) and associated particles in the cen

Physicscongenital hereditary and neonatal diseases and abnormalitiesNuclear and High Energy PhysicsParticle physicsTime projection chamber010308 nuclear & particles physicsAtlas detector01 natural sciencesCharged particleNuclear physicsMuon spectrometerPseudorapidity0103 physical sciencesTransverse momentumRapidityMultiplicity (chemistry)010306 general physicsPhysics Letters B
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Ds+ meson production at central rapidity in proton–proton collisions at s=7 TeV

2012

The pt-differential inclusive production cross section of the prompt charm-strange meson D_s in the rapidity range |y| phi pi, with phi -> KK, and its charge conjugate, about 480 D_s mesons were counted, after selection cuts, in the transverse momentum range 2

Quantum chromodynamicsPhysicsNuclear and High Energy PhysicsParticle physicsAntiparticleLarge Hadron ColliderMeson010308 nuclear & particles physicsHigh Energy Physics::LatticeNuclear TheoryHigh Energy Physics::PhenomenologyHadronElementary particle7. Clean energy01 natural sciencesNuclear physics0103 physical sciencesHigh Energy Physics::ExperimentRapidityNuclear Experiment010306 general physicsLeptonPhysics Letters B
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Charged-Particle Multiplicity Density at Midrapidity in Central Pb-Pb Collisions atsNN=2.76  TeV

2010

The first measurement of the charged-particle multiplicity density at midrapidity in Pb-Pb collisions at a center-of-mass energy per nucleon pair root s(NN) = 2.76 TeV is presented. For an event sample corresponding to the most central 5% of the hadronic cross section, the pseudorapidity density of primary charged particles at midrapidity is 1584 +/- 4(stat) +/- 76(syst), which corresponds to 8.3 +/- 0.4(syst) per participating nucleon pair. This represents an increase of about a factor 1.9 relative to pp collisions at similar collision energies, and about a factor 2.2 to central Au-Au collisions at root s(NN) = 0.2 TeV. This measurement provides the first experimental constraint for models…

PhysicsParticle physicsLarge Hadron Collider010308 nuclear & particles physicsNuclear TheoryHadronGeneral Physics and AstronomyElementary particle01 natural sciencesCharged particleBaryonNuclear physicsPseudorapidity0103 physical sciencesHigh Energy Physics::ExperimentRapidityNuclear Experiment010306 general physicsNucleonPhysical Review Letters
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Linear and non-linear flow mode in Pb–Pb collisions at sNN=2.76 TeV

2017

The second and the third order anisotropic flow, V2 and V3, are mostly determined by the corresponding initial spatial anisotropy coefficients, e2 and e3, in the initial density distribution. In addition to their dependence on the same order initial anisotropy coefficient, higher order anisotropic flow, Vn (n > 3), can also have a significant contribution from lower order initial anisotropy coefficients, which leads to mode-coupling effects. In this Letter we investigate the linear and non-linear modes in higher order anisotropic flow Vn for n = 4, 5, 6 with the ALICE detector at the Large Hadron Collider. The measurements are done for particles in the pseudorapidity range |η| < 0.8 and the…

PhysicsNuclear and High Energy Physics010308 nuclear & particles physicsHadron01 natural sciencesNuclear physicsThird orderViscosityFlow (mathematics)Pseudorapidity0103 physical sciencesRapidityBoundary value problem010306 general physicsAnisotropyPhysics Letters B
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Magnetohydrodynamic study on the effect of the gravity stratification on flux rope ejections

2013

Context. Coronal mass ejections (CMEs) are the most violent phenomenon found on the Sun. One model that explains their occurrence is the flux rope ejection model. A magnetic flux rope is ejected from the solar corona and reaches the interplanetary space where it interacts with the pre-existing magnetic fields and plasma. Both gravity and the stratification of the corona affect the early evolution of the flux rope. Aims. Our aim is to study the role of gravitational stratification on the propagation of CMEs. In particular, we assess how it influences the speed and shape of CMEs and under what conditions the flux rope ejection becomes a CME or when it is quenched. Methods. We ran a set of MHD…

Sun: coronal mass ejections (CMEs) – Sun: corona – magnetohydrodynamics (MHD)PhysicsSpace and Planetary SciencePhysics::Space PhysicsAstrophysics::Solar and Stellar AstrophysicsStratification (water)Astronomy and AstrophysicsAstrophysics::Earth and Planetary AstrophysicsMagnetohydrodynamic driveMechanicsMagnetohydrodynamicsSettore FIS/06 - Fisica Per Il Sistema Terra E Il Mezzo CircumterrestreRopeProceedings of the International Astronomical Union
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The Polarised Valence Quark Distribution from semi-inclusive DIS

2007

The semi-inclusive difference asymmetry A^{h^{+}-h^{-}} for hadrons of opposite charge has been measured by the COMPASS experiment at CERN. The data were collected in the years 2002-2004 using a 160 GeV polarised muon beam scattered off a large polarised ^6LiD target and cover the range 0.006 &lt; x &lt; 0.7 and 1 &lt; Q^2 &lt; 100 (GeV/c)^2. In leading order QCD (LO) the asymmetry A_d^{h^{+}-h^{-}} measures the valence quark polarisation and provides an evaluation of the first moment of Delta u_v + Delta d_v which is found to be equal to 0.40 +- 0.07 (stat.) +- 0.05 (syst.) over the measured range of x at Q^2 = 10 (GeV/c)^2. When combined with the first moment of g_1^d previously measured …

QuarkNuclear and High Energy PhysicsParticle physicsmagnetic spectrometer: COMPASSStructure functionsmedia_common.quotation_subjectHadronpolarization: longitudinalFOS: Physical sciencespolarized targetcross section: ratioDeep inelastic scattering; Structure functionsmuon deuteron: deep inelastic scattering01 natural sciencesAsymmetryx-dependenceHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)charged particle: multiple productionnegative particle: electroproductionExperiment-HEP13.88.+e0103 physical sciencesstructure function: moment010306 general physicsNuclear Experimentmedia_commonPhysicsQuantum chromodynamicsMuonValence (chemistry)010308 nuclear & particles physicsHigh Energy Physics::Phenomenologycross section: differenceCERN SPSDeep inelastic scatteringpositive particle: electroproductionDeuteriumquark: valenceHigh Energy Physics::Experimentmuon: polarized beamquark: polarization140-180 GeVspin: asymmetry13.60.HbDeep inelastic scatteringParticle Physics - Experimentexperimental results
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Collins and Sivers asymmetries for pions and kaons in muon-deuteron DIS

2008

The measurements of the Collins and Sivers asymmetries of identified hadrons produced in deep-inelastic scattering of 160 GeV/c muons on a transversely polarised 6LiD target at COMPASS are presented. The results for charged pions and charged and neutral kaons correspond to all data available, which were collected from 2002 to 2004. For all final state particles both the Collins and Sivers asymmetries turn out to be small, compatible with zero within the statistical errors, in line with the previously published results for not identified charged hadrons, and with the expected cancellation between the u- and d-quark contributions.

QuarkNuclear and High Energy PhysicsParticle physicsSivers asymmetryHadronNuclear TheoryFOS: Physical sciences01 natural sciencesCOMPASSHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)PionIdentifiedCompass0103 physical sciencesTransverse spin effects; Deuteron; Collins asymmetry; Sivers asymmetry; COMPASSDeuteronTransverse spin effect010306 general physicsNuclear ExperimentPhysicsMuon010308 nuclear & particles physicsScatteringHigh Energy Physics::PhenomenologyTransverse single-spin asymmetryTransverse spin effectsCollins asymmetryhadronsDeuteriumTransversityHigh Energy Physics::Experiment
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Azimuthally Differential Pion Femtoscopy in Pb-Pb Collisions at sNN=2.76  TeV

2017

We present the first azimuthally differential measurements of the pion source size relative to the second harmonic event plane in Pb-Pb collisions at a center-of-mass energy per nucleon-nucleon pair of √sNN = 2.76 TeV. The measurements have been performed in the centrality range 0%-50% and for pion pair transverse momenta 0.2 < kT < 0.7 GeV/c. We find that the Rside and Rout radii, which characterize the pion source size in the directions perpendicular and parallel to the pion transverse momentum, oscillate out of phase, similar to what was observed at the Relativistic Heavy Ion Collider. The final-state source eccentricity, estimated via Rside oscillations, is found to be significantly sma…

PhysicsParticle physicsLarge Hadron Collider010308 nuclear & particles physicsOscillationmedia_common.quotation_subjectNuclear TheoryHadronGeneral Physics and Astronomy01 natural sciencesNuclear physicsTransverse planePion0103 physical sciencesRapidityEccentricity (behavior)Nuclear Experiment010306 general physicsRelativistic Heavy Ion Collidermedia_commonPhysical Review Letters
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Midrapidity Antiproton-to-Proton Ratio inppCollisons ats=0.9and 7 TeV Measured by the ALICE Experiment

2010

The ratio of the yields of antiprotons to protons in pp collisions has been measured by the ALICE experiment at root s = 0.9 and 7 TeV during the initial running periods of the Large Hadron Collider. The measurement covers the transverse momentum interval 0.45 < p(t) < 1.05 GeV/c and rapidity vertical bar y vertical bar < 0.5. The ratio is measured to be R-vertical bar y vertical bar<0.5 = 0.957 +/- 0.006(stat) +/- 0.0014(syst) at 0.9 Tev and R-vertical bar y vertical bar<0.5 = 0.991 +/- 0.005 +/- 0.014(syst) at 7 TeV and it is independent of both rapidity and transverse momentum. The results are consistent with the conventional model of baryon-number transport and set stringent limits on a…

PhysicsParticle physicsLarge Hadron ColliderProton010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyHadronGeneral Physics and Astronomy01 natural sciences7. Clean energyParticle identificationBaryonNuclear physicsAntiproton0103 physical sciencesHigh Energy Physics::ExperimentRapidityNuclear Experiment010306 general physicsBar (unit)Physical Review Letters
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Simulating AIA observations of a flux rope ejection

2014

D.H.M. would like to thank STFC, the Leverhulme Trust and the European Commission’s Seventh Framework Programme (FP7/2007-2013) for their financial support. P.P. would like to thank the European Commission’s Seventh Framework Programme (FP7/2007-2013) under grant agreement SWIFF (project 263340, http://www.swiff.eu) and STFC for financial support. These results were obtained in the framework of the projects GOA/2009-009 (KU Leuven), G.0729.11 (FWO-Vlaanderen) and C 90347 (ESA Prodex 9). The research leading to these results has also received funding from the European Commission’s Seventh Framework Programme (FP7/2007-2013) under the grant agreements SOLSPANET (project No. 269299, http:// ww…

Magnetohydrodynamics (MHD)corona [Sun]Sun: coronal mass ejections (CMEs)FOS: Physical sciencesAstrophysicsmagnetohydrodynamics (MHD)7. Clean energyProminencesObservatoryRadiative transferQB AstronomyAstrophysics::Solar and Stellar AstrophysicsQA MathematicsQASun: magnetic fieldsSolar and Stellar Astrophysics (astro-ph.SR)QBPhysicsUV radiation [Sun]Line-of-sightSun: coronaAstronomy and AstrophysicsPlasmaSun: UV radiationCoronacoronal mass ejections (CMEs) [Sun]Magnetic fluxSun: filamentsAstrophysics - Solar and Stellar Astrophysicsmagnetic fields [Sun]13. Climate actionSpace and Planetary ScienceExtreme ultravioletPhysics::Space Physicsfilaments prominences [Sun]Rope
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Elliptic Flow of Charged Particles in Pb-Pb Collisions atsNN=2.76  TeV

2010

We report the first measurement of charged particle elliptic flow in Pb-Pb collisions at root s(NN) p = 2.76 TeV with the ALICE detector at the CERN Large Hadron Collider. The measurement is performed in the central pseudorapidity region (vertical bar eta vertical bar < 0.8) and transverse momentum range 0.2 < p(t) < 5.0 GeV/c. The elliptic flow signal v(2), measured using the 4-particle correlation method, averaged over transverse momentum and pseudorapidity is 0.087 +/- 0.002(stat) +/- 0.003(syst) in the 40%-50% centrality class. The differential elliptic flow v(2)(p(t)) reaches a maximum of 0.2 near p(t) = 3 GeV/c. Compared to RHIC Au-Au collisions at root s(NN) = 200 GeV, the elliptic f…

PhysicsRange (particle radiation)Particle physicsLarge Hadron Collider010308 nuclear & particles physicsHadronElliptic flowGeneral Physics and Astronomy01 natural sciencesCharged particleNuclear physicsPseudorapidity0103 physical sciencesQuark–gluon plasmaHigh Energy Physics::ExperimentRapidityNuclear Experiment010306 general physicsPhysical Review Letters
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Jet-like correlations with neutral pion triggers in pp and central Pb–Pb collisions at 2.76 TeV

2016

Physics letters / B B763, 238 - 250 (2016). doi:10.1016/j.physletb.2016.10.048

heavy ion: scattering:Kjerne- og elementærpartikkelfysikk: 431 [VDP]ROOT-S(NN)=200 GEVQUARK-GLUON PLASMA; TRANSVERSE-MOMENTUM DEPENDENCE; LEAD-LEAD COLLISIONS; ROOT-S(NN)=2.76 TEV; ROOT-S-NN=2.76 TEV; ATLAS DETECTOR; SUPPRESSION; COLLABORATION; PERSPECTIVE; HADRONSHadronATLAS DETECTORCOLLABORATION01 natural sciencespi: triggerfragmentation functionParticle identificationHigh Energy Physics - ExperimentQUARK-GLUON PLASMAHADRON CORRELATIONSHigh Energy Physics - Experiment (hep-ex)ALICEp-Pb collisionsANISOTROPIC FLOWLEAD-LEADscattering [p p][PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear Experiment (nucl-ex)ROOT-S(NN)=2.76 TEVPERSPECTIVENuclear ExperimentMonte CarloNuclear ExperimentPhysicsTime projection chamberHADRONSPerturbative QCDneutral pion ; lead-lead ; correlationsuppressioncharged particlelcsh:QC1-999Charged particleTRANSVERSE-MOMENTUM DEPENDENCE CENTRAL AU+AU COLLISIONS LEAD-LEAD COLLISIONS PLUS AU COLLISIONS QUARK-GLUON PLASMA HADRON CORRELATIONS ROOT-S-NN=2.76 TEV ROOT-S(NN)=200 GEV CHARGED-PARTICLES ANISOTROPIC FLOW.:Mathematics and natural scienses: 400::Physics: 430::Nuclear and elementary particle physics: 431 [VDP]PRIRODNE ZNANOSTI. Fizika.:Nuclear and elementary particle physics: 431 [VDP]CHARGED-PARTICLESflowLEAD-LEAD COLLISIONSperturbation theory [quantum chromodynamics]correlation: two-particleCOLLISIONSParticle physicsp p: scatteringPLUS AU COLLISIONSNuclear and High Energy PhysicseducationVDP::Matematikk og naturvitenskap: 400::Fysikk: 430::Kjerne- og elementærpartikkelfysikk: 431FOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]transverse momentumtriggerstrigger [pi]114 Physical sciencesQUARK-GLUON PLASMA; TRANSVERSE-MOMENTUM DEPENDENCE; LEAD-LEAD; COLLISIONS; ROOT-S(NN)=2.76 TEV; ROOT-S-NN=2.76 TEV; ATLAS DETECTOR; SUPPRESSION; COLLABORATION; PERSPECTIVE; HADRONS530ROOT-S-NN=2.76 TEVNuclear physicsPionTRANSVERSE-MOMENTUM DEPENDENCEscattering [heavy ion]0103 physical sciencesFragmentation functionddc:530Nuclear Physics - Experimentquantum chromodynamics: perturbation theory010306 general physicscapturetwo-particle correlationstwo-particle [correlation]enhancementSUPPRESSIONneutral pionVDP::Mathematics and natural scienses: 400::Physics: 430::Nuclear and elementary particle physics: 431ta114CENTRAL AU+AU COLLISIONS010308 nuclear & particles physicsbackground:Matematikk og naturvitenskap: 400::Fysikk: 430::Kjerne- og elementærpartikkelfysikk: 431 [VDP]NATURAL SCIENCES. Physics.lead-leadcorrelationQuark–gluon plasmaproton-proton collisionsHigh Energy Physics::Experimenthadronlcsh:Physics
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Production of muons from heavy-flavour hadron decays in p–Pb collisions at sNN=5.02 TeV

2017

Abstract The production of muons from heavy-flavour hadron decays in p–Pb collisions at s NN = 5.02 TeV was studied for 2 p T 16 GeV/c with the ALICE detector at the CERN LHC. The measurement was performed at forward (p-going direction) and backward (Pb-going direction) rapidity, in the ranges of rapidity in the centre-of-mass system (cms) 2.03 y cms 3.53 and − 4.46 y cms − 2.96 , respectively. The production cross sections and nuclear modification factors are presented as a function of transverse momentum ( p T ). At forward rapidity, the nuclear modification factor is compatible with unity while at backward rapidity, in the interval 2.5 p T 3.5 GeV/c, it is above unity by more than 2σ. Th…

PhysicsNuclear and High Energy PhysicsParticle physicsMuonLarge Hadron ColliderPhysics::Instrumentation and Detectors010308 nuclear & particles physicsHadronFlavourNuclear matter7. Clean energy01 natural sciencesNuclear physics0103 physical sciencesQuark–gluon plasmaHigh Energy Physics::ExperimentProduction (computer science)RapidityNuclear Experiment010306 general physicsPhysics Letters B
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Neutron emission from electromagnetic dissociation of Pb nuclei at $\sqrt {s_{NN}} = 2.76$ TeV measured with the ALICE ZDC

2014

The ALICE Zero Degree Calorimeter system (ZDC) is composed of two identical sets of calorimeters, placed at opposite sides with respect to the interaction point, 114 meters away from it, complemented by two small forward electromagnetic calorimeters (ZEM). Each set of detectors consists of a neutron (ZN) and a proton (ZP) ZDC. They are placed at zero degrees with respect to the LHC axis and allow to detect particles emitted close to beam direction, in particular neutrons and protons emerging from hadronic heavy-ion collisions (spectator nucleons) and those emitted from electromagnetic processes. For neutrons emitted by these two processes, the ZN calorimeters have nearly 100% acceptance. Du…

PhysicsParticle physicsLarge Hadron ColliderInteraction pointProtonNeutron emissionPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaPhysicsQC1-999HadronNuclear Theory7. Clean energyCalorimeterNuclear physicsPhysics and Astronomy (all)NeutronHigh Energy Physics::ExperimentNuclear Physics - ExperimentNucleonNuclear Experiment
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Centrality dependence of the pseudorapidity density distribution for charged particles in Pb–Pb collisions at sNN=2.76 TeV

2017

We present the charged-particle pseudorapidity density in Pb-Pb collisions at $\sqrt{s_{\mathrm{NN}}}=5.02\,\mathrm{Te\kern-.25exV}$ in centrality classes measured by ALICE. The measurement covers a wide pseudorapidity range from $-3.5$ to $5$, which is sufficient for reliable estimates of the total number of charged particles produced in the collisions. For the most central (0-5%) collisions we find $21\,400\pm 1\,300$ while for the most peripheral (80-90%) we find $230\pm 38$. This corresponds to an increase of $(27\pm4)\%$ over the results at $\sqrt{s_{\mathrm{NN}}}=2.76\,\mathrm{Te\kern-.25exV}$ previously reported by ALICE. The energy dependence of the total number of charged particles…

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron Collider010308 nuclear & particles physicsExtrapolation01 natural sciencesCharged particleColor-glass condensateNuclear physicsPseudorapidity0103 physical sciencesQuark–gluon plasmaRapidityImpact parameterCentralityNuclear Experiment010306 general physicsNucleonGlauberScalingPhysics Letters B
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Multiplicity dependence of jet-like two-particle correlation structures in p–Pb collisions at sNN=5.02 TeV

2015

Two-particle angular correlations between unidentified charged trigger and associated particles are measured by the ALICE detector in p-Pb collisions at a nucleon-nucleon centre-of-mass energy of 5.02 TeV. The transverse-momentum range 0.7<pT,assoc<pT,trig<5.0 GeV/c is examined, to include correlations induced by jets originating from low momentum-transfer scatterings (minijets). The correlations expressed as associated yield per trigger particle are obtained in the pseudorapidity range |η|<0.9. The near-side long-range pseudorapidity correlations observed in high-multiplicity p-Pb collisions are subtracted from both near-side short-range and away-side correlations in order to remove the no…

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron Collider010308 nuclear & particles physicsScatteringBinary number01 natural sciencesUncorrelatedNuclear physicsCorrelationPseudorapidity0103 physical sciencesHigh Energy Physics::ExperimentMultiplicity (chemistry)Nuclear Experiment010306 general physicsGlauberPhysics Letters B
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Tracing the ICME plasma with a MHD simulation

2021

The determination of the chemical composition of interplanetary coronal mass ejection (ICME) plasma is an open issue. More specifically, it is not yet fully understood how remote sensing observations of the solar corona plasma during solar disturbances evolve into plasma properties measured in situ away from the Sun. The ambient conditions of the background interplanetary plasma are important for space weather because they influence the evolutions, arrival times, and geo-effectiveness of the disturbances. The Reverse In situ and MHD APproach (RIMAP) is a technique to reconstruct the heliosphere on the ecliptic plane (including the magnetic Parker spiral) directly from in situ measurements a…

Sun: coronal mass ejections (CMEs)FOS: Physical sciencesInterplanetary mediumAstrophysicsSpace weathermagnetohydrodynamics (MHD)Physics - Space PhysicsPhysics::Plasma PhysicsAstrophysics::Solar and Stellar AstrophysicsSun: abundancesSolar and Stellar Astrophysics (astro-ph.SR)PhysicsAstronomy and AstrophysicsPlasmasolar-terrestrial relationsSpace Physics (physics.space-ph)Physics - Plasma PhysicsComputational physicsPlasma Physics (physics.plasm-ph)Solar windAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsHeliospheric current sheetMagnetohydrodynamicsInterplanetary spaceflightHeliosphere
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MHD simulations of the in situ generation of kink and sausage waves in the solar corona by collision of dense plasma clumps

2019

Funding: This research has received funding from the UK Science and Technology Facilities Council (Consolidated Grant ST/K000950/1) and the European Union Horizon 2020 research and innovation programme (grant agreement No. 647214). P.A. acknowledges funding from his STFC Ernest Rutherford Fellowship (No. ST/R004285/1). This research was supported by the Research Council of Norway through its Centres of Excellence scheme, project number 262622. Context. Magnetohydrodynamic (MHD) waves are ubiquitous in the solar corona where the highly structured magnetic fields provide efficient wave guides for their propagation. While MHD waves have been observed originating from lower layers of the solar …

Magnetohydrodynamics (MHD)010504 meteorology & atmospheric sciencescorona [Sun]F300NDASFOS: Physical sciencesContext (language use)AstrophysicsF500Parameter space01 natural sciences0103 physical sciencesQB AstronomyAstrophysics::Solar and Stellar AstrophysicsMagnetohydrodynamic drivehelioseismology [Sun]Sun: oscillations010303 astronomy & astrophysicsSun: magnetic fieldsQCSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesQBSun: helioseismologyPhysicsSun: coronaComputer Science::Information Retrievaloscillations [Sun]Astronomy and AstrophysicsMechanicsPlasmaMagnetic fieldWavelengthAmplitudeQC Physicsmagnetic fields [Sun]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsMagnetohydrodynamicsAstronomy & Astrophysics
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Chromospheric evaporation and phase mixing of Alfvén waves in coronal loops

2020

Phase mixing of Alfv\'en waves has been studied extensively as a possible coronal heating mechanism but without the full thermodynamic consequences considered self-consistently. It has been argued that in some cases, the thermodynamic feedback of the heating could substantially affect the transverse density gradient and even inhibit the phase mixing process. In this paper, we use MHD simulations with the appropriate thermodynamical terms included to quantify the evaporation following heating by phase mixing of Alfv\'en waves in a coronal loop and the effect of this evaporation on the transverse density profile. The numerical simulations were performed using the Lare2D code. We set up a 2D l…

Sun: generalatmosphere [Sun]Magnetohydrodynamics (MHD)corona [Sun]010504 meteorology & atmospheric sciencesDensity gradientThermodynamic equilibriumT-NDASEvaporationAstrophysics01 natural sciencesAlfvén wave0103 physical sciencesgeneral [Sun]QB AstronomyAstrophysics::Solar and Stellar AstrophysicsSun: oscillations010303 astronomy & astrophysicsQCQB0105 earth and related environmental sciencesPhysicsSun: coronaoscillations [Sun]Astronomy and AstrophysicsMechanicsCoronal loopDissipationTransverse planeQC PhysicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsWavesMagnetohydrodynamicsBDCSun: atmosphere
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The Deuteron Spin-dependent Structure Function g1(d) and its First Moment

2007

We present a measurement of the deuteron spin-dependent structure function g1d based on the data collected by the COMPASS experiment at CERN during the years 2002-2004. The data provide an accurate evaluation for Gamma_1^d, the first moment of g1d(x), and for the matrix element of the singlet axial current, a0. The results of QCD fits in the next to leading order (NLO) on all g1 deep inelastic scattering data are also presented. They provide two solutions with the gluon spin distribution function Delta G positive or negative, which describe the data equally well. In both cases, at Q^2 = 3 (GeV/c)^2 the first moment of Delta G is found to be of the order of 0.2 - 0.3 in absolute value.

Nuclear and High Energy PhysicsParticle physicsg(1)FOS: Physical sciencesAbsolute valuespinspin structure function g101 natural sciencesCOMPASSHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)polarised deep inelastic scatteringdeep inelastic scatteringstructure function0103 physical sciencesCOMPASS experimentA(1)polarised deep inelastic scattering; COMPASS; spin structure function g1; QCD analysisSinglet state010306 general physicsSpin-½Quantum chromodynamicsPhysics010308 nuclear & particles physicsDeep inelastic scatteringGluonQCD analysisDistribution functionHigh Energy Physics::ExperimentParticle Physics - Experiment
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Multi-strange baryon production in p Pb collisions at sNN=5.02 TeV

2016

The multi-strange baryon yields in Pb--Pb collisions have been shown to exhibit an enhancement relative to pp reactions. In this work, $\Xi$ and $\Omega$ production rates have been measured with the ALICE experiment as a function of transverse momentum, ${p_{\rm T}}$, in p-Pb collisions at a centre-of-mass energy of ${\sqrt{s_{\rm NN}}}$ = 5.02 TeV. The results cover the kinematic ranges 0.6 GeV/$c<{p_{\rm T}} <$7.2 GeV/$c$ and 0.8 GeV/$c<{p_{\rm T}}<$ 5 GeV/$c$, for $\Xi$ and $\Omega$ respectively, in the common rapidity interval -0.5 $<{y_{\rm CMS}}<$ 0. Multi-strange baryons have been identified by reconstructing their weak decays into charged particles. The ${p_{\rm T}}$ spectra are ana…

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsHadronHyperonStrangeness7. Clean energy01 natural sciencesCharged particleNuclear physicsBaryonPion0103 physical sciencesQuark–gluon plasmaRapidityNuclear Experiment010306 general physicsPhysics Letters B
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Modelling of asymmetric nanojets in coronal loops

2021

Context. Observations of reconnection jets in the solar corona are emerging as a possible diagnostic for studying highly elusive coronal heating. Such jets, and in particular those termed nanojets, can be observed in coronal loops and have been linked to nanoflares. However, while models successfully describe the bilateral post-reconnection magnetic slingshot effect that leads to the jets, observations reveal that nanojets are unidirectional or highly asymmetric, with only the jet travelling inward with respect to the coronal loop’s curvature being clearly observed. Aims. The aim of this work is to address the role of the curvature of the coronal loop in the generation and evolution of asym…

F300media_common.quotation_subjectFOS: Physical sciencesAstrophysicsF500magnetic fieldsCurvaturemagnetohydrodynamics (MHD)AsymmetryAstrophysics::Solar and Stellar AstrophysicsMagnetohydrodynamic driveSolar and Stellar Astrophysics (astro-ph.SR)media_commonPhysicsJet (fluid)SunAstronomy and AstrophysicsMechanicsCoronal loopNanoflaresMagnetic fieldAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceatmospherePhysics::Space PhysicsMagnetohydrodynamicscoronaSettore FIS/06 - Fisica Per Il Sistema Terra E Il Mezzo Circumterrestre
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A new measurement of the Collins and Sivers asymmetries on a transversely polarised deuteron target

2007

New high precision measurements of the Collins and Sivers asymmetries of charged hadrons produced in deep-inelastic scattering of muons on a transversely polarised 6LiD target are presented. The data were taken in 2003 and 2004 with the COMPASS spectrometer using the muon beam of the CERN SPS at 160 GeV/c. Both the Collins and Sivers asymmetries turn out to be compatible with zero, within the present statistical errors, which are more than a factor of 2 smaller than those of the published COMPASS results from the 2002 data. The final results from the 2002, 2003 and 2004 runs are compared with naive expectations and with existing model calculations.

QuarkdeuteronNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSivers asymmetryHadrontransversity and Sivers functionFOS: Physical sciencesCOMPASS01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)nucleon structure; transverse spin and transverse momentum; transversity and Sivers functions; deuteron; COMPASS experimentCompass0103 physical sciencesCOMPASS experimentCollins010306 general physicsNuclear ExperimentCOMPASS experimenttransversityPhysicsLarge Hadron ColliderMuonSpectrometer010308 nuclear & particles physicsScatteringtransversity and Sivers functionsnucleon structureHigh Energy Physics::Experimenttransverse spin and transverse momentumasymmetryParticle Physics - Experimenttransverse single-spin asymmetry
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Origin and Ion Charge State Evolution of Solar Wind Transients during 4 – 7 August 2011

2016

We present study of the complex event consisting of several solar wind transients detected by Advanced Composition Explorer (ACE) on 4 -- 7 August 2011, that caused a geomagnetic storm with Dst$=-$110 nT. The supposed coronal sources -- three flares and coronal mass ejections (CMEs) occurred on 2 -- 4 August 2011 in the active region (AR) 11261. To investigate the solar origin and formation of these transients we studied kinematic and thermodynamic properties of the expanding coronal structures using the Solar Dynamics Observatory/Atmospheric Imaging Assembly (SDO/AIA) EUV images and the differential emission measure (DEM) diagnostics. The Helioseismic and Magnetic Imager (HMI) magnetic fie…

010504 meteorology & atmospheric sciencesMHDSolar windAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxAstrophysics01 natural sciencesPhysics - Space PhysicsModelsIonization0103 physical sciencesCoronal mass ejectionQB AstronomyAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsQCQB0105 earth and related environmental sciencesGeomagnetic stormPhysicsAstronomy and Astrophysics3rd-DASPlasmaCoronaSpace Physics (physics.space-ph)Solar windQC PhysicsMagnetic field13. Climate actionSpace and Planetary SciencePhysics::Space PhysicsCoronal mass ejectionsMagnetohydrodynamicsSolar Physics
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Neutral pion and η meson production in proton–proton collisions at s=0.9 TeV and s=7 TeV

2012

The first measurements of the invariant differential cross sections of inclusive pi(0) and eta meson production at mid-rapidity in proton-proton collisions root s = 0.9 TeV and root s = 7 TeV are reported. The pi(0) measurement covers the ranges 0.4 < p(T) < 7 GeV/c and 0.3 < p(T) < 25 GeV/c for these two energies, respectively. The production of eta mesons was measured at root s = 7 TeV in the range 0.4 < p(T) < 15 GeV/c. Next-to-Leading Order perturbative QCD calculations, which are consistent with the pi(0) spectrum at root s = 0.9 TeV, overestimate those of pi(0) and eta mesons at root s = 7 TeV, but agree with the measured eta/pi(0) ratio at root s = 7 TeV. (C) 2012 CERN. Published by …

PhysicsQuantum chromodynamicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderMeson010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyEta mesonHadronPerturbative QCDElementary particle01 natural sciencesNuclear physicsPion0103 physical sciencesPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsPhysics Letters B
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A prospective new diagnostic technique for distinguishing eruptive and noneruptive active regions

2019

This research has received funding from the Science and Technology Facilities Council (UK) through the consolidated grant ST/N000609/1 and the European Research Council (ERC) under the European Union Horizon 2020 research and innovation program (grant agreement No. 647214). This work used the DiRAC@Durham facility managed by the Institute for Computational Cosmology on behalf of the STFC DiRAC HPC Facility (www.dirac.ac.uk). The equipment was funded by BEIS capital funding via STFC capital grants ST/P002293/1, ST/R002371/1, and ST/S002502/1, Durham University and STFC operations grant ST/R000832/1. DiRAC is part of the National e-Infrastructure. S.L.Y. would like to acknowledge STFC for sup…

Solar coronal mass ejections (310)010504 meteorology & atmospheric sciencesSpace weatherSolar magnetic fieldsSolar activityT-NDASLibrary scienceFOS: Physical sciencesSpace weather (2037)Solar coronaSolar activity (1475)Solar flares (1496)01 natural sciencesSolar coronal mass ejectionsSolar corona (1483)0103 physical sciencesmedia_common.cataloged_instanceAstrophysics::Solar and Stellar AstrophysicsQB AstronomyEuropean union010303 astronomy & astrophysicsQCSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesmedia_commonQBPhysicsEuropean researchSolar active region magnetic fieldsAstronomy and AstrophysicsSolar active region magnetic fields (1975)Solar magnetic fields (1503)Solar active regionsSolar active regions (1974)QC PhysicsAstrophysics - Solar and Stellar Astrophysics13. Climate actionSolar flaresSpace and Planetary SciencePhysics::Space Physics
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Transverse Momentum Distribution and Nuclear Modification Factor of Charged Particles inp+PbCollisions atsNN=5.02  TeV

2013

The transverse momentum (pT) distribution of primary charged particles is measured in minimum bias (non-single-diffractive) p + Pb collisions at root(NN)-N-s = 5.02 TeV with the ALICE detector at the LHC. The pT spectra measured near central rapidity in the range 0.5< p(T) < 20 GeV/c exhibit a weak pseudorapidity dependence. The nuclear modification factor R-pPb is consistent with unity for p(T) above 2 GeV/c. This measurement indicates that the strong suppression of hadron production at high p(T) observed in Pb + Pb collisions at the LHC is not due to an initial-state effect. The measurement is compared to theoretical calculations. DOI: 10.1103/PhysRevLett.110.082302

PhysicsRange (particle radiation)Large Hadron Collider010308 nuclear & particles physicsHadronGeneral Physics and Astronomy01 natural sciencesCharged particleSpectral lineNuclear physicsPseudorapidity0103 physical sciencesHigh Energy Physics::ExperimentRapidityNuclear Experiment010306 general physicsJet quenchingPhysical Review Letters
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Centrality Dependence of the Charged-Particle Multiplicity Density at Midrapidity in Pb-Pb Collisions atsNN=5.02  TeV

2016

The pseudorapidity density of charged particles, dNch/dη, at midrapidity in Pb-Pb collisions has been measured at a center-of-mass energy per nucleon pair of √sNN=5.02 TeV. For the 5% most central collisions, we measure a value of 1943 ± 54. The rise in dNch/dη as a function of √sNN p is steeper than that observed in proton-proton collisions and follows the trend established by measurements at lower energy. The increase of dNch/dη as a function of the average number of participant nucleons, ⟨Npart⟩, calculated in a Glauber model, is compared with the previous measurement at √sNN=2.76 TeV. A constant factor of about 1.2 describes the increase in dNch/dη from √sNN=2.76 to 5.02 TeV for all cen…

PhysicsParticle physicsLarge Hadron Collider010308 nuclear & particles physicsGeneral Physics and Astronomy01 natural sciencesCharged particleNuclear physicsPseudorapidity0103 physical sciencesQuark–gluon plasmaImpact parameterMultiplicity (chemistry)Nuclear Experiment010306 general physicsNucleonGlauberPhysical Review Letters
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Connecting Solar Orbiter remote-sensing observations and Parker Solar Probe in situ measurements with a numerical MHD reconstruction of the Parker sp…

2022

As a key feature, NASA's Parker Solar Probe (PSP) and ESA-NASA's Solar Orbiter (SO) missions cooperate to trace solar wind and transients from their sources on the Sun to the inner interplanetary space. The goal of this work is to accurately reconstruct the interplanetary Parker spiral and the connection between coronal features observed remotely by the Metis coronagraph on-board SO and those detected in situ by PSP at the time of the first PSP-SO quadrature of January 2021. We use the Reverse In-situ and MHD Approach (RIMAP), a hybrid analytical-numerical method performing data-driven reconstructions of the Parker spiral. RIMAP solves the MHD equations on the equatorial plane with the PLUT…

Plasma Physics (physics.plasm-ph)Settore FIS/05 - Astronomia E AstrofisicaAstrophysics - Solar and Stellar AstrophysicsPhysics - Space PhysicsSpace and Planetary ScienceFOS: Physical sciencesAstronomy and Astrophysicsmagnetohydrodynamics (MHD) – methods: numerical – solar wind – Sun: heliosphere – Sun: coronamagnetohydrodynamics(MHD)methods:numericalsolar windSun:heliosphereSun:coronaPhysics - Plasma PhysicsSolar and Stellar Astrophysics (astro-ph.SR)Space Physics (physics.space-ph)
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Azimuthal anisotropy of charged jet production in sNN=2.76 TeV Pb–Pb collisions

2016

We present measurements of the azimuthal dependence of charged jet production in central and semicentral √sNN = 2.76 TeV Pb–Pb collisions with respect to the second harmonic event plane, quantified as vch jet 2 . Jet finding is performed employing the anti-kT algorithm with a resolution parameter R = 0.2 using charged tracks from the ALICE tracking system. The contribution of the azimuthal anisotropy of the underlying event is taken into account event-by-event. The remaining (statistical) region-to-region fluctuations are removed on an ensemble basis by unfolding the jet spectra for different event plane orientations independently. Significant non-zero vch jet 2 is observed in semi-central …

Quantum chromodynamicsPhysicsNuclear and High Energy PhysicsJet (fluid)Particle physics010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical Phenomena01 natural sciencesCharged particleNuclear physics0103 physical sciencesQuark–gluon plasmaHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsAnisotropyParton showerEvent (particle physics)Event generatorPhysics Letters B
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Determination of the event collision time with the ALICE detector at the LHC

2017

The European physical journal / Plus 132(2), 99 (2017). doi:10.1140/epjp/i2017-11279-1

Physics - Instrumentation and DetectorsPhysics::Instrumentation and Detectorsmeasurement methodsGeneral Physics and Astronomycollision time01 natural sciencesParticle identificationALICEscattering [p p]Nuclear Experiment (nucl-ex)Detectors and Experimental Techniquesscattering [nucleus nucleus]time resolutionNuclear ExperimentPhysicsLarge Hadron ColliderDetectorInstrumentation and Detectors (physics.ins-det)nucleus nucleus: scatteringPower (physics)PRIRODNE ZNANOSTI. Fizika.Time of flightLHCParticle physicsp p: scatteringPhysics and Astronomy (all) ALICE LHCeventFOS: Physical sciencesPhysics and Astronomy(all)[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]time-of-flight530114 Physical sciencesNuclear physicsALICE detectorPhysics and Astronomy (all)0103 physical sciencesddc:530Nuclear Physics - Experiment[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]:Matematikk og Naturvitenskap: 400::Fysikk: 430::Kjerne- og elementærpartikkelfysikk: 431 [VDP]010306 general physicsp nucleus: scattering010308 nuclear & particles physicsscattering [p nucleus]PERFORMANCECollisionNATURAL SCIENCES. Physics.efficiencyALICE ; event ; collision timeALICE (propellant)particle identificationEvent (particle physics)
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Inclusive J/ψ production in pp collisions at s=2.76 TeV

2012

The ALICE Collaboration has measured inclusive J/psi production in pp collisions at a center of mass energy sqrt(s)=2.76 TeV at the LHC. The results presented in this Letter refer to the rapidity ranges |y|<0.9 and 2.5

PhysicsNuclear and High Energy PhysicsParticle physicsParticle propertiesLuminosity (scattering theory)Large Hadron ColliderPhysics::Instrumentation and Detectors010308 nuclear & particles physicsElementary particle01 natural sciences0103 physical sciencesRapidityProduction (computer science)Center of massNuclear Experiment010306 general physicsLeptonPhysics Letters B
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Performance of the ALICE VZERO system

2013

ALICE is an LHC experiment devoted to the study of strongly interacting matter in proton-proton, proton--nucleus and nucleus-nucleus collisions at ultra-relativistic energies. The ALICE VZERO system, made of two scintillator arrays at asymmetric positions, one on each side of the interaction point, plays a central role in ALICE. In addition to its core function as a trigger, the VZERO system is used to monitor LHC beam conditions, to reject beam-induced backgrounds and to measure basic physics quantities such as luminosity, particle multiplicity, centrality and event plane direction in nucleus-nucleus collisions. After describing the VZERO system, this publication presents its performance o…

Particle physicsPhysics::Instrumentation and DetectorsLarge detector-systems performance Trigger detectors Large detector systems for particle and astroparticle physics Heavy-ion detectorsmedia_common.quotation_subjectHeavy-ion detectorsNuclear Theorylarge detector-systems performanceFOS: Physical sciencesVZERO detectorlarge detector systems for particle and astroparticle physicsScintillator[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesAsymmetrytrigger detectors; large detector systems for particle and astroparticle physics; heavy-ion detectors; large detector-systems performancetrigger detectorsNuclear physics0103 physical sciencesALICE; trigger; V0NUCLEAR COLLISIONSNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentInstrumentationNuclear ExperimentV0 DETECTORMathematical PhysicsCore functionLarge detector-systems performance; Trigger detectors; Large detector systems for particle and astroparticle physics; Heavy-ion detectors; V0 DETECTOR; NUCLEAR COLLISIONSTrigger detectormedia_commonLarge detector-systems performancePhysicsLarge Hadron ColliderInteraction pointLarge detector systems for particle and astroparticle physics010308 nuclear & particles physicsALICE experimentTrigger detectorsLarge detector systems for particle and astroparticle physicheavy-ion detectorsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGCentralityLarge detector-systems performance; Trigger detectors; Large detector systems for particle and astroparticle physics; Heavy-ion detectorsParticle Physics - Experiment
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First Determination of 2D Speed Distribution within the Bodies of Coronal Mass Ejections with Cross-correlation Analysis

2019

The determination of the speed of Coronal Mass Ejections (CMEs) is usually done by tracking brighter features (such as the CME front and core) in visible light coronagraphic images and by deriving unidimensional profiles of the CME speed as a function of altitude or time. Nevertheless, CMEs are usually characterized by the presence of significant density inhomogeneities propagating outward with different radial and latitudinal projected speeds, resulting in a complex evolution eventually forming the Interplanetary CME. In this work, we demonstrate for the first time how coronagraphic image sequences can be analyzed with cross-correlation technique to derive 2D maps of the almost instantaneo…

Magnetohydrodynamics (MHD)010504 meteorology & atmospheric sciencesDistribution (number theory)Sun: coronal mass ejections (CMEs)FOS: Physical sciencesAstrophysicspolarimetric [Techniques]magnetohydrodynamics (MHD)01 natural sciences0103 physical sciencesCoronal mass ejectionQB AstronomyAstrophysics::Solar and Stellar Astrophysicsmedia_common.cataloged_instanceEuropean uniondata analysis [Methods]010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)QCQB0105 earth and related environmental sciencesmedia_commonPhysicsUV radiation [Sun]Horizon (archaeology)Cross correlation analysisDASAstronomy and AstrophysicsSun: UV radiationmethods: data analysiscoronal mass ejections (CMEs) [Sun]techniques: polarimetricQC PhysicsAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary SciencePhysics::Space PhysicsAstrophysics::Earth and Planetary AstrophysicsThe Astrophysical Journal
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Measurement of the Cross Section for Electromagnetic Dissociation with Neutron Emission in Pb-Pb Collisions atsNN=2.76  TeV

2012

The first measurement of neutron emission in electromagnetic dissociation of Pb-208 nuclei at the LHC is presented. The measurement is performed using the neutron zero degree calorimeters of the ALICE experiment, which detect neutral particles close to beam rapidity. The measured cross sections of single and mutual electromagnetic dissociation of Pb nuclei at root s(NN) = 2.76 TeV with neutron emission are sigma(singleEMD) = 187.4 +/- 0.2(stat)(-11.2)(+13.2) (syst) b and sigma(mutualEMD) = 5. 7 +/- 0.1(stat) +/- 0.4(syst) b, respectively. The experimental results are compared to the predictions from a relativistic electromagnetic dissociation model. DOI: 10.1103/PhysRevLett.109.252302

PhysicsLarge Hadron ColliderIsotope010308 nuclear & particles physicsStable isotope ratioNeutron emissionAstrophysics::High Energy Astrophysical PhenomenaGeneral Physics and AstronomySigma01 natural sciencesDissociation (chemistry)Nuclear physics0103 physical sciencesHigh Energy Physics::ExperimentNeutronRapidityAtomic physicsNuclear Experiment010306 general physicsPhysical Review Letters
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The importance of magnetic-field-oriented thermal conduction in the interaction of SNR shocks with interstellar clouds

2008

We explore the importance of magnetic-field-oriented thermal conduction in the interaction of supernova remnant (SNR) shocks with radiative gas clouds and in determining the mass and energy exchange between the clouds and the hot surrounding medium. We perform 2.5D MHD simulations of a shock impacting on an isolated gas cloud, including anisotropic thermal conduction and radiative cooling; we consider the representative case of a Mach 50 shock impacting on a cloud ten-fold denser than the ambient medium. We consider different configurations of the ambient magnetic field and compare MHD models with or without the thermal conduction. The efficiency of the thermal conduction in the presence of…

PhysicsRadiative coolingsupernovaeAstrophysics (astro-ph)Interstellar cloudFOS: Physical sciencesAstronomy and Astrophysicsheat conductionAstrophysicsMagnetohydrodynamicThermal conductionAstrophysicsComputational physicsMagnetic fieldSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceThermalRadiative transferMagnetohydrodynamicsSupernova remnantAstrophysics::Galaxy Astrophysics
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Numerical Simulations of a Flux Rope Ejection

2015

Coronal mass ejections (CMEs) are the most violent phenomena observed on the Sun. One of the most successful models to explain CMEs is the flux rope ejection model, where a magnetic flux rope is expelled from the solar corona after a long phase along which the flux rope stays in equilibrium while magnetic energy is being accumulated. However, still many questions are outstanding on the detailed mechanism of the ejection and observations continuously provide new data to interpret and put in the context. Currently, extreme ultraviolet (EUV) images from the Atmospheric Imaging Assembly (AIA) on board the Solar Dynamic Observatory (SDO) are providing new insights into the early phase of CME evo…

SimulationsPhysicsNDASAstronomy and AstrophysicsCoronal loopAstrophysicsCoronaMagnetic fluxNanoflaresMagnetohydrodynamicsQC PhysicsCoronal mass ejections—magnetohydrodynamics—simulations—coronaSpace and Planetary ScienceMagnetic helicityPhysics::Space PhysicsCoronal mass ejectionsCoronal mass ejectionCoronaAstrophysics::Solar and Stellar AstrophysicsMagnetic cloudQCRopeJournal of Astrophysics and Astronomy
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Acoustic Wave Properties in Footpoints of Coronal Loops in 3D MHD Simulations

2021

Acoustic waves excited in the photosphere and below might play an integral part in the heating of the solar chromosphere and corona. However, it is yet not fully clear how much of the initially acoustic wave flux reaches the corona and in what form. We investigate the wave propagation, damping, transmission, and conversion in the lower layers of the solar atmosphere using 3D numerical MHD simulations. A model of a gravitationally stratified expanding straight coronal loop, stretching from photosphere to photosphere, is perturbed at one footpoint by an acoustic driver with a period of 370 seconds. For this period acoustic cutoff regions are present below the transition region (TR). About 2% …

PhysicsPhotosphere010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaSolar physics Solar atmosphere Solar oscillations Solar coronal waves Solar chromosphere Solar coronal loops Magnetohydrodynamical simulations MagnetohydrodynamicsFOS: Physical sciencesAstronomy and AstrophysicsAcoustic waveCoronal loop01 natural sciencesCoronaComputational physicsStanding waveAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary Science0103 physical sciencesCutoffAstrophysics::Solar and Stellar AstrophysicsMagnetohydrodynamics010303 astronomy & astrophysicsChromosphereSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesThe Astrophysical Journal
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Asymmetric Twisting of Coronal Loops

2023

The bright solar corona entirely consists of closed magnetic loops rooted in the photosphere. Photospheric motions are important drivers of magnetic stressing, which eventually leads to energy release into heat. These motions are chaotic and obviously different from one footpoint to the other, and in fact, there is strong evidence that loops are finely stranded. One may also expect strong transient variations along the field lines, but at a glance, coronal loops ever appear more or less uniformly bright from one footpoint to the other. We aim to understand how much coronal loops can preserve their own symmetry against asymmetric boundary motions that are expected to occur at loop footpoints…

Settore FIS/05 - Astronomia E AstrofisicaPhysics and Astronomy (miscellaneous)Chemistry (miscellaneous)activitysun: activityGeneral Mathematicssunplasmas: magnetohydrodynamics (MHD)Computer Science (miscellaneous)plasmascoronamagnetohydrodynamics (MHD)sun: coronaSymmetry
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Coherent ψ(2S) photo-production in ultra-peripheral Pb Pb collisions at sNN=2.76 TeV

2015

We have performed the first measurement of the coherent ψ(2S) photo-production cross section in ultraperipheral Pb–Pb collisions at the LHC. This charmonium excited state is reconstructed via the ψ(2S) → l +l − and ψ(2S) → J/ψπ+π− decays, where the J/ψ decays into two leptons. The analysis is based on an event sample corresponding to an integrated luminosity of about 22 μb−1. The cross section for coherent ψ(2S) production in the rapidity interval −0.9 < y < 0.9 is dσcoh ψ(2S)/dy = 0.83±0.19 stat+syst mb. The ψ(2S) to J/ψ coherent cross section ratio is 0.34+0.08 −0.07(stat + syst). The obtained results are compared to predictions from theoretical models.

Nuclear physicsPhysicsNuclear and High Energy PhysicsParticle physicsMesonBranching fractionHadronRapidityWave function7. Clean energyGlauberParticle identificationCrystal BallPhysics Letters B
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Suppression of ϒ(1S) at forward rapidity in Pb–Pb collisions at sNN=2.76 TeV

2014

We report on the measurement of the inclusive Υ (1S) production in Pb–Pb collisions at √sNN = 2.76 TeV carried out at forward rapidity (2.5 < y < 4) and down to zero transverse momentum using its μ+μ− decay channel with the ALICE detector at the Large Hadron Collider. A strong suppression of the inclusive Υ (1S) yield is observed with respect to pp collisions scaled by the number of independent nucleon– nucleon collisions. The nuclear modification factor, for events in the 0–90% centrality range, amounts to 0.30 ± 0.05(stat) ± 0.04(syst). The observed Υ (1S) suppression tends to increase with the centrality of the collision and seems more pronounced than in corresponding mid-rapidity measur…

PhysicsNuclear physicsNuclear and High Energy PhysicsRange (particle radiation)Large Hadron ColliderQuark–gluon plasmaTransverse momentumHigh Energy Physics::ExperimentModification factorRapidityNuclear ExperimentNucleonPhysics Letters B
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Centrality determination of Pb-Pb collisions atsNN=2.76TeV with ALICE

2013

This publication describes the methods used to measure the centrality of inelastic Pb-Pb collisions at a center-of-mass energy of 2.76 TeV per colliding nucleon pair with ALICE. The centrality is a key parameter in the study of the properties of QCD matter at extreme temperature and energy density, because it is directly related to the initial overlap region of the colliding nuclei. Geometrical properties of the collision, such as the number of participating nucleons and the number of binary nucleon-nucleon collisions, are deduced from a Glauber model with a sharp impact parameter selection and shown to be consistent with those extracted from the data. The centrality determination provides …

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsNuclear TheoryBinary numberCollision01 natural sciencesMeasure (mathematics)Nuclear physics0103 physical sciencesImpact parameterNuclear Experiment010306 general physicsNucleonCentralityGlauberQCD matterPhysical Review C
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Measurement of jet suppression in central Pb–Pb collisions at sNN=2.76 TeV

2015

The transverse momentum(p(T)) spectrum and nuclear modification factor (R-AA) of reconstructed jets in 0-10% and 10-30% central Pb-Pb collisions at root s(NN) = 2.76 TeV were measured. Jets were reconstructed using the anti-k(T) jet algorithm with a resolution parameter of R = 0.2 from charged and neutral particles, utilizing the ALICE tracking detectors and Electromagnetic Calorimeter (EMCal). The jet p(T) spectra are reported in the pseudorapidity interval of \eta(jet)\ 5 GeV/c to suppress jets constructed from the combinatorial background in Pb-Pb collisions. The leading charged particle requirement applied to jet spectra both in pp and Pb-Pb collisions had a negligible effect on the R-A…

PhysicsNuclear and High Energy PhysicsParticle physicsJet (fluid)Large Hadron ColliderAstrophysics::High Energy Astrophysical PhenomenaSpectral lineCharged particleNuclear physicsPseudorapidityHigh Energy Physics::ExperimentRapidityNuclear ExperimentJet quenchingNeutral particlePhysics Letters B
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Measurement of the Spin Structure of the Deuteron in the DIS Region

2005

We present a new measurement of the longitudinal spin asymmetry A_1^d and the spin-dependent structure function g_1^d of the deuteron in the range 1 GeV^2 &lt; Q^2 &lt; 100 GeV^2 and 0.004&lt; x &lt;0.7. The data were obtained by the COMPASS experiment at CERN using a 160 GeV polarised muon beam and a large polarised 6-LiD target. The results are in agreement with those from previous experiments and improve considerably the statistical accuracy in the region 0.004 &lt; x &lt; 0.03.

Nuclear and High Energy PhysicsParticle physicsmedia_common.quotation_subjectFOS: Physical sciencesSpin structure01 natural sciencesAsymmetryCOMPASSHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)deep inelastic scatteringstructure function0103 physical sciencesCOMPASS experiment010306 general physicsNuclear Experimentmedia_commonSpin-½PhysicsLarge Hadron ColliderMuon010308 nuclear & particles physicsDeep inelastic scatteringstructure function; COMPASS; DEEP INELASTIC-SCATTERINGstructure functionsDEEP INELASTIC-SCATTERINGHigh Energy Physics::ExperimentParticle Physics - ExperimentBeam (structure)
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Multiplicity dependence of charged pion, kaon, and (anti)proton production at large transverse momentum in p–Pb collisions at sNN=5.02 TeV

2016

The production of charged pions, kaons and (anti)protons has been measured at mid-rapidity ($-0.5 10$ GeV/$c$), the particle ratios are consistent with those reported for pp and Pb-Pb collisions at the LHC energies. At intermediate $p_{\rm T}$ the (anti)proton $R_{\rm pPb}$ shows a Cronin-like enhancement, while pions and kaons show little or no nuclear modification. At high $p_{\rm T}$ the charged pion, kaon and (anti)proton $R_{\rm pPb}$ are consistent with unity within statistical and systematic uncertainties.

PhysicsNuclear and High Energy PhysicsParticle physicsProton010308 nuclear & particles physicsNuclear TheoryHadron7. Clean energy01 natural sciencesParticle identificationCharged particleNuclear physicsPionAntiproton0103 physical sciencesQuark–gluon plasmaHigh Energy Physics::ExperimentRapidityNuclear Experiment010306 general physicsPhysics Letters B
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Effect of coronal loop structure on wave heating through phase mixing

2020

Context. The mechanism(s) behind coronal heating still elude(s) direct observation and modelling of viable theoretical processes and the subsequent effect on coronal structures is one of the key tools available to assess possible heating mechanisms. Wave heating via the phase mixing of magnetohydrodynamic (MHD) transverse waves has been proposed as a possible way to convert magnetic energy into thermal energy, but MHD models increasingly suggest this is not an efficient enough mechanism. Aims. We modelled heating by phase mixing transverse MHD waves in various configurations in order to investigate whether certain circumstances can enhance the heating sufficiently to sustain the million deg…

PhysicsMagnetohydrodynamics (MHD)Magnetic energySun: corona010308 nuclear & particles physicsF300Astronomy and AstrophysicsTransverse waveAstrophysicsCoronal loopMechanicsF500Dissipation01 natural sciencesTransverse planeSpace and Planetary Science0103 physical sciencesPhysics::Space PhysicsAstrophysics::Solar and Stellar AstrophysicsMagnetohydrodynamic driveBoundary value problemSun: oscillationsMagnetohydrodynamics010303 astronomy & astrophysicsSun: atmosphere
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Magnetohydrodynamic simulations of the ejection of a magnetic flux rope

2013

Context. Coronal mass ejections (CME's) are one of the most violent phenomena found on the Sun. One model to explain their occurrence is the flux rope ejection model. In this model, magnetic flux ropes form slowly over time periods of days to weeks. They then lose equilibrium and are ejected from the solar corona over a few hours. The contrasting time scales of formation and ejection pose a serious problem for numerical simulations. Aims: We simulate the whole life span of a flux rope from slow formation to rapid ejection and investigate whether magnetic flux ropes formed from a continuous magnetic field distribution, during a quasi-static evolution, can erupt to produce a CME. Methods: To …

Q ScienceMagnetohydrodynamics (MHD)coronal mass ejections [Sun]010504 meteorology & atmospheric sciencescorona [Sun]FluxAstrophysicsmagnetic fields01 natural sciencesmagnetohydrodynamics (MHD)0103 physical sciencesCoronal mass ejectionAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysics0105 earth and related environmental sciencesPhysicsSun: coronal mass ejectionsSun: coronaQSunAstronomy and AstrophysicsCoronal loopCoronaMagnetic fluxNanoflares13. Climate actionSpace and Planetary ScienceMagnetic fieldsPhysics::Space PhysicsCoronal mass ejectionsCoronaMagnetohydrodynamicsRope
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A new technique for observationally derived boundary conditions for space weather

2018

This research has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No 647214). D.H.M. would like to thank STFC and the Leverhulme Trust for their financial support. ARY was supported by STFC consortium grant ST/N000781/1 to the universities of Dundee and Durham. Context.  In recent years, space weather research has focused on developing modelling techniques to predict the arrival time and properties of coronal mass ejections (CMEs) at the Earth. The aim of this paper is to propose a new modelling technique suitable for the next generation of Space Weather predictive tools that is both efficie…

Atmospheric Science010504 meteorology & atmospheric sciencesMHDNDASWeather forecastingFluxFOS: Physical sciencesContext (language use)Space weatherlcsh:QC851-999computer.software_genre01 natural sciencesSolar Corona0103 physical sciencesCMECoronal mass ejectionQB AstronomyAstrophysics::Solar and Stellar AstrophysicsQA MathematicsBoundary value problemQA010303 astronomy & astrophysicsR2CSolar and Stellar Astrophysics (astro-ph.SR)QB0105 earth and related environmental sciencesPhysicssolar CoronaMechanicsMagnetic fluxAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary SciencePhysics::Space Physicslcsh:Meteorology. ClimatologyMagnetohydrodynamicsBDCcomputerJournal of Space Weather and Space Climate
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Constraining the pass-band of future space-based coronagraphs for observations of solar eruptions in the FeXIV 530.3 nm “green line”

2017

This research has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No 647214) and from the UK Science and Technology Facilities Council. Observations of the solar corona in the FeXIV 530.3 nm “green line” have been very important in the past, and are planned for future coronagraphs on-board forthcoming space missions such as PROBA-3 and Aditya. For these instruments, a very important parameter to be optimized is the spectral width of the band-pass filter to be centred over the “green line”. Focusing on solar eruptions, motions occurring along the line of sight will Doppler shift the line prof…

coronal mass ejections [Sun]corona [Sun]media_common.quotation_subjectAstrophysics01 natural sciences010309 opticssymbols.namesakeSuperposition principle0103 physical sciencesSpectral widthQB AstronomySun: Coronal mass ejections010303 astronomy & astrophysicsQCmedia_commonLine (formation)Spectral purityQBPhysicsLine-of-sightnumerical [Methods]Sun: CoronaAstronomyInstrumentation: CoronagraphsAstronomy and AstrophysicsDASQC Physics13. Climate actionSkySpace and Planetary Sciencecoronagraphs [Instrumentation]Methods: NumericalsymbolsMagnetohydrodynamicsDoppler effectExperimental Astronomy
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Centrality evolution of the charged-particle pseudorapidity density over a broad pseudorapidity range in Pb–Pb collisions at sNN=2.76 TeV

2016

State Committee of Science, World Federation of Scientists (WFS) and Swiss Fonds Kidagan, Armenia; Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq), Financiadora de Estudos e Projetos (FINEP), Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP); National Natural Science Foundation of China (NSFC), the Chinese Ministry of Education (CMOE) and the Ministry of Science and Technology of China (MSTC); Ministry of Education and Youth of the Czech Republic; Danish Natural Science Research Council, the Carlsberg Foundation and the Danish National Research Foundation; The European Research Council under the European Community's Seventh Framework Programme; Helsinki Inst…

PhysicsNuclear and High Energy PhysicsLatin AmericansHigher educationEuropean community010308 nuclear & particles physicsbusiness.industryAtomic energyEuropean researchIndustrial researchLibrary science01 natural sciences7. Clean energyBildungNuclear physics0103 physical sciences010306 general physicsChinabusinessPhysics Letters B
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Uncertainties in polarimetric 3D reconstructions of coronal mass ejections

2015

P.P. acknowledges STFC for financial support. Date of Acceptance: 21/01/2015 Aims. The aim of this work is to quantify the uncertainties in the three-dimensional (3D) reconstruction of the location of coronal mass ejections (CMEs) obtained with the so-called polarization ratio technique. The method takes advantage of the different distributions along the line of sight of total (tB) and polarized (pB) brightnesses emitted by Thomson scattering to estimate the average location of the emitting plasma. This is particularly important to correctly identify of CME propagation angles and unprojected velocities, thus allowing better capabilities for space weather forecastings. Methods. To this end, …

Electron densitycorona [Sun]Sun: coronal mass ejections (CMEs)NDASDensityFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSpace weatherpolarimetric [Techniques]Position (vector)Coronal mass ejectionQCSolar and Stellar Astrophysics (astro-ph.SR)PhysicsLine-of-sightSun: coronaPlane (geometry)Techniques: polarimetricAstronomy and Astrophysicscoronal mass ejections (CMEs) [Sun]ViewpointsQC PhysicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsHaloCenter of mass
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Measurement of an Excess in the Yield ofJ/ψat Very LowpTin Pb–Pb Collisions atsNN=2.76  TeV

2016

We report on the first measurement of an excess in the yield of J/ψ at very low transverse momentum (pT< 0.3 GeV/c) in peripheral hadronic Pb-Pb collisions at √sNN = 2.76 TeV, performed by ALICE at the CERN LHC. Remarkably, the measured nuclear modification factor of J/ψ in the rapidity range 2.5< y< 4 reaches about 7 (2) in the pT range 0- 0.3 GeV/c in the 70-90% (50-70%) centrality class. The J/ψ production cross section associated with the observed excess is obtained under the hypothesis that coherent photoproduction of J/ψ is the underlying physics mechanism. If confirmed, the observation of J/ψ coherent photoproduction in Pb-Pb collisions at impact parameters smaller than twice the nuc…

Nuclear reactionPhysicsParticle physics010308 nuclear & particles physicsBranching fractionNuclear TheoryHadronGeneral Physics and AstronomyQuarkonium01 natural sciences7. Clean energyNuclear physics13. Climate action0103 physical sciencesQuark–gluon plasmaHigh Energy Physics::ExperimentRapidityImpact parameterNuclear Experiment010306 general physicsGlauberPhysical Review Letters
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Future capabilities of CME polarimetric 3D reconstructions with the METIS instrument: A numerical test

2015

D.H.M. would like to thank STFC and the Leverhulme Trust for their financial support. P.P. would like to thank STFC and the Leverhulme Trust. The computational work for this paper was carried out on the joint STFC and SFC (SRIF) funded cluster at the University of St Andrews (Scotland, UK). Context. Understanding the 3D structure of coronal mass ejections (CMEs) is crucial for understanding the nature and origin of solar eruptions. However, owing to the optical thinness of the solar corona we can only observe the line of sight integrated emission. As a consequence the resulting projection effects hide the true 3D structure of CMEs. To derive information on the 3D structure of CMEs from whit…

Magnetohydrodynamics (MHD)corona [Sun]Sun: coronal mass ejections (CMEs)Sun: filaments prominencesNDASFOS: Physical sciencesLibrary scienceAstrophysicspolarimetric [Techniques]MetisQB AstronomyAstrophysics::Solar and Stellar AstrophysicsNumerical testsQCSolar and Stellar Astrophysics (astro-ph.SR)QBPhysicsSun: coronaTechniques: polarimetricAstronomy and Astrophysicscoronal mass ejections (CMEs) [Sun]QC PhysicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space Physicsfilaments prominences [Sun]
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Centrality dependence ofπ,K, andpproduction in Pb-Pb collisions atsNN=2.76TeV

2013

In this paper measurements are presented of pi(+/-), K-+/-, p, and (p) over bar production at midrapidity (vertical bar y vertical bar < 0.5), in Pb-Pb collisions at root s(NN) = 2.76 TeV as a function of centrality. The measurement covers the transverse-momentum (p(T)) range from 100, 200, and 300 MeV/c up to 3, 3, and 4.6 GeV/c for pi, K, and p, respectively. The measured p(T) distributions and yields are compared to expectations based on hydrodynamic, thermal and recombination models. The spectral shapes of central collisions show a stronger radial flow than measured at lower energies, which can be described in hydrodynamic models. In peripheral collisions, the p(T) distributions are not…

PhysicsNuclear and High Energy PhysicsRange (particle radiation)Proton010308 nuclear & particles physicsRoot (chord)01 natural sciences7. Clean energyNuclear physicsPionYield (chemistry)0103 physical sciencesQuark–gluon plasmaPiNuclear Experiment010306 general physicsBar (unit)Physical Review C
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Event-shape engineering for inclusive spectra and elliptic flow in Pb-Pb collisions atsNN=2.76TeV

2016

We report on results obtained with the event-shape engineering technique applied to Pb-Pb collisions at √sNN=2.76 TeV. By selecting events in the same centrality interval, but with very different average flow, different initial-state conditions can be studied. We find the effect of the event-shape selection on the elliptic flow coefficient v2 to be almost independent of transverse momentum pT, which is as expected if this effect is attributable to fluctuations in the initial geometry of the system. Charged-hadron, -pion, -kaon, and -proton transverse momentum distributions are found to be harder in events with higher-than-average elliptic flow, indicating an interplay between radial and ell…

PhysicsParticle physicsProton010308 nuclear & particles physicsHadronElliptic flowParton01 natural sciencesNuclear physicsPionFlow (mathematics)0103 physical sciencesRapidityNuclear Experiment010306 general physicsGlauberPhysical Review C
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Production of inclusive ϒ(1S) and ϒ(2S) in p–Pb collisions at sNN=5.02 TeV

2015

We report on the production of inclusive Y{hooktop}(1S) and Y{hooktop}(2S) in p-Pb collisions at √sNN=5.02 TeV at the LHC. The measurement is performed with the ALICE detector at backward (-4.46<ycms<-2.96) and forward (2.03<ycms<3.53) rapidity down to zero transverse momentum. The production cross sections of the Y{hooktop}(1S) and Y{hooktop}(2S) are presented, as well as the nuclear modification factor and the ratio of the forward to backward yields of Y{hooktop}(1S). A suppression of the inclusive Y{hooktop}(1S) yield in p-Pb collisions with respect to the yield from pp collisions scaled by the number of binary nucleon-nucleon collisions is observed at forward rapidity but not at backwar…

Quantum chromodynamicsNuclear physicsPhysicsNuclear and High Energy PhysicsLarge Hadron ColliderYield (chemistry)Transverse momentumBinary numberProduction (computer science)RapidityNuclear Experiment7. Clean energyColor-glass condensatePhysics Letters B
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K*(892)0 and ϕ(1020) meson production at high transverse momentum in pp and Pb-Pb collisions at sNN=2.76 TeV

2017

The yields of the K*(892)(0) and phi(1020) resonances are measured in Pb-Pb collisions at root s(NN) = 2.76 TeV through their hadronic decays using the ALICE detector. The measurements are performed in multiple centrality intervals at mid-rapidity (vertical bar y vertical bar <0.5) in the transverse-momentum ranges 0.3 <p(T) <5 GeV/c for the K*(892)(0) and 0.5 <p(T) <5 GeV/c for the phi(1020). The yields of K*(892)(0) are suppressed in central Pb-Pb collisions with respect to pp and peripheral Pb-Pb collisions (perhaps due to rescattering of its decay products in the hadronic medium), while the longer-lived phi(1020) meson is not suppressed. These particles are also used as probes to study …

Quantum chromodynamicsPhysicsQuarkNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderLuminosity (scattering theory)Meson010308 nuclear & particles physicsNuclear TheoryHadronLambda01 natural sciencesSpectral lineNuclear physicsPionYield (chemistry)Quark–gluon plasma0103 physical sciencesParticleHigh Energy Physics::ExperimentRapidityNuclear Experiment010306 general physicsPhysical Review C
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Correlated Event-by-Event Fluctuations of Flow Harmonics in Pb-Pb Collisions at sNN=2.76  TeV

2016

We report the measurements of correlations between event-by-event fluctuations of amplitudes of anisotropic flow harmonics in nucleus-nucleus collisions, obtained for the first time using a new analysis method based on multiparticle cumulants in mixed harmonics. This novel method is robust against systematic biases originating from non-flow effects and by construction any dependence on symmetry planes is eliminated. We demonstrate that correlations of flow harmonics exhibit a better sensitivity to medium properties than the individual flow harmonics. The new measurements are performed in Pb-Pb collisions at the centre-of-mass energy per nucleon pair of $\sqrt{s_{_{\rm NN}}}=2.76$ TeV by the…

PhysicsLarge Hadron Collider010308 nuclear & particles physicsElliptic flowGeneral Physics and Astronomy01 natural sciencesHarmonic analysisNuclear physicsFlow (mathematics)Harmonics0103 physical sciencesQuark–gluon plasmaImpact parameterNuclear Experiment010306 general physicsEnergy (signal processing)Physical Review Letters
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Particle identification in ALICE: a Bayesian approach

2016

We present a Bayesian approach to particle identification (PID) within the ALICE experiment. The aim is to more effectively combine the particle identification capabilities of its various detectors. After a brief explanation of the adopted methodology and formalism, the performance of the Bayesian PID approach for charged pions, kaons and protons in the central barrel of ALICE is studied. PID is performed via measurements of specific energy loss ($\mathrm{d}E/\mathrm{d}x$) and time-of-flight. PID efficiencies and misidentification probabilities are extracted and compared with Monte Carlo simulations using high-purity samples of identified particles in the decay channels ${\rm K}^0_S \righta…

:Kjerne- og elementærpartikkelfysikk: 431 [VDP]Monte Carlo methodGeneral Physics and AstronomyPID controllerPP01 natural sciencesParticle identificationHigh Energy Physics - ExperimentParticle identificationHigh Energy Physics - Experiment (hep-ex)ALICEHadron-Hadron scattering (experiments)Heavy-ion collisionNuclear and High Energy Physics Hadron-Hadron scattering (experiments) Heavy Ion Experiments Heavy-ion collision Quark gluon plasma Particle identification Bayesianscattering [p p][PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear Experiment (nucl-ex)Detectors and Experimental TechniquesNuclear ExperimentNuclear ExperimentPhysicsefficiency [particle identification]PB COLLISIONSVDP::Kjerne- og elementærpartikkelfysikk: 431Monte Carlo [numerical calculations]PB COLLISIONS PP PERFORMANCE.:Mathematics and natural scienses: 400::Physics: 430::Nuclear and elementary particle physics: 431 [VDP]PRIRODNE ZNANOSTI. Fizika.Time of flight:Nuclear and elementary particle physics: 431 [VDP]VDP::Nuclear and elementary particle physics: 431performancemomentum spectrum [charged particle]Nuclear and High Energy PhysicsParticle physicsMesoneducationBayesian probabilityFOS: Physical sciencesQuark gluon plasma[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]114 Physical sciencesBayesianNuclear physicsPhysics and Astronomy (all)PionHeavy Ion Experiments0103 physical sciencesddc:530010306 general physics010308 nuclear & particles physicsBayesian approach:Matematikk og naturvitenskap: 400::Fysikk: 430::Kjerne- og elementærpartikkelfysikk: 431 [VDP]ALICE experimentPERFORMANCEparticle identification ; Bayesian approachNATURAL SCIENCES. Physics.PB COLLISIONS; TEV; PP; PERFORMANCEPhysics - Data Analysis Statistics and ProbabilityQuark–gluon plasmaBayesian [statistics]TEVHigh Energy Physics::Experimentparticle identificationData Analysis Statistics and Probability (physics.data-an)
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Contribution of observed multi frequency spectrum of Alfvén waves to coronal heating

2019

Context. Whilst there are observational indications that transverse magnetohydrodynamic (MHD) waves carry enough energy to maintain the thermal structure of the solar corona, it is not clear whether such energy can be efficiently and effectively converted into heating. Phase-mixing of Alfvén waves is considered a candidate mechanism, as it can develop transverse gradient where magnetic energy can be converted into thermal energy. However, phase-mixing is a process that crucially depends on the amplitude and period of the transverse oscillations, and only recently have we obtained a complete measurement of the power spectrum for transverse oscillations in the corona. Aims. We aim to investig…

atmosphere [Sun]Magnetohydrodynamics (MHD)corona [Sun]T-NDASContext (language use)Astrophysics01 natural sciences03 medical and health sciences0103 physical sciencesQB AstronomyAstrophysics::Solar and Stellar AstrophysicsQA MathematicsSun: oscillationsQASun: magnetic fields010303 astronomy & astrophysicsQCQB030304 developmental biologyPhysics0303 health sciencesMagnetic energySun: coronaoscillations [Sun]Spectral densityAstronomy and AstrophysicsTransverse waveCoronal loopComputational physicsTransverse planeQC PhysicsAmplitudemagnetic fields [Sun]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsWavesMagnetohydrodynamicsSun: atmosphereAstronomy &amp; Astrophysics
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A space weather tool for identifying eruptive active regions

2019

Funding: UK Science and Technology Facilities Council (UK) through the consolidated grant ST/N000609/1 and the European Research Council (ERC) under the European Union Horizon 2020 research and innovation program (grant agreement No. 647214); UK STFC via the Consolidated Grant SMC1/YST025 and SMC1/YST037 (S.L.Y.); UK STFC and the ERC (SynergyGrant: WHOLE SUN, Grant Agreement No. 810218) for financial support (DHM). One of the main goals of solar physics is the timely identification of eruptive active regions. Space missions such as Solar Orbiter or future Space Weather forecasting missions would largely benefit from this achievement.Our aim is to produce a relatively simple technique that c…

010504 meteorology & atmospheric sciencesSpace weatherSolar magnetic fieldsFOS: Physical sciencesSpace weather01 natural sciences3rd-NDASSolar coronal mass ejections0103 physical sciencesRegional sciencemedia_common.cataloged_instanceQB AstronomyEuropean union010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)QC0105 earth and related environmental sciencesmedia_commonQBPhysicsHorizon (archaeology)European researchAstronomy and AstrophysicsSolar active region magnetic fieldsSolar active regionsQC PhysicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary Science
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Gluon polarization in the nucleon from quasi-real photoproduction of high-pT hadron pairs

2006

Abstract We present a determination of the gluon polarization Δ G / G in the nucleon, based on the helicity asymmetry of quasi-real photoproduction events, Q 2 1 ( GeV / c ) 2 , with a pair of large transverse-momentum hadrons in the final state. The data were obtained by the COMPASS experiment at CERN using a 160 GeV polarized muon beam scattered on a polarized 6 LiD target. The helicity asymmetry for the selected events is 〈 A ∥ / D 〉 = 0.002 ± 0.019 ( stat ) ± 0.003 ( syst ) . From this value, we obtain in a leading-order QCD analysis Δ G / G = 0.024 ± 0.089 ( stat ) ± 0.057 ( syst ) at x g = 0.095 and μ 2 ≃ 3 ( GeV / c ) 2 .

Quantum chromodynamicsPhysicsNuclear and High Energy PhysicsParticle physicsMuon010308 nuclear & particles physicsHadronDeep inelastic scattering01 natural sciencesHelicityGluonNuclear physics0103 physical sciencesCOMPASS experimentHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsNucleonPhysics Letters B
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Centrality dependence of particle production inp−Pbcollisions atsNN=5.02TeV

2015

We report measurements of the primary charged-particle pseudorapidity density and transverse momentum distributions in p-Pb collisions at root s(NN) = 5.02 TeV and investigate their correlation with experimental observables sensitive to the centrality of the collision. Centrality classes are defined by using different event-activity estimators, i.e., charged-particle multiplicities measured in three different pseudorapidity regions as well as the energy measured at beam rapidity (zero degree). The procedures to determine the centrality, quantified by the number of participants (N-part) or the number of nucleon-nucleon binary collisions (N-coll) are described. We show that, in contrast to Pb…

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron Collider010308 nuclear & particles physicsHadronMultiplicity (mathematics)16. Peace & justice01 natural sciencesNuclear physicsPseudorapidity0103 physical sciencesRapidityNuclear Experiment010306 general physicsNucleonCentralityEvent generatorPhysical Review C
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Centrality dependence of the nuclear modification factor of charged pions, kaons, and protons in Pb-Pb collisions atsNN=2.76TeV

2016

Transverse momentum (pT) spectra of pions, kaons, and protons up to pT=20GeV/c have been measured in Pb-Pb collisions at √sNN=2.76TeV using the ALICE detector for six different centrality classes covering 0%–80%. The proton-to-pion and the kaon-to-pion ratios both show a distinct peak at pT≈3GeV/c in central Pb-Pb collisions that decreases for more peripheral collisions. For pT>10GeV/c, the nuclear modification factor is found to be the same for all three particle species in each centrality interval within systematic uncertainties of 10%–20%. This suggests there is no direct interplay between the energy loss in the medium and the particle species composition in the hard core of the quenched…

PhysicsSemileptonic decayParticle physics010308 nuclear & particles physicsNuclear TheoryHadron01 natural sciencesCharged particleParticle identificationBaryonNuclear physicsPion0103 physical sciencesQuark–gluon plasmaHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsJet quenchingPhysical Review C
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J/ψPolarization inppCollisions ats=7  TeV

2012

The ALICE Collaboration has studied J/psi production in pp collisions at root s = 7 TeV at the LHC through its muon pair decay. The polar and azimuthal angle distributions of the decay muons were measured, and results on the J/psi polarization parameters lambda(theta) and lambda(phi) were obtained. The study was performed in the kinematic region 2: 5 < y < 4, 2 < p(t) < 8 GeV/c, in the helicity and Collins-Soper reference frames. In both frames, the polarization parameters are compatible with zero, within uncertainties.

PhysicsParticle physicsMuonLarge Hadron ColliderPhysics::Instrumentation and Detectors010308 nuclear & particles physicsGeneral Physics and AstronomyLambdaPolarization (waves)01 natural sciencesHelicityNuclear physicsAzimuthAngular distribution0103 physical sciencesHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsReference framePhysical Review Letters
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Determining the source and eruption dynamics of a stealth CME using NLFFF modelling and MHD simulations

2021

Coronal mass ejections (CMEs) that exhibit weak or no eruption signatures in the low corona, known as stealth CMEs, are problematic as upon arrival at Earth they can lead to geomagnetic disturbances that were not predicted by space weather forecasters. We investigate the origin and eruption of a stealth event that occurred on 2015 January 3 that was responsible for a strong geomagnetic storm upon its arrival at Earth. To simulate the coronal magnetic field and plasma parameters of the eruption we use a coupled approach. This approach combines an evolutionary nonlinear force-free field model of the global corona with a MHD simulation. The combined simulation approach accurately reproduces th…

Magnetohydrodynamics (MHD)010504 meteorology & atmospheric sciencesSun: coronal mass ejections (CMEs)FOS: Physical sciencesAstrophysics01 natural sciencesPhysics::GeophysicsAeronauticsMethods: data analysis0103 physical sciencesQB AstronomyAstrophysics::Solar and Stellar Astrophysicsdata analysis [Methods]Sun: magnetic fields010303 astronomy & astrophysicsQCSolar and Stellar Astrophysics (astro-ph.SR)QB0105 earth and related environmental sciencesPhysicsAstronomy and Astrophysics3rd-DAScoronal mass ejections (CMEs) [Sun]QC PhysicsAstrophysics - Solar and Stellar Astrophysicsmagnetic fields [Sun]13. Climate actionSpace and Planetary SciencePhysics::Space PhysicsAstronomy &amp; Astrophysics
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Modeling magnetohydrodynamics and non equilibrium SoHO/UVCS line emission of CME shocks

2008

We provide a guideline to interpret the UVCS emission lines (in particular O VI and Si XII) during shock wave propagation in the outer solar corona. We use a numerical MHD model performing a set of simulations of shock waves generated in the corona and from the result we compute the plasma emission for the O VI and Si XII including the effects of NEI. We analyze the radiative and spectral properties of our model with the support of a detailed radiation model including Doppler dimming and an analytical model for shocks, and, finally, we synthesize the expected O VI 1032A line profile. We explain several spectral features of the observations like the absence of discontinuities in the O VI emi…

PhysicsShock waveMagnetohydrodynamics (MHD)Sun: coronaSun: coronal mass ejections (CMEs)Astrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsPlasmaAstrophysicsShock (mechanics)Magnetic fieldSpace and Planetary SciencePhysics::Space PhysicsRadiative transferAstrophysics::Solar and Stellar AstrophysicsEmission spectrumMagnetohydrodynamicsAstrophysics::Galaxy AstrophysicsLine (formation)
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J/ production as a function of charged-particle pseudorapidity density in p–Pb collisions at

2017

We report measurements of the inclusive J/ψ yield and average transverse momentum as a function of charged-particle pseudorapidity density dNch/dη in p–Pb collisions at sNN=5.02TeV with ALICE at the LHC. The observables are normalised to their corresponding averages in non-single diffractive events. An increase of the normalised J/ψ yield with normalised dNch/dη, measured at mid-rapidity, is observed at mid-rapidity and backward rapidity. At forward rapidity, a saturation of the relative yield is observed for high charged-particle multiplicities. The normalised average transverse momentum at forward and backward rapidities increases with multiplicity at low multiplicities and saturates beyo…

PhysicsNuclear and High Energy PhysicsLarge Hadron Collider010308 nuclear & particles physicsMonte Carlo methodObservableMultiplicity (mathematics)01 natural sciencesCharged particleNuclear physicsPseudorapidity0103 physical sciencesTransverse momentumRapidityNuclear Experiment010306 general physicsPhysics Letters
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Modeling Magnetohydrodynamics And Non Equilibrium SoHO/UVCS Line Emission Of Cme Shocks

2007

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High Performance Computing on the COMETA Grid Infrastructure

2008

We present the High Performance Computing (HPC) projects jointly developed at the INAF - Osservatorio Astronomico di Palermo and at the DSFA - Universita` di Palermo which benefits of the Grid infrastructure of COMETA. We have contributed to setup the infrastructure in order to run HPC applications on the Grid. We report on our experience regarding to porting HPC applications to the Grid and to the first HPC simulations performed. The most demanding simulations describe the interaction of a magnetized supernova shock wave with an interstellar gas cloud. We discuss the resources required for the simulations, the performance and the scalability of our code on the Grid, and present first resul…

MagnetohydrodynamicsSettore FIS/05 - Astronomia E AstrofisicaHigh Performance ComputingHydrodynamicsAstrophysics
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Probing the physics of the solar atmosphere with the Multi-slit Solar Explorer (MUSE): I. Coronal Heating

2022

The Multi-slit Solar Explorer (MUSE) is a proposed NASA MIDEX mission, currently in Phase A, composed of a multi-slit EUV spectrograph (in three narrow spectral bands centered around 171A, 284A, and 108A) and an EUV context imager (in two narrow passbands around 195A and 304A). MUSE will provide unprecedented spectral and imaging diagnostics of the solar corona at high spatial (&lt;0.5 arcsec), and temporal resolution (down to ~0.5s) thanks to its innovative multi-slit design. By obtaining spectra in 4 bright EUV lines (Fe IX 171A , Fe XV 284A, Fe XIX-Fe XXI 108A) covering a wide range of transition region and coronal temperatures along 37 slits simultaneously, MUSE will for the first time …

F300FOS: Physical sciencesF500Astronomy & AstrophysicsACTIVE-REGIONEVENTSFLOWSSolar coronal heating Theoretical models Solar instrumentsINTERFACE-REGIONMAGNETIC RECONNECTIONQB AstronomyTRANSITION REGIONInstrumentation and Methods for Astrophysics (astro-ph.IM)Solar and Stellar Astrophysics (astro-ph.SR)QCQBMCCScience & TechnologyHOT PLASMAAstronomy and Astrophysics3rd-DASALFVENIC WAVESSIMULATIONSQC PhysicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysical SciencesEUV IMAGING SPECTROMETERAstrophysics - Instrumentation and Methods for Astrophysics
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