Search results for "physics.space-ph"

showing 10 items of 22 documents

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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Radio emissions from double RHESSI TGFs

2016

Abstract A detailed analysis of Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) terrestrial gamma ray flashes (TGFs) is performed in association with World Wide Lightning Location Network (WWLLN) sources and very low frequency (VLF) sferics recorded at Duke University. RHESSI clock offset is evaluated and found to experience changes on the 5 August 2005 and 21 October 2013, based on the analysis of TGF‐WWLLN matches. The clock offsets were found for all three periods of observations with standard deviations less than 100 μs. This result opens the possibility for the precise comparative analyses of RHESSI TGFs with the other types of data (WWLLN, radio measurements, etc.) In ca…

Atmospheric ScienceHigh energy010504 meteorology & atmospheric sciencesAtmospheric ElectricityFOS: Physical sciencesRHESSI clock offsetterrestrial gamma ray flashesAstrophysicsRadio atmospheric01 natural sciencesLightningPhysical Geography and Environmental GeoscienceAerosol and CloudsAtmospheric SciencesRemote SensingPhysics - Space Physics0103 physical sciencesEarth and Planetary Sciences (miscellaneous)Instruments and TechniquesVery low frequency010303 astronomy & astrophysicsResearch ArticlesTGF‐WWLLN match0105 earth and related environmental sciencesRadiative ProcessesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Remote Sensing and DisastersGamma raymultipeak TGFsWorld wideLightningRHESSI TGFsSpace Physics (physics.space-ph)Geophysicsradio emission from TGFClock offset13. Climate actionSpace and Planetary ScienceAtmospheric ProcessesAstrophysics - High Energy Astrophysical PhenomenaNatural HazardsResearch Article
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Application of spin-exchange relaxation-free magnetometry to the Cosmic Axion Spin Precession Experiment

2018

The Cosmic Axion Spin Precession Experiment (CASPEr) seeks to measure oscillating torques on nuclear spins caused by axion or axion-like-particle (ALP) dark matter via nuclear magnetic resonance (NMR) techniques. A sample spin-polarized along a leading magnetic field experiences a resonance when the Larmor frequency matches the axion/ALP Compton frequency, generating precessing transverse nuclear magnetization. Here we demonstrate a Spin-Exchange Relaxation-Free (SERF) magnetometer with sensitivity $\approx 1~{\rm fT/\sqrt{Hz}}$ and an effective sensing volume of 0.1 $\rm{cm^3}$ that may be useful for NMR detection in CASPEr. A potential drawback of SERF-magnetometer-based NMR detection is …

Physics - Instrumentation and DetectorsMagnetometerAtomic Physics (physics.atom-ph)FOS: Physical sciences01 natural sciences7. Clean energylaw.inventionPhysics - Atomic Physics010309 opticsMagnetizationPhysics - Space Physicslaw0103 physical sciences010306 general physicsAxionLarmor precessionPhysicsSpinsAstronomy and AstrophysicsInstrumentation and Detectors (physics.ins-det)Magnetic fluxSpace Physics (physics.space-ph)Magnetic fieldSpace and Planetary SciencePrecessionAtomic physicsPhysics of the Dark Universe
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Limiting P-odd interactions of cosmic fields with electrons, protons and neutrons

2014

We propose methods for extracting limits on the strength of P-odd interactions of pseudoscalar and pseudovector cosmic fields with electrons, protons and neutrons. Candidates for such fields are dark matter (including axions) and dark energy, as well as several more exotic sources described by standard-model extensions. Calculations of parity nonconserving amplitudes and atomic electric dipole moments induced by these fields are performed for H, Li, Na, K, Rb, Cs, Ba+, Tl, Dy, Fr, and Ra+. From these calculations and existing measurements in Dy, Cs and Tl, we constrain the interaction strengths of the parity-violating static pseudovector cosmic field to be 7*10^(-15) GeV with an electron, a…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Field (physics)ProtonNuclear TheoryAtomic Physics (physics.atom-ph)Dark matterNuclear TheoryGeneral Physics and AstronomyFOS: Physical sciencesElectronSpace Physics (physics.space-ph)Physics - Atomic PhysicsNuclear physicsPseudoscalarNuclear Theory (nucl-th)DipoleHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Physics - Space PhysicsNeutronPseudovectorAstrophysics - Cosmology and Nongalactic Astrophysics
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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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Report of the COSPAR Mars special regions colloquium

2010

International audience; In this paper we present the findings of a COSPAR Mars Special Regions Colloquium held in Rome in 2007. We review and discuss the definition of Mars Special Regions, the physical parameters used to define Mars Special Regions, and physical features on Mars that can be interpreted as Mars Special Regions. We conclude that any region experiencing temperatures > -25 degrees C for a few hours a year and a water activity > 0.5 can potentially allow the replication of terrestrial microorganisms. Physical features on Mars that can be interpreted as meeting these conditions constitute a Mars Special Region. Based on current knowledge of the martian environment and the conser…

Atmospheric Science010504 meteorology & atmospheric sciencesPlanetary protectionLiquid waterAerospace EngineeringTerrainBACTERIAL-ACTIVITY01 natural sciencesSPACECRAFT SURFACESAstrobiologyWater-vaporSouth-pole snow0103 physical sciencesBacterial activitySpace research010303 astronomy & astrophysicsBacterial activity0105 earth and related environmental sciencesMartianCommittee on Space ResearchCOSPAR mars special regions colloquiumNear-surfaceAstronomy and AstrophysicsMars Exploration Program15. Life on landGround ice[PHYS.PHYS.PHYS-SPACE-PH]Physics [physics]/Physics [physics]/Space Physics [physics.space-ph]GeophysicsLiquid water13. Climate actionSpace and Planetary ScienceGeneral Earth and Planetary SciencesHigh obliquitySea-iceUpper martian surfaceSpace-craft surfacesGeology
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Radiation Hardness Assurance Through System-Level Testing: Risk Acceptance, Facility Requirements, Test Methodology, and Data Exploitation

2021

International audience; Functional verification schemes at a level different from component-level testing are emerging as a cost-effective tool for those space systems for which the risk associated with a lower level of assurance can be accepted. Despite the promising potential, system-level radiation testing can be applied to the functional verification of systems under restricted intrinsic boundaries. Most of them are related to the use of hadrons as opposed to heavy ions. Hadrons are preferred for the irradiation of any bulky system, in general, because of their deeper penetration capabilities. General guidelines about the test preparation and procedure for a high-level radiation test ar…

Small satelllitessmall satellitesComputer scienceRadiation effects02 engineering and technologytest methodology01 natural sciencesSpace missionsSpace explorationsystem-level testing0202 electrical engineering electronic engineering information engineeringRadiation hardeningTechnik [600]Reliability (statistics)avaruustekniikka[PHYS]Physics [physics]protonselektroniikkalaitteetrisk acceptance[PHYS.PHYS.PHYS-SPACE-PH]Physics [physics]/Physics [physics]/Space Physics [physics.space-ph]Commercial off-the-shelf (COTS)Test (assessment)facilitiesPerformance evaluationTotal ionizing doseSystem verificationtestmethodologyNuclear and High Energy Physicstotal ionizing dose (TID)0103 physical scienceselektroniikkaRadiation hardening (electronics)Electrical and Electronic Engineeringsingle-event effect (SEE)Functional verification010308 nuclear & particles physics600: Technikneutrons020206 networking & telecommunicationsTest methodSystem level testingReliability engineering[SPI.TRON]Engineering Sciences [physics]/ElectronicsNuclear Energy and EngineeringtestausmenetelmätsäteilyfysiikkaOrbit (dynamics)radiation hardness assurancejärjestelmätddc:600
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Parity-violating interactions of cosmic fields with atoms, molecules, and nuclei: Concepts and calculations for laboratory searches and extracting li…

2014

We propose methods and present calculations that can be used to search for evidence of cosmic fields by investigating the parity-violating effects, including parity nonconservation amplitudes and electric dipole moments, that they induce in atoms. The results are used to constrain important fundamental parameters describing the strength of the interaction of various cosmic fields with electrons, protons, and neutrons. Candidates for such fields are dark matter (including axions) and dark energy, as well as several more exotic sources described by standard-model extensions. Existing parity nonconservation experiments in Cs, Dy, Yb, and Tl are combined with our calculations to directly place …

Nuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Nuclear TheoryAtomic Physics (physics.atom-ph)Dark matterFOS: Physical sciencesCosmic rayElectron01 natural sciencesPhysics - Atomic PhysicsNuclear physicsNuclear Theory (nucl-th)High Energy Physics - Phenomenology (hep-ph)Physics - Space Physics0103 physical sciencesNeutron010306 general physicsNuclear ExperimentPseudovectorPhysics010308 nuclear & particles physicsSpace Physics (physics.space-ph)PseudoscalarDipoleHigh Energy Physics - PhenomenologyNucleonAstrophysics - Cosmology and Nongalactic Astrophysics
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Enhanced detection of terrestrial gamma-ray flashes by AGILE

2015

Abstract At the end of March 2015 the onboard software configuration of the Astrorivelatore Gamma a Immagini Leggero (AGILE) satellite was modified in order to disable the veto signal of the anticoincidence shield for the minicalorimeter instrument. The motivation for such a change was the understanding that the dead time induced by the anticoincidence prevented the detection of a large fraction of Terrestrial Gamma‐Ray Flashes (TGFs). The configuration change was highly successful resulting in an increase of one order of magnitude in TGF detection rate. As expected, the largest fraction of the new events has short duration (<100 μs), and part of them has simultaneous association with light…

High Energy Astrophysical Phenomena (astro-ph.HE)Solar Physics Astrophysics and AstronomyAtmospheric ScienceFOS: Physical sciencesterrestrial gamma-ray flashesterrestrial gamma‐ray flashesatmospheric electricity; terrestrial gamma-ray flashesTGFSpace Physics (physics.space-ph)LightningResearch Lettersatmospheric electricityPhysics - Space PhysicsAtmospheric ProcessesResearch Letter:Matematikk og Naturvitenskap: 400 [VDP]Instruments and TechniquesAGILE TGFAstrophysics - High Energy Astrophysical Phenomena
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Aalto-1, multi-payload CubeSat: Design, integration and launch

2021

The design, integration, testing, and launch of the first Finnish satellite Aalto-1 is briefly presented in this paper. Aalto-1, a three-unit CubeSat, launched into Sun-synchronous polar orbit at an altitude of approximately 500 km, is operational since June 2017. It carries three experimental payloads: Aalto Spectral Imager (AaSI), Radiation Monitor (RADMON), and Electrostatic Plasma Brake (EPB). AaSI is a hyperspectral imager in visible and near-infrared (NIR) wavelength bands, RADMON is an energetic particle detector and EPB is a de-orbiting technology demonstration payload. The platform was designed to accommodate multiple payloads while ensuring sufficient data, power, radio, mechanica…

Computer sciencePolar orbitFOS: Physical sciencesAerospace Engineering02 engineering and technologyDesign strategy01 natural sciences7. Clean energyPhysics - Space Physicsmittauslaitteet0203 mechanical engineering0103 physical sciencesBrakeAalto-1CubeSatGround segmentAerospace engineeringInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsavaruustekniikkaAalto spectral imagerRadiation monitortutkimussatelliitit020301 aerospace & aeronauticsRadiationSpacecraftbusiness.industryPayloadCubeSatElectrostatic plasma brakesäteilySpace Physics (physics.space-ph)satelliititHyperspectralSatelliteAstrophysics - Instrumentation and Methods for Astrophysicsbusinesskosminen säteily
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