Search results for "Space and Planetary Science"

showing 10 items of 2189 documents

Minimum fuel control of the planar circular restricted three-body problem

2012

The circular restricted three-body problem is considered to model the dynamics of an artificial body submitted to the attraction of two planets. Minimization of the fuel consumption of the spacecraft during the transfer, e.g. from the Earth to the Moon, is considered. In the light of the controllability results of Caillau and Daoud (SIAM J Control Optim, 2012), existence for this optimal control problem is discussed under simplifying assumptions. Thanks to Pontryagin maximum principle, the properties of fuel minimizing controls is detailed, revealing a bang-bang structure which is typical of L1-minimization problems. Because of the resulting non-smoothness of the Hamiltonian two-point bound…

[ MATH.MATH-OC ] Mathematics [math]/Optimization and Control [math.OC]Lagrangian point02 engineering and technology01 natural sciences0203 mechanical engineeringControl theory0103 physical sciencesApplied mathematicsBoundary value problemCircular orbit010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSMathematical PhysicsMathematics020301 aerospace & aeronauticsApplied MathematicsConjugate points[MATH.MATH-OC] Mathematics [math]/Optimization and Control [math.OC]Astronomy and AstrophysicsOptimal controlThree-body problemControllabilityComputational MathematicsSpace and Planetary ScienceModeling and Simulation[MATH.MATH-OC]Mathematics [math]/Optimization and Control [math.OC]Hamiltonian (control theory)Celestial Mechanics and Dynamical Astronomy
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Shaken Snow Globes: Kinematic Tracers of the Multiphase Condensation Cascade in Massive Galaxies, Groups, and Clusters

2018

We propose a novel method to constrain turbulence and bulk motions in massive galaxies, groups and clusters, exploring both simulations and observations. As emerged in the recent picture of the top-down multiphase condensation, the hot gaseous halos are tightly linked to all other phases in terms of cospatiality and thermodynamics. While hot halos (10^7 K) are perturbed by subsonic turbulence, warm (10^4 K) ionized and neutral filaments condense out of the turbulent eddies. The peaks condense into cold molecular clouds (< 100 K) raining in the core via chaotic cold accretion (CCA). We show all phases are tightly linked via the ensemble (wide-aperture) velocity dispersion along the line o…

[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Astrophysics01 natural sciencesSpectral lineGalaxy groupAbsorption (logic)010303 astronomy & astrophysicsLine (formation)hydrodynamicPhysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)Velocity dispersionPhysics - Fluid DynamicsComputational Physics (physics.comp-ph)active [galaxies]astro-ph.COspectroscopic [techniques]Astrophysics - High Energy Astrophysical PhenomenaPhysics - Computational PhysicsAstrophysics - Cosmology and Nongalactic Astrophysics[ INFO ] Computer Science [cs]Cosmology and Nongalactic Astrophysics (astro-ph.CO)astro-ph.GAgalaxies: activeFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsISM [radio lines]0103 physical sciences[ PHYS.PHYS.PHYS-GEN-PH ] Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]/dk/atira/pure/subjectarea/asjc/1900/1912[INFO]Computer Science [cs]Astrophysics::Galaxy Astrophysicsradio lines: ISM010308 nuclear & particles physicsMolecular cloudturbulenceFluid Dynamics (physics.flu-dyn)Astronomy and AstrophysicsAstronomy and AstrophysicAstrophysics - Astrophysics of GalaxiesX-rays: galaxies: clusterGalaxyAccretion (astrophysics)[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]physics.flu-dynphysics.comp-phSpace and Planetary ScienceX-rays: galaxies: clustersAstrophysics of Galaxies (astro-ph.GA)hydrodynamics/dk/atira/pure/subjectarea/asjc/3100/3103galaxies: clusters [X-rays][PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]techniques: spectroscopic
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The 30 Year Search for the Compact Object in SN 1987A

2018

Despite more than 30 years of searches, the compact object in Supernova (SN) 1987A has not yet been detected. We present new limits on the compact object in SN 1987A using millimeter, near-infrared, optical, ultraviolet, and X-ray observations from ALMA, VLT, HST, and Chandra. The limits are approximately 0.1 mJy ($0.1\times 10^{-26}$ erg s$^{-1}$ cm$^{-2}$ Hz$^{-1}$) at 213 GHz, 1 Lsun ($6\times 10^{-29}$ erg s$^{-1}$ cm$^{-2}$ Hz$^{-1}$) in optical if our line-of-sight is free of ejecta dust, and $10^{36}$ erg s$^{-1}$ ($2\times 10^{-30}$ erg s$^{-1}$ cm$^{-2}$ Hz$^{-1}$) in 2-10 keV X-rays. Our X-ray limits are an order of magnitude less constraining than previous limits because we use a…

[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]AstrophysicsPhysical Chemistry01 natural sciences7. Clean energyAtomicLuminosityParticle and Plasma PhysicsQB460Astrophysics::Solar and Stellar AstrophysicsAbsorption (logic)10. No inequality010303 astronomy & astrophysicsQBHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HEAccretion (meteorology)SUPERNOVA REMNANT 1987ASupernovaAstrophysics - High Energy Astrophysical PhenomenaAstronomical and Space SciencesPhysical Chemistry (incl. Structural)NEUTRON-STARSCIRCUMSTELLAR RINGX-RAYSAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesBLUE SUPERGIANTSAstrophysics::Cosmology and Extragalactic AstrophysicsCompact starAstronomy & Astrophysicsstars: neutronneutron [stars]Pulsarindividual [supernovae]0103 physical sciencesblack holes [stars]NuclearINTEGRAL FIELD SPECTROSCOPY010306 general physicsUNDERGROUND SCINTILLATION TELESCOPEsupernovae: individualAstrophysics::Galaxy AstrophysicsOrganic ChemistryMolecularAstronomy and AstrophysicsHUBBLE-SPACE-TELESCOPEEffective temperatureNeutron starRAY EMISSION-LINESPhysics and Astronomyindividual (SN 1987A) [supernovae]13. Climate actionSpace and Planetary ScienceLARGE-MAGELLANIC-CLOUD[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]stars: black holes
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A Hard Look at the Neutron Stars and Accretion Disks in 4U 1636-53, GX 17+2, and 4U 1705-44 with NuStar

2017

We present $\emph{NuSTAR}$ observations of neutron star (NS) low-mass X-ray binaries: 4U 1636-53, GX 17+2, and 4U 1705-44. We observed 4U 1636-53 in the hard state, with an Eddington fraction, $F_{\mathrm{Edd}}$, of 0.01; GX 17+2 and 4U 1705-44 were in the soft state with fractions of 0.57 and 0.10, respectively. Each spectrum shows evidence for a relativistically broadened Fe K$_{\alpha}$ line. Through accretion disk reflection modeling, we constrain the radius of the inner disk in 4U 1636-53 to be $R_{in}=1.03\pm0.03$ ISCO (innermost stable circular orbit) assuming a dimensionless spin parameter $a_{*}=cJ/GM^{2}=0.0$, and $R_{in}=1.08\pm0.06$ ISCO for $a_{*}=0.3$ (errors quoted at 1 $\sig…

[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]FOS: Physical sciencesAstrophysics01 natural sciencesstars: neutronX-rays: binariesSettore FIS/05 - Astronomia E Astrofisicaaccretion0103 physical sciencesaccretion accretion disks stars: neutron X-rays: binaries X-rays: individual: 4U 1636-53 GX 17+2 4U 1705-44010303 astronomy & astrophysicsLine (formation)Spin-½PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Accretion (meteorology)010308 nuclear & particles physicsEquation of state (cosmology)neutron X-rays: binaries X-rays: individual: 4U 1636-53 GX 17+2 4U 1705-44 [accretion accretion disks stars]accretion disksAstronomy and AstrophysicsRadiusNeutron starReflection (mathematics)Space and Planetary Science[SDU]Sciences of the Universe [physics]Astrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]X-rays: individualDimensionless quantity
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Recent changes in measured wind in the NE Atlantic and variability of correlation with NAO

2010

The paper deals with wind measurements, recorded since the 1950s, at twelve meteorological stations along a transect near the westernmost European border, between 64° and 44° N. Extreme wind speed tends to decrease sharply near the northern boundary (at Reykjavick), near the middle of the study area (at Shannon and Valentia) and near the southern boundary (at Brest and Cap Ferret), to increase at Thorshavn, with less significant trends at the other stations. Average wind speeds confirm the above tendencies, with an additional increasing speed at Lerwick, Kirkwall, Malin Head, Belle-Ile and Cap Ferret. To compare changes in wind activity, the data have been subdivided into three periods: unt…

[ SDU.OCEAN ] Sciences of the Universe [physics]/Ocean AtmosphereAtmospheric Science010504 meteorology & atmospheric sciencesCorrelation coefficientMeteorologyKeywords. Meteorology and atmospheric dynamics (Climatology[SDE.MCG]Environmental Sciences/Global Changes010502 geochemistry & geophysics01 natural sciencesWind speedLatitudeKeywords. Meteorology and atmospheric dynamics (Climatology; General circulation)Trend surface analysisEarth and Planetary Sciences (miscellaneous)lcsh:ScienceTransectExtreme value theory0105 earth and related environmental sciences[SDU.OCEAN]Sciences of the Universe [physics]/Ocean AtmosphereClimatologyAtmospheric dynamicsGeneral circulationlcsh:QC801-809General circulation)GeologyAstronomy and AstrophysicsWesterlieslcsh:QC1-999lcsh:Geophysics. Cosmic physics[ SDE.MCG ] Environmental Sciences/Global Changes[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/Climatology13. Climate actionSpace and Planetary ScienceNorth Atlantic oscillationClimatologylcsh:Q[ SDU.STU.CL ] Sciences of the Universe [physics]/Earth Sciences/Climatologylcsh:PhysicsGeologyAnnales Geophysicae
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Global atmospheric response to specific linear combinations of the main SST modes. Part I: numerical experiments and preliminary results

1996

Abstract. This article investigates through numerical experiments the controversial question of the impact of El Niño-Southern Oscillation (ENSO) phenomena on climate according to large-scale and regional-scale interhemispheric thermal contrast. Eight experiments (two considering only inversed Atlantic thermal anomalies and six combining ENSO warm phase with large-scale interhemispheric contrast and Atlantic anomaly patterns) were performed with the Météo-France atmospheric general circulation model. The definition of boundary conditions from observed composites and principal components is presented and preliminary results concerning the month of August, especially over West Africa and the …

[ SDU.OCEAN ] Sciences of the Universe [physics]/Ocean AtmosphereAtmospheric Science010504 meteorology & atmospheric sciencesMeteorologyAtmospheric circulation010502 geochemistry & geophysics01 natural sciencesWest africaEarth and Planetary Sciences (miscellaneous)Linear combinationlcsh:ScienceSouthern Hemisphere0105 earth and related environmental sciences[SDU.OCEAN]Sciences of the Universe [physics]/Ocean AtmosphereAnomaly (natural sciences)lcsh:QC801-809Northern HemisphereGeologyAstronomy and Astrophysics[ SDU.STU ] Sciences of the Universe [physics]/Earth Scienceslcsh:QC1-999lcsh:Geophysics. Cosmic physicsEl Niño Southern Oscillation13. Climate actionSpace and Planetary Science[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/ClimatologyGeneral Circulation ModelClimatologyEnvironmental sciencelcsh:Qlcsh:Physics
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The relationship between the Sahelian and previous 2nd Guinean rainy seasons: a monsoon regulation by soil wetness?

2002

The correlation of 0.61 found between observed July–September Sahelian rainfall in year 0 and September–November Guinean rainfall in year - 1, led us to explore the statistical relationships between precipitation, soil moisture and near surface Moist Static Energy (MSE) gradients in West Africa. These analyses were performed over successive 30-year periods and specifically, the most recent period between 1968–1998. It is shown from observations, National Centers for Environmental Predictions and National Center for Atmospheric Research (NCEP/NCAR) reanalyses and from the Global Soil Wetness Project (GSWP) database, that wet Sahelian rainy seasons are preceded by abnormally wet soils over th…

[ SDU.OCEAN ] Sciences of the Universe [physics]/Ocean AtmosphereAtmospheric ScienceMeteorologyMonsoonAtmospheric sciencesHydrology (agriculture)Dry seasonEarth and Planetary Sciences (miscellaneous)Moist static energyPrecipitationlcsh:ScienceWater contentMoisture[SDU.OCEAN] Sciences of the Universe [physics]/Ocean Atmospherelcsh:QC801-809GeologyAstronomy and Astrophysics[ SDU.STU ] Sciences of the Universe [physics]/Earth Scienceslcsh:QC1-999lcsh:Geophysics. Cosmic physicsSpace and Planetary ScienceSoil water[SDU.STU] Sciences of the Universe [physics]/Earth SciencesEnvironmental sciencelcsh:Qlcsh:PhysicsAnnales Geophysicae
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Foreword for the thematic volume of the 8ISCPP. Recent advances in present and past cephalopod studies.

2012

3 pages, éditorial.; International audience

[ SDV.BID ] Life Sciences [q-bio]/Biodiversity010506 paleontology[ SDE.BE ] Environmental Sciences/Biodiversity and EcologybiologyPaleontology[SDV.BID]Life Sciences [q-bio]/Biodiversity010502 geochemistry & geophysicsbiology.organism_classification01 natural sciencesCephalopod[SDE.BE] Environmental Sciences/Biodiversity and EcologyOceanographyThematic mapGeographySpace and Planetary Science[SDU.STU.PG] Sciences of the Universe [physics]/Earth Sciences/Paleontology[SDE.BE]Environmental Sciences/Biodiversity and Ecology[SDU.STU.PG]Sciences of the Universe [physics]/Earth Sciences/Paleontology0105 earth and related environmental sciencesVolume (compression)[SDV.BID] Life Sciences [q-bio]/Biodiversity[ SDU.STU.PG ] Sciences of the Universe [physics]/Earth Sciences/Paleontology
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Constraints on the origin of cosmic rays above 10^18 eV from large-scale anisotropy searches in data of the Pierre Auger Observatory

2012

A thorough search for large-scale anisotropies in the distribution of arrival directions of cosmic rays detected above 10(18) eV at the Pierre Auger Observatory is reported. For the first time, these large-scale anisotropy searches are performed as a function of both the right ascension and the declination and expressed in terms of dipole and quadrupole moments. Within the systematic uncertainties, no significant deviation from isotropy is revealed. Upper limits on dipole and quadrupole amplitudes are derived under the hypothesis that any cosmic ray anisotropy is dominated by such moments in this energy range. These upper limits provide constraints on the production of cosmic rays above 10(…

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]AstronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysics01 natural sciencesMAGNETIC-FIELDScosmic raysObservatory0103 physical sciencesUltra-high-energy cosmic rayAnisotropyastroparticle physics – cosmic rays010303 astronomy & astrophysicsCiencias ExactasHigh Energy Astrophysical Phenomena (astro-ph.HE)Pierre Auger ObservatoryAstroparticle physicsPhysicsCOSMIC cancer database010308 nuclear & particles physicsOBSERVATÓRIOS[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsAstronomyastroparticle physicFísicaAstronomy and AstrophysicsRadiación cósmica13. Climate actionSpace and Planetary Scienceastroparticle physicsExperimental High Energy PhysicsQuadrupoleComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica de partículasFísica nuclearAstroparticle physicsAstrophysics - High Energy Astrophysical Phenomena
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γ-RAY AND PARSEC-SCALE JET PROPERTIES OF A COMPLETE SAMPLE OF BLAZARS FROM THE MOJAVE PROGRAM

2011

著者人数: 145名

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Cosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical Phenomenagalaxies: activePopulationFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesRadio spectrumLuminosityRelativistic beamingquasars: generalgamma rays: galaxiesgalaxies0103 physical sciencesgalaxie [gamma rays]educationBlazar010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)radio continuum: galaxiesPhysicseducation.field_of_studygeneral [quasars]general [BL Lacertae objects]010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astronomy and AstrophysicsQuasarBL Lacertae objects: generalgalaxies: jetsgalaxies [radio continuum]BL Lacertae objects: general; galaxies: active; galaxies: jets; gamma rays: galaxies; quasars: general; galaxies quasars: generaljet [galaxies]BL Lacertae objects: general; galaxies: active; galaxies: jets; gamma rays: galaxies; quasars: general; radio continuum: galaxiesSpace and Planetary Scienceactive [galaxies]Spectral energy distributionAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic AstrophysicsFermi Gamma-ray Space TelescopeThe Astrophysical Journal
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