Search results for "Planet"

showing 10 items of 5662 documents

Geometric and numerical techniques in optimal control of the two and three-body problems

2009

The objective of this article is to present geometric and numerical techniques developed to study the orbit transfer between Keplerian elliptic orbits in the two-body problem or between quasi-Keplerian orbits in the Earth-Moon transfer when low propulsion is used. We concentrate our study on the energy minimization problem. From Pontryagin's maximum principle, the optimal solution can be found solving the shooting equation for smooth Hamiltonian dynamics. A first step in the analysis is to find in the Kepler case an analytical solution for the averaged Hamiltonian, which corresponds to a Riemannian metric. This will allow to compute the solution for the original Kepler problem, using a nume…

[ MATH.MATH-OC ] Mathematics [math]/Optimization and Control [math.OC][MATH.MATH-OC] Mathematics [math]/Optimization and Control [math.OC][MATH.MATH-OC]Mathematics [math]/Optimization and Control [math.OC]Astrophysics::Earth and Planetary Astrophysics
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Conjugate and cut loci in averaged orbital transfer

2006

The objective of this Note is to describe the conjugate and cut loci associated with the averaged energy minimization problem in coplanar orbit transfer.

[ MATH.MATH-OC ] Mathematics [math]/Optimization and Control [math.OC]genetic structures[MATH.MATH-OC] Mathematics [math]/Optimization and Control [math.OC][MATH.MATH-OC]Mathematics [math]/Optimization and Control [math.OC]Astrophysics::Earth and Planetary AstrophysicsQuantitative Biology::Genomicseye diseases
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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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Using of a uncertainty model of an polyarticulated coordinates measuring arm to validate the measurement in a manufacturing processsus

2014

International audience; Coordinates Measuring Arms (CMA) are increasingly used to control industrial parts and are often an alternative to CMM controls that require conditions of laboratory measurement and involve significant costs. However, the control of uncertainties is often not guaranteed because the measurement process is complex and there is no standard for setting a framework qualification process of the measurement process.The proposed study, in this paper, is a first approach to model the measurement uncertainties of a CMA with contact sensor. The problem is complex because there are many sources of uncertainty, largely due to variability in the handling carried out by the operato…

[ SPI.MECA.GEME ] Engineering Sciences [physics]/Mechanics [physics.med-ph]/Mechanical engineering [physics.class-ph]0209 industrial biotechnologyEngineeringMonte Carlo method02 engineering and technologyMetrology01 natural sciences010309 opticsCMA Modelling020901 industrial engineering & automationOperator (computer programming)Control theory0103 physical sciencesCalibration[SPI.MECA.GEME] Engineering Sciences [physics]/Mechanics [physics.med-ph]/Mechanical engineering [physics.class-ph]SimulationGeneral Environmental Sciencebusiness.industryProcess (computing)UncertaintyCovarianceMetrology[SPI.MECA.GEME]Engineering Sciences [physics]/Mechanics [physics.med-ph]/Mechanical engineering [physics.class-ph]NoiseGeneral Earth and Planetary SciencesbusinessEncoderMonte Carlo Method
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