Search results for "Earth"

showing 10 items of 12204 documents

XMM-Newton observation of the supernova remnant Kes 78 (G32.8-0.1): Evidence for shock-cloud interaction

2017

The Galactic supernova remnant Kes 78 is surrounded by dense molecular clouds, whose projected position overlaps with the extended HESS gamma-ray source HESS J1852-000. The X-ray emission from the remnant has been recently revealed by Suzaku observations, which have shown indications for a hard X-ray component in the spectra, possibly associated with synchrotron radiation. We aim at describing the spatial distribution of the physical properties of the X-ray emitting plasma and at revealing the effects of the interaction of the remnant with the inhomogeneous ambient medium. We also aim at investigating the origin of the gamma-ray emission, which may be Inverse Compton radiation associated wi…

010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaHadronSynchrotron radiationFOS: Physical sciencesElectronAstrophysicsISM: individual objects: Kes 7801 natural sciencesSpectral linelaw.inventionlawISM: cloud0103 physical sciencesSupernova remnant010303 astronomy & astrophysicsISM: supernova remnantAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Molecular cloudAstronomy and AstrophysicsPlasmaAstronomy and AstrophysicAcceleration of particleSynchrotronX-rays: ISM13. Climate actionSpace and Planetary ScienceAstrophysics - High Energy Astrophysical Phenomena
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First light observations of the solar wind in the outer corona with the Metis coronagraph

2021

In this work, we present an investigation of the wind in the solar corona that has been initiated by observations of the resonantly scattered ultraviolet emission of the coronal plasma obtained with UVCS-SOHO, designed to measure the wind outflow speed by applying Doppler dimming diagnostics. Metis on Solar Orbiter complements the UVCS spectroscopic observations that were performed during solar activity cycle 23 by simultaneously imaging the polarized visible light and the H I Lyman-α corona in order to obtain high spatial and temporal resolution maps of the outward velocity of the continuously expanding solar atmosphere. The Metis observations, taken on May 15, 2020, provide the first H I …

010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaSolar windFOS: Physical sciencesAstrophysics01 natural sciencesWind speedlaw.inventionsymbols.namesakeSun: corona – solar wind – Sun: UV radiationlaw0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsCoronagraphSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesPhysics[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]Sun: coronaAstronomy and AstrophysicsPlasmaSolar wind Sun: corona Sun: UV radiationSun: UV radiationCoronaSolar windAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceTemporal resolutionPhysics::Space PhysicssymbolsOutflowDoppler effect
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Deep XMM-Newton Observations Reveal the Origin of Recombining Plasma in the Supernova Remnant W44

2019

Recent X-ray studies revealed over-ionized recombining plasmas (RPs) in a dozen mixed-morphology (MM) supernova remnants (SNRs). However, the physical process of the over-ionization has not been fully understood yet. Here we report on spatially resolved spectroscopy of X-ray emission from W44, one of the over-ionized MM-SNRs, using XMM-Newton data from deep observations, aiming to clarify the physical origin of the over-ionization. We find that combination of low electron temperature and low recombination timescale is achieved in the region interacting with dense molecular clouds. Moreover, a clear anti-correlation between the electron temperature and the recombining timescale is obtained f…

010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaSupernova remnants (1667)FOS: Physical sciencesAstrophysicsMolecular cloud01 natural sciencesX-ray astronomySettore FIS/05 - Astronomia E AstrofisicaPlasma astrophysics (1261)Supernova remnant0103 physical sciencesPlasma astrophysicsSupernova remnantAdiabatic processSpectroscopy010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsX-ray astronomyMolecular cloudAstronomy and AstrophysicsPlasmaSupernovaSpace and Planetary ScienceMolecular clouds (1072)Electron temperatureX-ray astronomy (1810)Astrophysics - High Energy Astrophysical PhenomenaThe Astrophysical Journal
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IGR J17329-2731: The birth of a symbiotic X-ray binary

2018

We report on the results of the multiwavelength campaign carried out after the discovery of the INTEGRAL transient IGR J17329-2731. The optical data collected with the SOAR telescope allowed us to identify the donor star in this system as a late M giant at a distance of 2.7$^{+3.4}_{-1.2}$ kpc. The data collected quasi-simultaneously with XMM-Newton and NuSTAR showed the presence of a modulation with a period of 6680$\pm$3 s in the X-ray light curves of the source. This unveils that the compact object hosted in this system is a slowly rotating neutron star. The broadband X-ray spectrum showed the presence of a strong absorption ($\gg$10$^{23}$ cm$^{-2}$) and prominent emission lines at 6.4 …

010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaX-ray binaryFOS: Physical sciencesFluxAstrophysicsCompact star01 natural sciencesSpectral linelaw.inventionTelescopeSettore FIS/05 - Astronomia E Astrofisicalaw0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsEmission spectrum010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAstronomy and AstrophysicsAstronomy and AstrophysicLight curveX-rays: binarieNeutron starX-rays: individuals: IGR J17329-273113. Climate actionSpace and Planetary ScienceAstrophysics - High Energy Astrophysical Phenomena
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Inter-annual climate variability in Europe during the Oligocene icehouse

2017

Abstract New sclerochronological data suggest that a variability comparable to the North Atlantic Oscillation (NAO) was already present during the middle Oligocene, about 20 Myr earlier than formerly assumed. Annual increment width data of long-lived marine bivalves of Oligocene (30–25 Ma) strata from Central Europe revealed a distinct quasi-decadal climate variability modulated on 2–12 (mainly 3–7) year cycles. As in many other modern bivalves, these periodic changes in shell growth were most likely related to changes in primary productivity, which in turn, were coupled to atmospheric circulation patterns. Stable carbon isotope values of the shells (δ 13 C shell ) further corroborated the …

010504 meteorology & atmospheric sciencesAtmospheric circulationPaleontology010502 geochemistry & geophysicsOceanography01 natural sciencesProxy (climate)Oceanography13. Climate actionNorth Atlantic oscillationIsotopes of carbonSclerochronologyClimatologyClimate model14. Life underwaterClimate stateCenozoicEcology Evolution Behavior and SystematicsGeology0105 earth and related environmental sciencesEarth-Surface ProcessesPalaeogeography, Palaeoclimatology, Palaeoecology
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Coastal precipitation regimes in Kenya.

1997

Kenya is under the influence of the seasonal reversal of the Indian ocean monsoons. However, its coastal belt, up to about 50 km inland, exhibits original climatic features. Hierarchical clustering...

010504 meteorology & atmospheric sciencesAtmospheric circulation[SHS.GEO] Humanities and Social Sciences/GeographyGeography Planning and Development0207 environmental engineeringSoil resilienceGeology02 engineering and technology[SHS.GEO]Humanities and Social Sciences/GeographySeasonality010502 geochemistry & geophysicsMonsoonmedicine.disease01 natural sciences[ SHS.GEO ] Humanities and Social Sciences/GeographyIndian oceanSea breeze13. Climate actionClimatologymedicineEnvironmental sciencePrecipitationSurface runoff020701 environmental engineering0105 earth and related environmental sciences
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Simulated European stalagmite record and its relation to a quasi-decadal climate mode

2013

Abstract. A synthetic stalagmite record for the Bunker cave is constructed using a combined climate-stalagmite modeling approach. The power spectrum of the simulated speleothem calcite δ18O record has a pronounced peak at quasi-decadal time scale. Interestingly, mixing processes in the soil and karst above the cave represent a natural low-pass filter of the speleothem climate archive. We identify a quasi-decadal mode characterized by a "tripole pattern" of sea surface temperature affecting stalagmite δ18O values. This pattern, which is well-known in literature as the quasi-decadal mode in the North Atlantic, propagates eastwards and affects western European temperature surrounding the cave.…

010504 meteorology & atmospheric sciencesAtmospheric circulationδ18OStratigraphylcsh:Environmental protectionSpeleothemStalagmite010502 geochemistry & geophysics01 natural scienceschemistry.chemical_compound03 medical and health sciencesCavelcsh:Environmental pollutionlcsh:TD169-171.8lcsh:Environmental sciences030304 developmental biology0105 earth and related environmental sciencesCalcitelcsh:GE1-350Global and Planetary Changegeography0303 health sciencesgeography.geographical_feature_categoryPaleontologyKarstchemistry13. Climate actionClimatologylcsh:TD172-193.5GeologyTeleconnectionClimate of the Past
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Optimized Class-Separability in Hyperspectral Images

2016

International audience; Image visualization techniques are mostly based on three bands as RGB color composite channels for human eye to characterize the scene. This, however, is not effective in case of hyper-spectral images (HSI) because they contain dozens of informative spectral bands. To eliminate redundancy of spectral information among these bands, dimensionality reduction (DR) is applied while at the same trying to retain maximum information. In this paper, we propose a new method of information-preserved hyper-spectral satellite image visualization that is based on fusion of unsupervised band selection techniques and color matching function (CMF) stretching. The results show consist…

010504 meteorology & atmospheric sciencesBand SelectionComputer science0211 other engineering and technologiesComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISION[SDU.STU]Sciences of the Universe [physics]/Earth Sciences02 engineering and technology[ SPI.SIGNAL ] Engineering Sciences [physics]/Signal and Image processing01 natural sciencesTransformation[SPI]Engineering Sciences [physics][ SPI.NRJ ] Engineering Sciences [physics]/Electric powerDisplay[ SPI ] Engineering Sciences [physics]Computer visionclass separabilityFusion021101 geological & geomatics engineering0105 earth and related environmental sciencesColor imagebusiness.industry[SPI.NRJ]Engineering Sciences [physics]/Electric powerHyperspectral imagingPattern recognition[ SDU.STU ] Sciences of the Universe [physics]/Earth SciencesImage segmentationSpectral bandsDimensionality reductionVisualization[SPI.TRON]Engineering Sciences [physics]/Electronics[ SPI.TRON ] Engineering Sciences [physics]/ElectronicsImaging spectroscopyFull spectral imagingRGB color modelArtificial intelligencehyper-spectral image visualizationbusiness[SPI.SIGNAL]Engineering Sciences [physics]/Signal and Image processing
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Strombolian eruptions and dynamics of magma degassing at Yasur Volcano (Vanuatu)

2020

Abstract Open vent basaltic volcanoes account for a substantial portion of the global atmospheric outgassing flux, largely through passive degassing and mild explosive activity. We present volcanic gas flux and composition data from Yasur Volcano, Vanuatu collected in July 2018. The average volcanic plume chemistry is characterised by a mean molar CO2/SO2 ratio of 2.14, H2O/SO2 of 148 and SO2/HCl of 1.02. The measured mean SO2 flux in the period of 6th to 9th July is 4.9 kg s−1. Therefore, the mean fluxes of the other species are 7.5 kg∙s−1 CO2, 208 kg∙s−1 H2O and 4.8 kg∙s−1 HCl. The degassing regime at Yasur volcano ranges from ‘passive’ to ‘active’ styles, with the latter including Stromb…

010504 meteorology & atmospheric sciencesBasaltic open vent volcanoessub-05Gas fluxes010502 geochemistry & geophysics01 natural sciencesStrombolian activityFlux (metallurgy)Geochemistry and PetrologyCrystal content in magmaPetrology0105 earth and related environmental sciencesBasaltgeographygeography.geographical_feature_categoryBasaltic open vent volcanoes Crystal content in magma Gas fluxes Magma fluxes Strombolian activity YasurStrombolian eruptionMagma fluxesOutgassingGeophysicsVolcanoVolcanic plumeMagmaInclusion (mineral)YasurGeology
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Photometric variability of the Be star CoRoT-ID 102761769

2010

Classical Be stars are rapid rotators of spectral type late O to early A and luminosity class V-III, wich exhibit Balmer emission lines and often a near infrared excess originating in an equatorially concentrated circumstellar envelope, both produced by sporadic mass ejection episodes. The causes of the abnormal mass loss (the so-called Be phenomenon) are as yet unknown. For the first time, we can now study in detail Be stars outside the Earth's atmosphere with sufficient temporal resolution. We investigate the variability of the Be Star CoRoT-ID 102761769 observed with the CoRoT satellite in the exoplanet field during the initial run. One low-resolution spectrum of the star was obtained wi…

010504 meteorology & atmospheric sciencesBe starFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsType (model theory)01 natural sciencesPartícules (Física nuclear)Luminositysymbols.namesake0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsStellar rotationBalmer seriesAstronomy and AstrophysicsCircumstellar envelopeLight curveStarsAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceEsteroidessymbolsAstrophysics::Earth and Planetary Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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