Search results for " Atmosphere"

showing 10 items of 292 documents

ARES. III. Unveiling the Two Faces of KELT-7 b with HST WFC3

2020

We present the analysis of the hot-Jupiter KELT-7b using transmission and emission spectroscopy from the Hubble Space Telescope (HST), both taken with the Wide Field Camera 3 (WFC3). Our study uncovers a rich transmission spectrum which is consistent with a cloud-free atmosphere and suggests the presence of H2O and H-. In contrast, the extracted emission spectrum does not contain strong absorption features and, although it is not consistent with a simple blackbody, it can be explained by a varying temperature-pressure profile, collision induced absorption (CIA) and H-. KELT-7 b had also been studied with other space-based instruments and we explore the effects of introducing these additiona…

010504 meteorology & atmospheric sciencesOpacityFOS: Physical sciencesEFFICIENTTransmission spectroscopy; Exoplanet atmospheres; Astronomy data analysisAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsAstronomy & Astrophysics01 natural sciencesAtmosphereHubble space telescope0103 physical sciencesTransmission spectroscopyEMISSION-SPECTRUMWATERBlack-body radiationEmission spectrumAbsorption (electromagnetic radiation)010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesEarth and Planetary Astrophysics (astro-ph.EP)PhysicsScience & TechnologyHOT JUPITERSAstronomy and AstrophysicsBIASESEXOPLANETSTransmission (telecommunications)13. Climate actionSpace and Planetary SciencePhysical SciencesAstronomy data analysisHD 209458BAstrophysics::Earth and Planetary AstrophysicsATMOSPHERESWide Field Camera 3Astrophysics - Earth and Planetary AstrophysicsExoplanet atmospheresThe Astronomical Journal
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The GAPS Programme with HARPS-N at TNG: . Atmospheric Rossiter-McLaughlin effect and improved parameters of KELT-9b

2019

In the framework of the GAPS project, we observed the planet-hosting star KELT-9 (A-type star, VsinI$\sim$110 km/s) with the HARPS-N spectrograph at the TNG. In this work we analyse the spectra and the extracted radial velocities (RVs), to constrain the physical parameters of the system and to detect the planetary atmosphere of KELT-9b. We extracted from the high-resolution optical spectra the mean stellar line profiles with an analysis based on the Least Square Deconvolution technique. Then, we computed the stellar RVs with a method optimized for fast rotators, by fitting the mean stellar line profile with a purely rotational profile instead of using a Gaussian function. The new spectra an…

010504 meteorology & atmospheric sciencesRossiter–McLaughlin effectFOS: Physical sciencesAstrophysics01 natural sciencesSpectral lineAtmospheretechniques: radial velocities0103 physical sciencesAstrophysics::Solar and Stellar Astrophysicsplanetary systems010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesEarth and Planetary Astrophysics (astro-ph.EP)planets and satellites: atmospheresPhysicsSettore FIS/05Astronomy and AstrophysicsPlanetary systemstars: individual: KELT-9ExoplanetRadial velocityAmplitudeAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics::Earth and Planetary AstrophysicsPlanetary masstechniques: spectroscopicAstrophysics - Earth and Planetary Astrophysics
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High-resolution 40Ar/39Ar chronostratigraphy of the post-caldera (<20 ka) volcanic activity at Pantelleria, Sicily Strait

2011

Abstract The island of Pantelleria (Sicily Strait), the type locality for pantellerite, has been the locus of major caldera-forming eruptions that culminated, ca. 50 ka ago, in the formation of the Cinque Denti caldera produced by the Green Tuff eruption. The post-caldera silicic activity since that time has been mostly confined inside the caldera and consists of smaller-energy eruptions represented by more than twenty coalescing pantelleritic centers structurally controlled by resurgence and trapdoor faulting of the caldera floor. A high-resolution 40Ar/39Ar study was conducted on key units spanning the recent (post-20 ka) intracaldera activity to better characterize the present-day status…

010504 meteorology & atmospheric sciencesSilicicForcing (mathematics)010502 geochemistry & geophysics01 natural sciencesPaleontologyGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)CalderaChronostratigraphy[SDU.ENVI]Sciences of the Universe [physics]/Continental interfaces environmentComputingMilieux_MISCELLANEOUS0105 earth and related environmental sciences40Ar/39Ar xenocrysts excess 40Ar anorthoclase[SDU.OCEAN]Sciences of the Universe [physics]/Ocean AtmosphereHorizon (geology)geographygeography.geographical_feature_categorySettore GEO/07 - Petrologia E PetrografiaSubsidencePaleosolSettore GEO/08 - Geochimica E VulcanologiaGeophysicsVolcano13. Climate actionSpace and Planetary ScienceGeology
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Star-disk interaction in classical T Tauri stars revealed using wavelet analysis

2016

The extension of the corona of classical T Tauri stars (CTTS) is under discussion. The standard model of magnetic configuration of CTTS predicts that coronal magnetic flux tubes connect the stellar atmosphere to the inner region of the disk. However, differential rotation may disrupt these long loops. The results from Hydrodynamic modeling of X-ray flares observed in CTTS confirming the star-disk connection hypothesis are still controversial. Some authors suggest the presence of the accretion disk prevent the stellar corona to extent beyond the co-rotation radius, while others simply are not confident with the methods used to derive loop lengths. We use independent procedures to determine t…

010504 meteorology & atmospheric sciencesStars: flareAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesX-rays: starsContext (language use)Astrophysics01 natural sciencesSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesOrion NebulaDifferential rotationAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsCoronal seismologyHigh Energy Astrophysical Phenomena (astro-ph.HE)Stellar atmosphereAstronomy and AstrophysicsCoronaT Tauri starStarsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena
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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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Evidence for marine biogenic influence on summertime Arctic aerosol

2017

International audience; We present vertically-resolved observations of aerosol composition during pristine summertime Arctic background conditions. The methansulfonic acid (MSA)-to-sulfate ratio peaked near the surface (mean 0.10), indicating a contribution from ocean-derived biogenic sulfur. Similarly, the organic aerosol (OA)-to-sulfate ratio increased towards the surface (mean 2.0). Both MSA-to-sulfate and OA-to-sulfate ratios were significantly correlated with FLEXPART-WRF-predicted airmass residence time over open water, indicating marine influenced OA. External mixing of sea salt aerosol from a larger number fraction of organic, sulfate and amine-containing particles, together with lo…

010504 meteorology & atmospheric sciencesmethanesulfonic acidchemistry.chemical_element010501 environmental sciencesAtmospheric sciences01 natural sciencesMethanesulfonic acidArctic aerosolchemistry.chemical_compoundmarine organic aerosolCloud condensation nucleiSulfateSea salt aerosol0105 earth and related environmental sciences[SDU.OCEAN]Sciences of the Universe [physics]/Ocean Atmosphereaerosol mass spectrometrySulfurArctic summerAerosolGeophysicsArcticchemistry13. Climate actionGeneral Earth and Planetary SciencesAerosol mass spectrometryEnvironmental sciencesecondary organic aerosol
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Identification of processes that control the stable isotope composition of rainwater in the humid tropical West-Central Africa.

2020

12 pages; International audience; This study interprets 11 years (2006 to 2016) and 6 months (March to August in 2017) of respectively monthly and daily isotopic (δD and δ18O) monitoring of rain at Douala (Cameroon), a humid tropical station in Western Africa. The main scope is to analyze the climate controls on precipitation isotopes at different timescales. Firstly, we examine the annual cycles of δ18O. Over the 11 years of survey, the annual cycle exhibits a W shape that is quite reproducible from year to year, with two minima in spring and autumn periods. Based on back trajectory calculations and remote sensing observations of water vapor isotopic composition, we show that the observed …

010504 meteorology & atmospheric sciencesδ18O0207 environmental engineeringHumid subtropical climate02 engineering and technologyAtmospheric sciencesAir back trajectory01 natural sciencesGPCP precipitation[SDU.STU.GC]Sciences of the Universe [physics]/Earth Sciences/GeochemistrySpring (hydrology)Precipitation020701 environmental engineeringδ18OComputingMilieux_MISCELLANEOUSAir mass0105 earth and related environmental sciencesWater Science and TechnologyWater vapor[SDU.OCEAN]Sciences of the Universe [physics]/Ocean Atmospheregeographygeography.geographical_feature_categoryStable isotope ratioAnnual cycleConvective activity[SDU]Sciences of the Universe [physics]13. Climate action[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/ClimatologyEnvironmental scienceWater vapor
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Insolation cycles as a major control equatorial Indian Ocean primary production

1997

Analysis of a continuous sedimentary record taken in the Maldives indicates that strong primary production fluctuations (70 to 390 grams of carbon per square meter per year) have occurred in the equatorial Indian Ocean during the past 910,000 years. The record of primary production is coherent and in phase with the February equatorial insolation, whereas it shows diverse phase behavior with δ 18 O, depending on the orbital frequency (eccentricity, obliquity, or precession) examined. These observations imply a direct control of productivity in the equatorial oceanic system by insolation. In the equatorial Indian Ocean, productivity is driven by the wind intensity of westerlies, which is rel…

010504 meteorology & atmospheric sciencesδ18Omedia_common.quotation_subject[SDU.STU]Sciences of the Universe [physics]/Earth SciencesForcing (mathematics)010502 geochemistry & geophysics01 natural sciencesPhysics::Geophysics100000-year problem14. Life underwaterEccentricity (behavior)Physics::Atmospheric and Oceanic Physics0105 earth and related environmental sciencesmedia_common[SDU.OCEAN]Sciences of the Universe [physics]/Ocean AtmosphereMultidisciplinaryEquatorial wavesWesterliesOceanographyProductivity (ecology)13. Climate action[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/ClimatologyClimatologyPhysics::Space PhysicsPrecessionAstrophysics::Earth and Planetary Astrophysics[SDU.STU.PG]Sciences of the Universe [physics]/Earth Sciences/PaleontologyGeology
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Carbon-isotope records of the Early Jurassic (Toarcian) Oceanix Anixic Event from the Valdorbia (Umbria-Marche Apennines) and Monte Mangart (Julian A…

2009

The Toarcian oceanic anoxic event (ca 183 Ma) coincides with a global perturbation marked by enhanced organic carbon burial and a general decrease in calcium carbonate production, probably triggered by changes in the composition of marine plankton and elevated carbon dioxide levels in the atmosphere. This study is based on high-resolution sampling of two stratigraphic successions, located in Valdorbia (Umbria-Marche Apennines) and Monte Mangart (Julian Alps), Italy, which represent expressions of the Toarcian oceanic anoxic event in deep-water pelagic sediments. These successions are characterized by the occurrence of black shales showing relatively low total organic carbon concentrations (…

010506 paleontologystratigraphic correlationStratigraphy[SDU.STU]Sciences of the Universe [physics]/Earth SciencesBiostratigraphy010502 geochemistry & geophysics01 natural sciencesPaleontologyCarbon isotopes cyclostratigraphy Early Jurassic oceanic anoxic event stratigraphic correlation.oceanic anoxic event14. Life underwateroceanic anoxiceventComputingMilieux_MISCELLANEOUS0105 earth and related environmental sciencesCarbon isotopes; cyclostratigraphy; Early Jurassic; oceanic anoxic event; stratigraphic correlationCarbon isotopes; cyclostratigraphy; Early Jurassic; oceanic anoxicevent; stratigraphic correlation.AmmoniteCarbon dioxide in Earth's atmosphereEarly JurassicCarbon isotopesGeologyPelagic sedimentCyclostratigraphyAnoxic waterslanguage.human_languageSettore GEO/08 - Geochimica E Vulcanologia13. Climate actionIsotopes of carbonlanguageSedimentary rockcyclostratigraphyGeology
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Understanding the uncertainty in global forest carbon turnover

2020

Abstract. The length of time that carbon remains in forest biomass is one of the largest uncertainties in the global carbon cycle, with both recent historical baselines and future responses to environmental change poorly constrained by available observations. In the absence of large-scale observations, models used for global assessments tend to fall back on simplified assumptions of the turnover rates of biomass and soil carbon pools. In this study, the biomass carbon turnover times calculated by an ensemble of contemporary terrestrial biosphere models (TBMs) are analysed to assess their current capability to accurately estimate biomass carbon turnover times in forests and how these times a…

0106 biological sciences010504 meteorology & atmospheric sciencesEnvironmental changelcsh:Life01 natural sciencesCarbon cyclelcsh:QH540-549.5ddc:550Baseline (configuration management)Ecology Evolution Behavior and Systematics0105 earth and related environmental sciencesEarth-Surface Processes[SDU.OCEAN]Sciences of the Universe [physics]/Ocean AtmosphereBiomass (ecology)lcsh:QE1-996.5BiosphereSoil carbon15. Life on landPlant functional typelcsh:GeologyEarth scienceslcsh:QH501-531[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/Climatology13. Climate actionTurnoverlcsh:EcologyPhysical geography010606 plant biology & botanyBiogeosciences
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