Search results for " atmosphere"

showing 10 items of 292 documents

Quantification of land-atmosphere exchanges of water, energy and carbon dioxide in space and time over the heterogeneous Barrax site

2008

International audience; To advance our understanding of land-atmosphere exchanges of water, energy and carbon dioxide (CO2) in space and time over heterogeneous land surfaces, two intensive field campaigns were carried out at the Barrax agricultural test site in Spain during 12-21 July 2004 (SPARC 2004) and 8-14 July 2005 (SEN2FLEX 2005) involving multiple field, satellite and airborne instruments for characterizing the state of the atmosphere, the vegetation and the soil from the visible to the microwave range of the spectrum. Part of the experimental area is a core site of area 25 km2, within which numerous crops are grown, on both irrigated and dry land, alongside fields of bare soil. Th…

[SPI.OTHER]Engineering Sciences [physics]/Otherenergie-uitwisselingEarth observation010504 meteorology & atmospheric sciences02 engineering and technologyatmosferische grenslaag01 natural sciencesBARRAXAIRBORNE INSTRUMENTchemistry.chemical_compoundremote sensingmetingLaboratory of Geo-information Science and Remote SensingAlterra - Centre for Water and ClimateWageningen Environmental Research020701 environmental engineeringWater energySATELLITEatmospheric boundary-layerENVIRONMENTAL SCIENCEVegetationCentre Geo-informationPE&RCkooldioxideRemote sensing (archaeology)Carbon dioxideaardoppervlakAlterra - Centrum Water en KlimaatPlanetary boundary layerAlterra - Centrum Geo-informatiewater0207 environmental engineeringWRSvegetatieAtmospherevegetationLaboratorium voor Geo-informatiekunde en Remote Sensingatmosfeer0105 earth and related environmental sciencesRemote sensingland surfaceSPAINCROPcarbon dioxide15. Life on landLAND ATMOSPHERERELATION SOL-PLANTE-ATMOSPHEREHETEROGENEOUS LAND SURFACEenergy exchangeSOILADLIB-ART-2682chemistry13. Climate actionITC-ISI-JOURNAL-ARTICLEatmosphereGeneral Earth and Planetary SciencesEnvironmental scienceSatellitemeasurement
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Could the acid-base status of Antarctic sea urchins indicate a better-than-expected resilience to near-future ocean acidification?

2015

13 pages; International audience; Increasing atmospheric carbon dioxide concentration alters the chemistry of the oceans towards more acidic conditions. Polar oceans are particularly affected due to their low temperature, low carbonate content and mixing patterns, for instance upwellings. Calcifying organisms are expected to be highly impacted by the decrease in the oceans' pH and carbonate ions concentration. In particular, sea urchins, members of the phylum Echinodermata, are hypothesized to be at risk due to their high-magnesium calcite skeleton. However, tolerance to ocean acidification in metazoans is first linked to acid–base regulation capacities of the extracellular fluids. No infor…

acid-base regulationClimate Change[SDE.MCG]Environmental Sciences/Global ChangesAntarctic RegionsAmphipneustes lorioliocean acidificationAcid–base homeostasisbiology.animalsea urchinsAnimalsEnvironmental ChemistrySterechinus neumayeriSeawater14. Life underwaterSouthern OceanSea urchinGeneral Environmental ScienceAcid-Base EquilibriumGlobal and Planetary ChangeCarbon dioxide in Earth's atmosphere[ SDE.BE ] Environmental Sciences/Biodiversity and EcologyEchinodermata [Echinoderms]EcologybiologyEcologyechinodermsOcean acidificationGlobal changebiology.organism_classificationacid–base regulation[ SDE.MCG ] Environmental Sciences/Global ChangesOceanography13. Climate actionAntarcticaSeawater[SDE.BE]Environmental Sciences/Biodiversity and Ecology
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The Pros and Cons of Beyond Standard Model Interpretations of ANITA Events

2019

The Antarctic Impulsive Transient Antenna (ANITA) experiment has observed two air shower events with energy $\sim 500~{\rm PeV}$ emerging from the Earth with exit angles $\sim 30^\circ$ above the horizon. As was immediately noted by the ANITA Collaboration, these events (in principle) could originate in the atmospheric decay of an upgoing $\tau$-lepton produced through a charged current interaction of a $\nu_\tau$ inside the Earth. However, the relatively steep arrival angles of these perplexing events create tension with the standard model (SM) neutrino-nucleon interaction cross section. Deepening the conundrum, the IceCube neutrino telescope and the Pierre Auger Observatory with substanti…

airAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesparticle: messengerAstrophysics01 natural scienceshorizonneutrino nucleon: interactioncharged currentIceCubeHigh Energy Physics - Phenomenology (hep-ph)Observatory0103 physical sciences010306 general physicsCharged currentHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPierre Auger Observatoryneutrino/tauCOSMIC cancer databaseshowers: atmosphere010308 nuclear & particles physicsHorizonANITAAstrophysics::Instrumentation and Methods for AstrophysicstensionsensitivityAugerfluxobservatoryHigh Energy Physics - Phenomenologyneutrino: detectorAir showerNeutrino detector[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Astrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Event (particle physics)Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)
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Neutral Iron Emission Lines From The Day-side Of KELT-9b -- The GAPS Programme With HARPS-N At TNG XX

2020

We present the first detection of atomic emission lines from the atmosphere of an exoplanet. We detect neutral iron lines from the day-side of KELT-9b (Teq $\sim$ 4, 000 K). We combined thousands of spectrally resolved lines observed during one night with the HARPS-N spectrograph (R $\sim$ 115, 000), mounted at the Telescopio Nazionale Galileo. We introduce a novel statistical approach to extract the planetary parameters from the binary mask cross-correlation analysis. We also adapt the concept of contribution function to the context of high spectral resolution observations, to identify the location in the planetary atmosphere where the detected emission originates. The average planetary li…

astro-ph.SR010504 meteorology & atmospheric sciencesContinuum (design consultancy)FOS: Physical sciencesContext (language use)Astrophysics01 natural sciencesExoplanet atmospheres; Exoplanet atmospheric composition; High resolution spectroscopyAtmosphereHigh resolution spectroscopy0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsEmission spectrumSpectral resolution010303 astronomy & astrophysicsSpectrographInstrumentation and Methods for Astrophysics (astro-ph.IM)Solar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesLine (formation)PhysicsEarth and Planetary Astrophysics (astro-ph.EP)Settore FIS/05Astronomy and AstrophysicsExoplanetAstrophysics - Solar and Stellar AstrophysicsExoplanet atmospheric composition13. Climate actionSpace and Planetary Scienceastro-ph.EPAstrophysics::Earth and Planetary AstrophysicsAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - Earth and Planetary AstrophysicsExoplanet atmospheresastro-ph.IM
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Mitigation of the impact of stellar activity on observations of transiting planets

2023

La tesi si concentra sulla quantificazione dell'impatto dell'attività stellare sulle osservazioni dei pianeti in transito e sull'identificazione di una metodologia per correggere questi effetti. In particolare, viene approfondito l'effetto delle macchie stellari, sia non occultate che occulte. La presenza di macchie sul disco stellare visibile può distorcere la curva della luce di transito primaria in modo dipendente dalla lunghezza d'onda, mimando la presenza di un'atmosfera. Per tener conto di questo effetto, la tesi presenta un metodo innovativo per stimare le proprietà delle macchie e la loro distribuzione dalle osservazioni fuori transito e, su questa base, correggere le curve di luce …

astronomystellar spotplanetary atmosphereSettore FIS/05 - Astronomia E Astrofisicastellar activityexoplanetspace missionsplanetary system
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Propagating Alfvén waves in open structures with random structuring

2022

Funding: The research leading to these results has received funding from the UK Science and Technology Facilities Council (consolidated grant ST/N000609/1), the European Union Horizon 2020 research and innovation programme (grant agreement No. 647214). IDM received funding from the Research Council of Norway through its Centres of Excellence scheme, project number 262622. We consider the behaviour of Alfvén waves propagating in a medium with random density perturbations. The imposed density perturbations have a broadband spectrum and their characteristic spatial scale may be defined according to the peak in the spectrum. The interaction of the boundary driven Alfvén waves with the medium ge…

atmosphere [Sun]MCCcorona [Sun]MHDoscillations [Sun]NDASAstronomy and AstrophysicsMHD – Sun: atmosphere – Sun: corona – Sun: oscillationsQC PhysicsSpace and Planetary ScienceQB AstronomySettore FIS/06 - Fisica Per Il Sistema Terra E Il Mezzo CircumterrestreQCQB
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Contribution of observed multi frequency spectrum of Alfvén waves to coronal heating

2019

Context. Whilst there are observational indications that transverse magnetohydrodynamic (MHD) waves carry enough energy to maintain the thermal structure of the solar corona, it is not clear whether such energy can be efficiently and effectively converted into heating. Phase-mixing of Alfvén waves is considered a candidate mechanism, as it can develop transverse gradient where magnetic energy can be converted into thermal energy. However, phase-mixing is a process that crucially depends on the amplitude and period of the transverse oscillations, and only recently have we obtained a complete measurement of the power spectrum for transverse oscillations in the corona. Aims. We aim to investig…

atmosphere [Sun]Magnetohydrodynamics (MHD)corona [Sun]T-NDASContext (language use)Astrophysics01 natural sciences03 medical and health sciences0103 physical sciencesQB AstronomyAstrophysics::Solar and Stellar AstrophysicsQA MathematicsSun: oscillationsQASun: magnetic fields010303 astronomy & astrophysicsQCQB030304 developmental biologyPhysics0303 health sciencesMagnetic energySun: coronaoscillations [Sun]Spectral densityAstronomy and AstrophysicsTransverse waveCoronal loopComputational physicsTransverse planeQC PhysicsAmplitudemagnetic fields [Sun]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsWavesMagnetohydrodynamicsSun: atmosphereAstronomy & Astrophysics
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Solar Coronal Loops Associated with Small-scale Mixed Polarity Surface Magnetic Fields

2017

L. P. Chitta et. al.

atmosphere [Sun]corona [Sun]010504 meteorology & atmospheric sciencesphotosphere [Sun]Polarity (physics)FOS: Physical sciencesFluxAstrophysics01 natural sciencesAtmosphereObservatory0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsSun: magnetic fields010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesPhysicsPhotosphereSun: coronaSun: photosphereAstronomy and AstrophysicsCoronal loopMagnetic fluxMagnetic fieldmagnetic fields [Sun]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsSun: atmosphere
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The unique skeleton of siliceous sponges (Porifera; Hexactinellida and Demospongiae) that evolved first from the Urmetazoa during the Proterozoic: a …

2007

Abstract. Sponges (phylum Porifera) had been considered as an enigmatic phylum, prior to the analysis of their genetic repertoire/tool kit. Already with the isolation of the first adhesion molecule, galectin, it became clear that the sequences of the sponge cell surface receptors and those of the molecules forming the intracellular signal transduction pathways, triggered by them, share high similarity to those identified in other metazoan phyla. These studies demonstrated that all metazoan phyla, including the Porifera, originate from one common ancestor, the Urmetazoa. The sponges evolved during a time prior to the Ediacaran-Cambrian boundary (542 million years ago (myr)). They appeared du…

biologyPhylum[SDU.OCEAN] Sciences of the Universe [physics]/Ocean Atmospherelcsh:QE1-996.5lcsh:Lifemyrbiology.organism_classification[SDU.ASTR] Sciences of the Universe [physics]/Astrophysics [astro-ph][SDU.ENVI] Sciences of the Universe [physics]/Continental interfaces environmentSuberites domunculaIntracellular signal transductionlcsh:GeologySpongelcsh:QH501-531Body planSponge spiculeEvolutionary biology[PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]lcsh:QH540-549.5Botany[SDU.STU] Sciences of the Universe [physics]/Earth Scienceslcsh:EcologyLiving fossilEcology Evolution Behavior and SystematicsEarth-Surface Processes
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Libri, spazi, atmosfere tra immaginazione e realtà

2021

Il saggio intreccia finzione narrativa e biblioteche reali. Prendendo come spunto occasionale due romanzi, La bibliothèque des amants di André Miquel e Firmino di Sam Savage, analizza gli elementi architettonici e relazionali che in una biblioteca generano atmosfere respingenti o accoglienti, alla luce dell’estetica delle atmosfere del filosofo Gernot Böhme. The essay focuses on libraries, weaving fiction and reality. Taking two novels as an occasional cue, La bibliothèque des amants by André Miquel and Firmino by Sam Savage, the paper analyzes the architectural and relational elements that in a library generate repelling or welcoming atmospheres, in the light of the aesthetics of the atmos…

booklibriGernot BöhmeaestheticsSettore M-FIL/04 - Esteticaestetica delle atmosferetheory of sensibilityspazioestetica.spaceaesthetics of atmosphereteoria della sensibilità
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