Search results for "Climate Action"

showing 10 items of 2410 documents

Numerical evidence for thermohaline circulation reversals during the Maastrichtian

2005

[1] The sensitivity of the Maastrichtian thermohaline circulation to the opening/closing of marine communications between the Arctic and North Pacific oceans is investigated through a set of numerical experiments using the model CLIMBER-2 (Earth Model of Intermediate Complexity). We show here that the opening or closing of an Arctic-Pacific marine gateway induces transitions between different equilibrium states of the thermohaline circulation. Sensitivity tests of the inferred modes of thermohaline circulation to atmospheric CO2 level changes have also been explored. An abrupt switch in deep convection from high northern to high southern latitudes, a change consistent with isotopic evidence…

010504 meteorology & atmospheric sciencesNorth Atlantic Deep Water010502 geochemistry & geophysics01 natural sciencesCretaceousLatitudeGeophysicsOceanographyShutdown of thermohaline circulationArctic13. Climate actionGeochemistry and PetrologyClimatologyThermohaline circulationClimate model14. Life underwatergeographic locationsGeologySea level0105 earth and related environmental sciencesGeochemistry, Geophysics, Geosystems
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Coralline alga reveals first marine record of subarctic North Pacific climate change

2007

[1] While recent changes in subarctic North Pacific climate had dramatic effects on ecosystems and fishery yields, past climate dynamics and teleconnection patterns are poorly understood due to the absence of century-long high-resolution marine records. We present the first 117-year long annually resolved marine climate history from the western Bering Sea/Aleutian Island region using information contained in the calcitic skeleton of the long-lived crustose coralline red alga Clathromorphum nereostratum, a previously unused climate archive. The skeletal δ18O-time series indicates significant warming and/or freshening of surface waters after the middle of the 20th century. Furthermore, the ti…

010504 meteorology & atmospheric sciencesOceanic climateClimate change010502 geochemistry & geophysics01 natural sciencesSubarctic climateNorth Pacific OscillationGeophysicsGeographyOceanography13. Climate actionClimatologyGeneral Earth and Planetary SciencesEcosystem14. Life underwaterCrustosePacific decadal oscillation0105 earth and related environmental sciencesTeleconnectionGeophysical Research Letters
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Flares from small to large: X-ray spectroscopy of Proxima Centauri with XMM-Newton

2003

(Abridged) We report results from a comprehensive study of the nearby M dwarf Proxima Centauri with the XMM-Newton satellite. We find strongly variable coronal X-ray emission, with flares ranging over a factor of 100 in peak flux. The low-level emission is found to be continuously variable. Several weak flares are characteristically preceded by an optical burst, compatible with predictions from standard solar flare models. We propose that the U band bursts are proxies for the elusive stellar non-thermal hard X-ray bursts suggested from solar observations. A very large X-ray flare was observed in its entirety, with a peak luminosity of 3.9E28 erg/s [0.15-10 keV] and a total X-ray energy of 1…

010504 meteorology & atmospheric sciencesOpacityAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxAstrophysicsAstrophysics01 natural scienceslaw.inventionLuminositylaw0103 physical sciencesAstrophysics::Solar and Stellar Astrophysicsstars: activity stars: coronae stars: individual: Proxima Centauri X-rays: starsSpectroscopy010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsSolar flareAstrophysics (astro-ph)Astronomy and AstrophysicsPlasma3. Good healthStars13. Climate actionSpace and Planetary SciencePhysics::Space PhysicsAstrophysics::Earth and Planetary AstrophysicsFlare
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GJ 357 b: A Super-Earth Orbiting an Extremely Inactive Host Star

2020

Aims. In this paper we present a deep X-ray observation of the nearby M dwarf GJ 357 and use it to put constraints on the atmospheric evolution of its planet, GJ 357 b. We also analyse the systematic errors in the stellar parameters of GJ 357 in order to see how they affect the perceived planetary properties. Methods. By comparing the observed X-ray luminosity of its host star, we estimate the age of GJ 357 b as derived from a recent XMM-Newton observation (log Lx [erg s-1] = 25.73), with Lx-age relations for M dwarfs. We find that GJ 357 presents one of the lowest X-ray activity levels ever measured for an M dwarf, and we put a lower limit on its age of 5 Gyr. Using this age limit, we perf…

010504 meteorology & atmospheric sciencesOpacityFOS: Physical sciencesAstrophysicsStar (graph theory)01 natural sciencesLuminosityPlanet0103 physical sciences010303 astronomy & astrophysicsstars [X rays]Solar and Stellar Astrophysics (astro-ph.SR)physical evolution [Planets and satellites]0105 earth and related environmental sciencesEnvelope (waves)PhysicsEarth and Planetary Astrophysics (astro-ph.EP)Secondary atmosphereSuper-EarthAstronomy and AstrophysicsRadiusPlanet star interactionsAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary Scienceterrestrial planets [Planets and satellites]atmospheres [Planets and satellites]Astrophysics - Earth and Planetary Astrophysics
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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 high overtone and combination levels of SF6 revisited at Doppler-limited resolution: A global effective rovibrational model for highly excited vi…

2017

Abstract Sulfur hexafluoride is an important prototypal molecule for modeling highly excited vibrational energy flow and multi quanta absorption processes in hexafluoride molecules of technological importance. It is also a strong greenhouse gas of anthropogenic origin. This heavy species, however, features many hot bands at room temperature (at which only 30% of the molecules lie in the ground vibrational state), especially those originating from the lowest, v 6 =1 vibrational state. Using a cryogenic long path cell with variable optical path length and temperatures regulated between 120 and 163 K, coupled to Synchrotron Radiation and a high resolution interferometer, Doppler-limited spectr…

010504 meteorology & atmospheric sciencesOvertoneInfrared spectroscopylow temperature01 natural sciences7. Clean energyHot bandSpectral linechemistry.chemical_compoundHexafluorideFar infraredhot bandRotation-vibration spectroscopy of SF 60103 physical sciencesSpectroscopy0105 earth and related environmental sciencesPhysics[PHYS]Physics [physics]Radiation[ PHYS ] Physics [physics]010304 chemical physicsRotational–vibrational spectroscopyAtomic and Molecular Physics and Opticschemistry13. Climate actiongreenhouse gasExcited stateinfrared absorptionAtomic physicstensorial formalismLong path cell
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Phanerozoic geological evolution of Northern and Central Africa: An overview.

2005

61 pages; International audience; The principal paleogeographic characteristics of North and Central Africa during the Paleozoic were the permanency of large exposed lands over central Africa, surrounded by northerly and northwesterly dipping pediplanes episodically flooded by epicontinental seas related to the Paleotethys Ocean. The intra-continental Congo–Zaire Basin was also a long-lived feature, as well as the Somali Basin from Late Carboniferous times, in conjunction with the development of the Karoo basins of southern Africa. This configuration, in combination with eustatic sea-level fluctuations, had a strong influence on facies distributions. Significant transgressions occurred duri…

010504 meteorology & atmospheric sciencesPaleozoicPhanerozoicInversion (geology)Northeastern Africa010502 geochemistry & geophysics[ SDU.STU.ST ] Sciences of the Universe [physics]/Earth Sciences/Stratigraphy01 natural sciencesDevonianPaleontologyPassive margin[ SDE.MCG.CG ] Environmental Sciences/Global Changes/domain_sde.mcg.cg14. Life underwaterNorthern AfricaWestern Africa0105 earth and related environmental sciencesEarth-Surface Processes[SDU.STU.TE]Sciences of the Universe [physics]/Earth Sciences/TectonicsgeographyNeotethysgeography.geographical_feature_categoryRiftCentral AfricaRiftingArabiaTectonicsInversionMagmatismGeologyOrogeny[ SDU.STU.TE ] Sciences of the Universe [physics]/Earth Sciences/TectonicsCraton13. Climate action[SDU.STU.ST]Sciences of the Universe [physics]/Earth Sciences/StratigraphyPaleogeographyOrdovicianPaleotethysGeology
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Radiogenic isotopes: new tools help reconstruct paleocean circulation and erosion input

2001

Ocean and atmosphere circulation and continental weathering regimes have undergone great changes over thousands of years as well as tens of millions of years. During the glacial stages of the Pleistocene, ocean circulation was generally more sluggish and deep water circulation in the Atlantic had a shallower flow. At the same time, weathering on the continents was enhanced by glacial erosion, particularly in high northern latitudes, which increased the input of erosional detritus into the ocean. In addition, atmospheric pressure gradients were larger, leading to higher wind speeds and increased supply of aeolian dust to the ocean. Prior to the onset of Northern Hemisphere glaciation and pro…

010504 meteorology & atmospheric sciencesPleistoceneNorth Atlantic Deep WaterOcean currentPhysical oceanography010502 geochemistry & geophysics01 natural sciencesOceanographyShutdown of thermohaline circulation13. Climate actionInterglacialGeneral Earth and Planetary SciencesThermohaline circulationGlacial periodGeology0105 earth and related environmental sciencesEOS
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A Search for IceCube Events in the Direction of ANITA Neutrino Candidates

2020

During the first three flights of the Antarctic Impulsive Transient Antenna (ANITA) experiment, the collaboration detected several neutrino candidates. Two of these candidate events were consistent with an ultra-high-energy up-going air shower and compatible with a tau neutrino interpretation. A third neutrino candidate event was detected in a search for Askaryan radiation in the Antarctic ice, although it is also consistent with the background expectation. The inferred emergence angle of the first two events is in tension with IceCube and ANITA limits on isotropic cosmogenic neutrino fluxes. Here, we test the hypothesis that these events are astrophysical in origin, possibly caused by a po…

010504 meteorology & atmospheric sciencesPoint sourceAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencesStandard ModelHigh Energy Physics - Phenomenology (hep-ph)Tau neutrino0103 physical sciencesTRACK RECONSTRUCTIONSource spectrum010303 astronomy & astrophysics0105 earth and related environmental sciencesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEIsotropyAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and Astrophysicshep-phHigh Energy Physics - PhenomenologyAir showerPhysics and Astronomy13. Climate actionSpace and Planetary ScienceNeutrinoAstrophysics - High Energy Astrophysical PhenomenaEvent (particle physics)
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A process-based anatomy of Mediterranean cyclones: from baroclinic lows to tropical-like systems

2021

Abstract. In this study, we address the question of the atmospheric processes that turn Mediterranean cyclones into severe storms. Our approach applies on-line potential vorticity (PV) budget diagnostics and piecewise PV inversion to WRF model simulations of the mature stage of 100 intense Mediterranean cyclones. We quantify the relative contributions of different processes to cyclone development and therefore deliver, for the first time, a comprehensive insight into the variety of cyclonic systems that develop in the Mediterranean from the perspective of cyclone dynamics. In particular, we show that all 100 cyclones are systematically influenced by two main PV anomalies: a major anomaly in…

010504 meteorology & atmospheric sciencesRadiative coolingSevere weatherBaroclinity0208 environmental biotechnologyDiabatic02 engineering and technology01 natural sciences020801 environmental engineeringTroposphere13. Climate actionMeteorology. ClimatologyClimatologyLatent heatWeather Research and Forecasting ModelCycloneEnvironmental scienceQC851-9990105 earth and related environmental sciencesWeather and Climate Dynamics
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