Search results for "HT"

showing 10 items of 20594 documents

Ash-plume dynamics and eruption source parameters by infrasound and thermal imagery: The 2010 Eyjafjallajökull eruption

2013

During operational ash-cloud forecasting, prediction of ash concentration and total erupted mass directly depends on the determination of mass eruption rate (MER), which is typically inferred from plume height. Uncertainties for plume heights are large, especially for bent-over plumes in which the ascent dynamics are strongly affected by the surrounding wind field. Here we show how uncertainties can be reduced if MER is derived directly from geophysical observations of source dynamics. The combination of infrasound measurements and thermal camera imagery allows for the infrasonic type of source to be constrained (a dipole in this case) and for the plume exit velocity to be calculated (54–14…

010504 meteorology & atmospheric sciencesMeteorologyInfrasound Thermal cameras Volcanic Plume dynamicsInfrasoundPlume heightInfrasound010502 geochemistry & geophysicsAtmospheric sciences01 natural sciencesGeochemistry and PetrologyThermalEarth and Planetary Sciences (miscellaneous)ddc:5500105 earth and related environmental sciencesPlume heightLead (sea ice)Escape velocityPlumeGeophysics13. Climate actionSpace and Planetary ScienceParticle-size distributionEruption rateAsh eruptionsMass eruption rateGeology
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A Cloud masking algorithm for the XBAER aerosol retrieval using MERIS data

2017

Abstract To determine aerosol optical thickness, AOT, and other geophysical parameters describing conditions in the atmosphere and at the earth's surface by inversion of remote sensing measurements from space based instrumentation, it is necessary to separate ground scenes into cloud free and cloudy or cloud contaminated. Identifying the presence of cloud in a ground scene and establishing an accurate and adequate cloud mask is a challenging task. In this study, measurements by the European Space Agency (ESA) MEdium Resolution Imaging Spectrometer (MERIS) have been used to develop a cloud identification and cloud mask algorithm for preprocessing prior to application of the new algorithm cal…

010504 meteorology & atmospheric sciencesMeteorologySYNOPbusiness.industryCloud topCloud fraction0211 other engineering and technologiesSoil ScienceGeologyCloud computing02 engineering and technology01 natural sciencesSCIAMACHYLidarCloud heightRadianceEnvironmental scienceComputers in Earth SciencesbusinessAlgorithm021101 geological & geomatics engineering0105 earth and related environmental sciencesRemote sensingRemote Sensing of Environment
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Retrieval of daily gross primary production over Europe and Africa from an ensemble of SEVIRI/MSG products

2018

The main goal of this paper is to derive a method for a daily gross primary production (GPP) product over Europe and Africa taking the full advantage of the SEVIRI/MSG satellite products from the European Organization for the Exploitation of Meteorological Satellites (EUMETSAT) sensors delivered from the Satellite Application Facility for Land Surface Analysis (LSA SAF) system. Special attention is paid to model the daily GPP response from an optimized Montheith's light use efficiency model under dry conditions by controlling water shortage limitations from the actual evapotranspiration and the potential evapotranspiration (PET). The PET was parameterized using the mean daily air temperatur…

010504 meteorology & atmospheric sciencesMeteorologySettore AGR/05 - ASSESTAMENTO FORESTALE E SELVICOLTURAWater stressBiome0211 other engineering and technologiesEddy covarianceDaily02 engineering and technologyManagement Monitoring Policy and LawAtmospheric sciences01 natural sciencesLight-Use EfficiencyEvapotranspirationComputers in Earth SciencesMSG021101 geological & geomatics engineering0105 earth and related environmental sciencesEarth-Surface ProcessesGlobal and Planetary ChangeConsistency analysisRelative biasPrimary production15. Life on landGeographyPhysical Geography13. Climate actionLSA SAFForest vegetationSatelliteLight-use efficiencyGPP
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Ray optics for absorbing particles with application to ice crystals at near-infrared wavelengths

2018

Abstract Light scattering by particles large compared to the wavelength of incident light is traditionally solved using ray optics which considers absorption inside the particle approximately, along the ray paths. To study the effects rising from this simplification, we have updated the ray-optics code SIRIS to take into account the propagation of light as inhomogeneous plane waves inside an absorbing particle. We investigate the impact of this correction on traditional ray-optics computations in the example case of light scattering by ice crystals through the extended near-infrared (NIR) wavelength regime. In this spectral range, ice changes from nearly transparent to opaque, and therefore…

010504 meteorology & atmospheric sciencesOpacityspektroskopiaIce crystalsPhysics::OpticsRay optics01 natural sciencesPOLARIZED-LIGHT SCATTERING114 Physical sciencesLight scattering010309 opticsScatteringMEDIAOptics0103 physical sciencesABSORPTIONInhomogeneous wavesCIRRUSray opticsSpectroscopy0105 earth and related environmental sciencesPhysicsta113absorbing mediaRadiationta115Geometrical opticsIce crystalsta114Scatteringbusiness.industryscatteringCLOUDSkiteetRayAtomic and Molecular Physics and OpticsoptiikkaSOLAR-RADIATIONWavelengthMAXWELLS EQUATIONSAbsorbing mediainhomogeneous wavesLight scattering by particlesPHASE MATRIXGEOMETRIC-OPTICSbusinessice crystalsAPPROXIMATION
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Fluid storage and migration properties of sheared Neptunian dykes

2019

Abstract Neptunian dykes are widely reported along the Tethyan carbonate platforms and are commonly considered as subsurface baffles or barriers to fluid flow. However, the fluid storage and migration properties of sheared Neptunian dykes are poorly known. For this reason, we investigate the inner structure and fluid flow properties of two Neptunian dykes, which can be characterized by different architectures if involved or not in brittle shearing processes. The dykes strike ca. WNW-ESE and crosscutting the tight Jurassic limestones exposed at Maranfusa Mt., NW Sicily, Italy. The unsheared and sheared Neptunian dykes are almost sub-vertical and at high-angle with respect to the horizontal p…

010504 meteorology & atmospheric sciencesOutcropStratigraphyCataclastic rockFault (geology)010502 geochemistry & geophysicsOceanography01 natural sciencesDFN modellingPetrographyNeptunian dykeBrecciaFault permeabilityFault architectureTight carbonatesPetrologySicily0105 earth and related environmental sciencesgeographygeography.geographical_feature_categoryGeologyCretaceousTectonicsGeophysicsEconomic GeologySedimentary rockGeology
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Titan's surface albedo variations over a Titan season from near-infrared CFHT/FTS spectra

2006

International audience; We have observed Titan in a series of campaigns from 1991 to 1996 with the Fourier Transform Spectrometer on the CFH telescope. The data acquired provide a lightcurve from the geometric albedos in the 0.9–View the MathML source spectral region. The 1991–1993 data were previously analyzed in Coustenis et al. [1995. Titan's surface: composition and variability from its near-infrared albedo. Icarus 118, 87–104] with a spherical particle code by McKay et al. [1989. The thermal structure of Titan's atmosphere. Icarus 80, 23–53]. We present here three new datasets from the 1994, 1995 and 1996 observations, with additional information from the 0.94-μm methane window on Tita…

010504 meteorology & atmospheric sciencesSatellitesCFHTAstrophysicsAtmospheric sciences01 natural sciencesMethaneAtmosphereMethane absorption coefficientssymbols.namesakechemistry.chemical_compoundNear-infraredPlanet0103 physical sciencesRadiative transfer010303 astronomy & astrophysicsSpectroscopy0105 earth and related environmental sciencesPhysicsAtmospheric methaneAstronomy and AstrophysicsTholinAlbedochemistry13. Climate actionSpace and Planetary SciencesymbolsTitan (rocket family)Titan
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PHYSICS-based retrieval of scattering albedo and vegetation optical depth using multi-sensor data integration

2017

Vegetation optical depth and scattering albedo are crucial parameters within the widely used τ-ω model for passive microwave remote sensing of vegetation and soil. A multi-sensor data integration approach using ICESat lidar vegetation heights and SMAP radar as well as radiometer data enables a direct retrieval of the two parameters on a physics-derived basis. The crucial step within the retrieval methodology is the calculus of the vegetation scattering coefficient KS, where one exact and three approximated solutions are provided. It is shown that, when using the assumption of a randomly oriented volume, the backscatter measurements of the radar provide a sufficient first order estimate and …

010504 meteorology & atmospheric sciencesScattering albedo0208 environmental biotechnologyradiometry02 engineering and technologyretrieval methodologycomputer.software_genre01 natural scienceslaw.inventionlawremote sensing by radarRadaractive-passive microwavesPhysics::Atmospheric and Oceanic PhysicsIndexespassive microwave remote sensingRemote sensingremote sensing by laser beamGeographyLidaroptical radarcrucial parametersmedicine.symptomvegetation scattering coefficientData integrationBackscattervegetation mappingta1171τ-ω modelsoilPhysics::GeophysicsICESat lidar vegetation heightsvegetationmedicineVegetation optical depthbackscatter0105 earth and related environmental sciencesRemote sensingsensor fusionRadiometerScatteringnovel multisensor approachSMAPAlbedoMulti-sensor020801 environmental engineeringradiometer dataVegetation (pathology)multisensor data integration approachcomputerICESatalbedo
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Innovative technical implementation of the Schumann resonances and its influence on organisms and biological cells

2019

Over the course of time in the digital age, oscillating processes were utilized in various realizations. Life without these became hardly imaginable. Schumann resonances are electromagnetical resonances or eigenfrequencies (radio waves), which originate from the oscillation in a hollow space shell. Their average basic frequency is 7,83Hz. The above-mentioned radio waves emerge from energy discharges such as thunderstorms, lightning or solar wind within the earth's surface and the ionosphere. They exist around the globe. Various scientists have discovered a correlation to our health on the basis of studies and experiments; their absence can result in a variety of disorders from headaches to …

010504 meteorology & atmospheric sciencesSchumann resonancesComputer scienceGeophysics01 natural sciencesLightningField (geography)03 medical and health sciencesSolar wind0302 clinical medicine030220 oncology & carcinogenesisThunderstormIonosphere0105 earth and related environmental sciencesRadio waveIOP Conference Series: Materials Science and Engineering
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Slow-Mode Magnetoacoustic Waves in Coronal Loops

2021

Rapidly decaying long-period oscillations often occur in hot coronal loops of active regions associated with small (or micro-) flares. This kind of wave activity was first discovered with the SOHO/SUMER spectrometer from Doppler velocity measurements of hot emission lines, thus also often called "SUMER" oscillations. They were mainly interpreted as global (or fundamental mode) standing slow magnetoacoustic waves. In addition, increasing evidence has suggested that the decaying harmonic type of pulsations detected in light curves of solar and stellar flares are likely caused by standing slow-mode waves. The study of slow magnetoacoustic waves in coronal loops has become a topic of particular…

010504 meteorology & atmospheric sciencesSolar activityFOS: Physical sciencesSolar corona01 natural sciencesStanding wave0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsEmission spectrum010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesCoronal seismologyPhysicsOscillationOscillations and wavesAstronomy and AstrophysicsCoronal loopLight curveThermal conductionCoronal loopsComputational physicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsMagnetohydrodynamics
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Understanding the Origins of Problem Geomagnetic Storms Associated with "Stealth" Coronal Mass Ejections.

2021

Geomagnetic storms are an important aspect of space weather and can result in significant impacts on space- and ground-based assets. The majority of strong storms are associated with the passage of interplanetary coronal mass ejections (ICMEs) in the near-Earth environment. In many cases, these ICMEs can be traced back unambiguously to a specific coronal mass ejection (CME) and solar activity on the frontside of the Sun. Hence, predicting the arrival of ICMEs at Earth from routine observations of CMEs and solar activity currently makes a major contribution to the forecasting of geomagnetic storms. However, it is clear that some ICMEs, which may also cause enhanced geomagnetic activity, cann…

010504 meteorology & atmospheric sciencesSpace weather01 natural scienceslaw.inventionDIMMINGSPhysics - Space PhysicslawRECONNECTIONCoronal mass ejectionQB Astronomy010303 astronomy & astrophysicsCoronagraphQCMISSIONQBSTREAMERSUN3rd-DASLow-coronal signaturesMagnetic StormsAstrophysics - Solar and Stellar AstrophysicsMagnetic stormsPhysical SciencesCURRENT SHEETSpace WeatherGeologyCoronal Mass EjectionsSettore FIS/06 - Fisica Per Il Sistema Terra E Il Mezzo CircumterrestreSpace weatherSOLAR-WIND HELIUMMAGNETIC CLOUDSFOS: Physical sciencesSolar cycle 24Astronomy & AstrophysicsArticleCurrent sheet0103 physical sciencesSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesGeomagnetic stormScience & TechnologyAstronomyAstronomy and AstrophysicsSpace Physics (physics.space-ph)EVOLUTIONEarth's magnetic fieldQC Physics13. Climate actionSpace and Planetary Science[SDU]Sciences of the Universe [physics]Low-Coronal SignaturesCoronal mass ejectionsMAGNETOHYDRODYNAMIC MODELSInterplanetary spaceflightSpace science reviews
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