Search results for " planetary"

showing 10 items of 5408 documents

On the importance of background subtraction in the analysis of coronal loops observed with TRACE

2010

In the framework of TRACE coronal observations, we compare the analysis and diagnostics of a loop after subtracting the background with two different and independent methods. The dataset includes sequences of images in the 171 A, 195 A filter bands of TRACE. One background subtraction method consists in taking as background values those obtained from interpolation between concentric strips around the analyzed loop. The other method is a pixel-to-pixel subtraction of the final image when the loop had completely faded out, already used by Reale & Ciaravella 2006. We compare the emission distributions along the loop obtained with the two methods and find that they are considerably differen…

PhysicsBackground subtractionTrace (linear algebra)Subtractionastrofisica Fisica solare Sun: corona Sun: X-rays gamma rays method: data analysisFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsSTRIPSCoronal loopFilter (signal processing)law.inventionComputational physicsLoop (topology)Settore FIS/05 - Astronomia E AstrofisicaAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencelawSolar and Stellar Astrophysics (astro-ph.SR)Interpolation
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Did the ancient crenarchaeal viruses from the dawn of life survive exceptionally well the eons of meteorite bombardment?

2009

The viruses of Crenarchaeota are unexpectedly diverse in their morphologies, and most have no, or few, genes related to bacterial, eukaryal, euryarchaeal, or other crenarchaeal viruses. Though several different virus morphotypes have been discovered in enrichment cultures of microbial communities collected from geothermally heated environments around the world, the origins of such differences are unknown. We present a model that combines consideration of Earth's geological history, the early emergence of hyperthermophiles, and the early formation of viruses from primordial genes with the intent to explain this vast diversity of crenarchaeal viruses. Several meteorite- or flood basalt-induce…

Extinction eventArchaeal VirusesbiologyEcologyvirusesCrenarchaeotaMeteoroidsrespiratory systembiology.organism_classificationExtinction BiologicalAgricultural and Biological Sciences (miscellaneous)HyperthermophileMeteoriteSpace and Planetary ScienceCrenarchaeotaEvolutionary biologyHost-Pathogen Interactionshuman activitiesAstrobiology
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The Managing and Restoring of Degraded Land in Post-Mining Areas

2022

Mining is an important branch of the economy, providing raw materials necessary for the economic and civilization development of the country [...]

Global and Planetary ChangeEcologyNature and Landscape ConservationLand
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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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Bibliometric analysis of publications by South African viticulture and oenology research centres

2012

We analysed the production, impact factor of, and scientific collaboration involved in viticulture and oenology articles associated with South African research centres published in international journals during the period 1990–2009. The articles under scrutiny were obtained from the Science Citation Index database, accessed via the Web of Knowledge platform. The search strategy employed specific viticulture and oenology terms and was restricted to the field ‘topic’. The results showed that 406 articles were published during the review period, with the most number of publications being in the South African Journal of Enology and Viticulture (n = 34), American Journal of Enology and Vit…

Bibliometric analysisScrutinyTECNOLOGIA DE ALIMENTOSSciencebibliometric indicatorsscientific publicationsLibrary scienceWineBibliometricsGeneral Biochemistry Genetics and Molecular Biologylcsh:Social SciencesSouth Africalcsh:Social sciences (General)Distillery Waste-WaterPatternslcsh:Sciencelcsh:Science (General)OenologyImpact FactorImpact factorCommunitiesScience Citation IndexInstitutional Collaborationviticulturelcsh:HInternationalizationGeographyScientific CollaborationCoauthorship NetworksGeneral Earth and Planetary Sciencesoenologylcsh:Qlcsh:H1-99ViticultureGeneral Agricultural and Biological SciencesResearch Collaborationlcsh:Q1-390South African Journal of Science
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Monochromatic Long-Period Seismicity Prior to the 2012 Earthquake Swarm at Little Sitkin Volcano, Alaska

2021

Detection of the earliest stages of unrest is one of the most challenging and yet critically needed aspects of volcano monitoring. We investigate a sequence of five unusual long-period (LP) earthquakes that occurred in the days prior to the onset of a months-long volcano-tectonic (VT) earthquake swarm beneath Little Sitkin volcano in the Aleutian Islands during late 2012. The long-period earthquakes had two distinctive characteristics: their signals were dominated by a monochromatic spectral peak at approximately 0.57 Hz and they had impulsive P and S-wave arrivals on a seismometer located on Amchitka Island 80 km to the southeast of the volcano. In each case, the monochromatic earthquakes …

Seismometerprecursory seismicitygeographygeography.geographical_feature_category010504 meteorology & atmospheric sciencesSciencevolcano seismologyQlong-period earthquakeInduced seismicity010502 geochemistry & geophysicsEarthquake swarm01 natural sciencesIntrusionearthquake swarmSillVolcanoresonanceLong periodGeneral Earth and Planetary SciencesMonochromatic colorSeismologyGeology0105 earth and related environmental sciencesFrontiers in Earth Science
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THE ACCELERATING JET OF 3C 279

2012

Analysis of the proper motions of the subparsec scale jet of the quasar 3C 279 at 15 GHz with the Very Long Baseline Array shows significant accelerations in four of nine superluminal features. Analysis of these motions is combined with the analysis of flux density light curves to constrain values of Lorentz factor and viewing angle (and their derivatives) for each component. The data for each of these components are consistent with significant changes to the Lorentz factor, viewing angle, and azimuthal angle, suggesting jet bending with changes in speed. We see that for these observed components Lorentz factors are in the range Γ = 10-41, viewing angles are in the range = 0.°1-5.°0, and in…

PhysicsSuperluminal motionLorentz transformationAstronomy and AstrophysicsAstrophysicsLight curveViewing anglePolarization (waves)symbols.namesakeLorentz factorFlow velocitySpace and Planetary ScienceAstronomiasymbolsVery Long Baseline ArrayThe Astronomical Journal
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Statistical upscaling of ecosystem CO2 fluxes across the terrestrial tundra and boreal domain: Regional patterns and uncertainties

2021

The regional variability in tundra and boreal carbon dioxide (CO2) fluxes can be high, complicating efforts to quantify sink-source patterns across the entire region. Statistical models are increasingly used to predict (i.e., upscale) CO2 fluxes across large spatial domains, but the reliability of different modeling techniques, each with different specifications and assumptions, has not been assessed in detail. Here, we compile eddy covariance and chamber measurements of annual and growing season CO2 fluxes of gross primary productivity (GPP), ecosystem respiration (ER), and net ecosystem exchange (NEE) during 1990–2015 from 148 terrestrial high-latitude (i.e., tundra and boreal) sites to a…

hiilidioksidi0106 biological sciences010504 meteorology & atmospheric sciencesBiomeikiroutaNORTHERN PEATLANDAtmospheric sciences01 natural sciencesCarbon Dioxide/analysisSoilremote sensingArctic/dk/atira/pure/sustainabledevelopmentgoals/climate_actionSDG 13 - Climate ActionEXCHANGEComputingMilieux_MISCELLANEOUSGeneral Environmental ScienceARCTIC TUNDRA[SDU.OCEAN]Sciences of the Universe [physics]/Ocean Atmospherearktinen alueGlobal and Planetary ChangeCLIMATE-CHANGEEcologyCARBON-DIOXIDE BALANCEUncertaintyCO balancekasvihuonekaasutBLACK SPRUCE FORESTgreenhouse gasTerrestrial ecosystemSeasonsEcosystem respiration1171 GeosciencesEddy covariancepaikkatietoanalyysiSOIL-MOISTURE010603 evolutionary biology114 Physical sciencesEnvironmental Chemistry[SDU.ENVI]Sciences of the Universe [physics]/Continental interfaces environmentTundraEcosystem0105 earth and related environmental sciencesCO2 balanceReproducibility of ResultsENERGY FLUXES15. Life on landTundraPERMAFROST CARBONCarbonlandBorealhiilinielut13. Climate actionGROWING-SEASONSpatial ecologyEnvironmental scienceSpatial variabilitykaukokartoitusempiricalpermafrost
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The B0.5IVe CoRoT target HD 49330. I. Photometric analysis from CoRoT data

2009

International audience; Context: Be stars undergo outbursts producing a circumstellar disk from the ejected material. The beating of non-radial pulsations has been put forward as a possible mechanism of ejection. Aims: We analyze the pulsational behavior of the early B0.5IVe star HD 49330 observed during the first CoRoT long run towards the Galactical anticenter (LRA1). This Be star is located close to the lower edge of the beta Cephei instability strip in the HR diagram and showed a 0.03 mag outburst during the CoRoT observations. It is thus an ideal case for testing the aforementioned hypothesis. Methods: We analyze the CoRoT light curve of HD 49330 using Fourier methods and non-linear le…

PhysicsBe starHertzsprung–Russell diagramAstrophysics::High Energy Astrophysical PhenomenaAstronomyAstronomy and AstrophysicsContext (language use)AstrophysicsLight curveStarssymbols.namesakeAmplitudeSpace and Planetary Science[SDU]Sciences of the Universe [physics]symbolsAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsEmission spectrumInstability strip[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics::Galaxy Astrophysics
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Measuring the electron temperatures of coronal mass ejections with future space-based multi-channel coronagraphs: a numerical test

2018

Context. The determination from coronagraphic observations of physical parameters of the plasma embedded in coronal mass ejections (CMEs) is of crucial importance for our understanding of the origin and evolution of these phenomena. Aims. The aim of this work is to perform the first ever numerical simulations of a CME as it will be observed by future two-channel (visible light VL and UV Ly-α) coronagraphs, such as the Metis instrument on-board ESA-Solar Orbiter mission, or any other future coronagraphs with the same spectral band-passes. These simulations are then used to test and optimize the plasma diagnostic techniques to be applied to future observations of CMEs. Methods. The CME diagno…

010504 meteorology & atmospheric sciencesSun: coronal mass ejections (CMEs)Plasma parametersT-NDASContext (language use)Astrophysics01 natural sciencessymbols.namesakeMethods: data analysis0103 physical sciencesRadiative transferCoronal mass ejectionAstrophysics::Solar and Stellar AstrophysicsQB Astronomydata analysis [Methods]010303 astronomy & astrophysicsQCQB0105 earth and related environmental sciencesPhysicsUV radiation [Sun]numerical [Methods]Methods: numericalAstronomy and AstrophysicsPlasmaSun: UV radiationPolarization (waves)coronal mass ejections (CMEs) [Sun]Computational physicsQC PhysicsPlasmasSpace and Planetary SciencePhysics::Space PhysicssymbolsMagnetohydrodynamicsDoppler effectAstronomy & Astrophysics
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