About: Analysis of plasma waves observed in the inner Saturn magnetosphere

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An Entity of Type : http://linked.opendata.cz/ontology/domain/vavai/Vysledek, within Data Space : linked.opendata.cz associated with source document(s)

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rdf:type	skos:Concept http://linked.opendata.cz/ontology/domain/vavai/Vysledek
Description	Experimentální studie plazmatických vln v magnetosféře Saturnu. (cs) Plasma waves observed in the Saturn magnetosphere provide an indication of the plasma population present in the rotationally dominated inner magnetosphere. Electrostatic cyclotron emissions often with harmonics and whistler mode emission are a common feature of Saturn’s inner magnetosphere. The electron observations for a region near 5RS outside and near a plasma injection region indicate a cooler low-energy (<100 eV), nearly isotropic plasma, and a much warmer (E>1000 eV) more pancake or butterfly distribution. We model the electron plasma distributions to conduct a linear dispersion analysis of the wave modes. The results suggest that the electrostatic electron cyclotron emissions can be generated by phase space density gradients associated with a loss cone that may be up to 20 wide. This loss cone is sometimes, but not always, observed because the field of view of the electron detectors does not include the magnetic field line at the time of the observations. Plasma waves observed in the Saturn magnetosphere provide an indication of the plasma population present in the rotationally dominated inner magnetosphere. Electrostatic cyclotron emissions often with harmonics and whistler mode emission are a common feature of Saturn’s inner magnetosphere. The electron observations for a region near 5RS outside and near a plasma injection region indicate a cooler low-energy (<100 eV), nearly isotropic plasma, and a much warmer (E>1000 eV) more pancake or butterfly distribution. We model the electron plasma distributions to conduct a linear dispersion analysis of the wave modes. The results suggest that the electrostatic electron cyclotron emissions can be generated by phase space density gradients associated with a loss cone that may be up to 20 wide. This loss cone is sometimes, but not always, observed because the field of view of the electron detectors does not include the magnetic field line at the time of the observations. (en)
Title	Analysis of plasma waves observed in the inner Saturn magnetosphere Analysis of plasma waves observed in the inner Saturn magnetosphere (en) Analýza plazmových vln pozorovaných ve vnitřní magnetosféře Saturnu (cs)
skos:prefLabel	Analysis of plasma waves observed in the inner Saturn magnetosphere Analysis of plasma waves observed in the inner Saturn magnetosphere (en) Analýza plazmových vln pozorovaných ve vnitřní magnetosféře Saturnu (cs)
skos:notation	RIV/68378289:_____/08:00313557!RIV09-AV0-68378289
http://linked.open...avai/riv/aktivita	P Z
http://linked.open...avai/riv/aktivity	P(IAA301120601), P(ME 842), Z(AV0Z30420517)
http://linked.open...iv/cisloPeriodika	9
http://linked.open...vai/riv/dodaniDat	2009
http://linked.open...aciTvurceVysledku	Santolík, Ondřej
http://linked.open.../riv/druhVysledku	J - Článek v odborném periodiku
http://linked.open...iv/duvernostUdaju	S - Úplné a pravdivé údaje nepodléhající ochraně podle zvláštních právních předpisů
http://linked.open...titaPredkladatele	Ústav fyziky atmosféry AV ČR, v. v. i.
http://linked.open...dnocenehoVysledku	355861
http://linked.open...ai/riv/idVysledku	RIV/68378289:_____/08:00313557
http://linked.open...riv/jazykVysledku	eng - angličtina
http://linked.open.../riv/klicovaSlova	Saturn magnetosphere; plasma waves (en)
http://linked.open.../riv/klicoveSlovo	Saturn magnetosphere plasma waves
http://linked.open...odStatuVydavatele	US - Spojené státy americké
http://linked.open...ontrolniKodProRIV	[9116E5681716]
http://linked.open...i/riv/nazevZdroje	Annales Geophysicae
http://linked.open...in/vavai/riv/obor	BL
http://linked.open...ichTvurcuVysledku	1 (xsd:int)
http://linked.open...cetTvurcuVysledku	6 (xsd:int)
http://linked.open...vavai/riv/projekt	http://linked.opendata.cz/resource/domain/vavai/projekt/ME%20842 Investigation of plasma waves in the magnetosphere and in the solar wind
http://linked.open...UplatneniVysledku	2008
http://linked.open...v/svazekPeriodika	26
http://linked.open...iv/tvurceVysledku	Santolík, Ondřej Gurnett, D. A. Coates, A. J. Hospodarsky, G. B. Menietti, J. D. Rymer, A. M.
http://linked.open...ain/vavai/riv/wos	000259702800009
http://linked.open...n/vavai/riv/zamer	Studium atmosférického obalu Země v interakci s pozemskými a kosmickými vlivy
issn	0992-7689
number of pages	14 (xsd:int)
is http://linked.open...avai/riv/vysledek of	Analysis of plasma waves observed in the inner Saturn magnetosphere Analysis of plasma waves observed in the inner Saturn magnetosphere Analysis of plasma waves observed in the inner Saturn magnetosphere Analysis of plasma waves observed in the inner Saturn magnetosphere

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