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Statements

Subject Item
n2:RIV%2F68378289%3A_____%2F08%3A00313557%21RIV09-AV0-68378289
rdf:type
skos:Concept n14:Vysledek
dcterms:description
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. Experimentální studie plazmatických vln v magnetosféře Saturnu. 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.
dcterms:title
Analysis of plasma waves observed in the inner Saturn magnetosphere Analysis of plasma waves observed in the inner Saturn magnetosphere Analýza plazmových vln pozorovaných ve vnitřní magnetosféře Saturnu
skos:prefLabel
Analysis of plasma waves observed in the inner Saturn magnetosphere Analysis of plasma waves observed in the inner Saturn magnetosphere Analýza plazmových vln pozorovaných ve vnitřní magnetosféře Saturnu
skos:notation
RIV/68378289:_____/08:00313557!RIV09-AV0-68378289
n3:aktivita
n6:P n6:Z
n3:aktivity
P(IAA301120601), P(ME 842), Z(AV0Z30420517)
n3:cisloPeriodika
9
n3:dodaniDat
n11:2009
n3:domaciTvurceVysledku
n12:9496726
n3:druhVysledku
n9:J
n3:duvernostUdaju
n17:S
n3:entitaPredkladatele
n5:predkladatel
n3:idSjednocenehoVysledku
355861
n3:idVysledku
RIV/68378289:_____/08:00313557
n3:jazykVysledku
n8:eng
n3:klicovaSlova
Saturn magnetosphere; plasma waves
n3:klicoveSlovo
n10:plasma%20waves n10:Saturn%20magnetosphere
n3:kodStatuVydavatele
US - Spojené státy americké
n3:kontrolniKodProRIV
[9116E5681716]
n3:nazevZdroje
Annales Geophysicae
n3:obor
n15:BL
n3:pocetDomacichTvurcuVysledku
1
n3:pocetTvurcuVysledku
6
n3:projekt
n13:IAA301120601 n13:ME%20842
n3:rokUplatneniVysledku
n11:2008
n3:svazekPeriodika
26
n3:tvurceVysledku
Gurnett, D. A. Santolík, Ondřej Hospodarsky, G. B. Coates, A. J. Menietti, J. D. Rymer, A. M.
n3:wos
000259702800009
n3:zamer
n18:AV0Z30420517
s:issn
0992-7689
s:numberOfPages
14