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Statements

Subject Item
n2:RIV%2F68378289%3A_____%2F03%3A04033512%21RIV%2F2004%2FAV0%2FA04004%2FN
rdf:type
skos:Concept n18:Vysledek
dcterms:description
The noise bands at lower hybrid resonance (LHR) frequency at a satellite position have already been observed and described. Observations onboard the MAGION 5 satellite revealed oblique noise bands above the local LHR frequency. Examples of such oblique bands, both in review (large time-scale) spectrograms, and in detailed (small time-scale) spectrograms are presented. Based on ray-tracing simulations, an explanation of these oblique bands is suggested. We show that they are formed due to the separation of nonducted whistler mode waves of different frequencies propagating near the so-called resonance cone. The influence of plasmaspheric disturbances upon these emissions is also discussed. We suggest that oblique noise bands are mainly formed under quiet conditions, when indistinct plasmapause is situated at higher L shells. The noise bands at lower hybrid resonance (LHR) frequency at a satellite position have already been observed and described. Observations onboard the MAGION 5 satellite revealed oblique noise bands above the local LHR frequency. Examples of such oblique bands, both in review (large time-scale) spectrograms, and in detailed (small time-scale) spectrograms are presented. Based on ray-tracing simulations, an explanation of these oblique bands is suggested. We show that they are formed due to the separation of nonducted whistler mode waves of different frequencies propagating near the so-called resonance cone. The influence of plasmaspheric disturbances upon these emissions is also discussed. We suggest that oblique noise bands are mainly formed under quiet conditions, when indistinct plasmapause is situated at higher L shells.
dcterms:title
Oblique noise bands above local LHR frequency. Oblique noise bands above local LHR frequency.
skos:prefLabel
Oblique noise bands above local LHR frequency. Oblique noise bands above local LHR frequency.
skos:notation
RIV/68378289:_____/03:04033512!RIV/2004/AV0/A04004/N
n3:strany
1253;1258
n3:aktivita
n16:Z n16:P
n3:aktivity
P(IAA3042703), P(OK 162), Z(AV0Z3042911)
n3:cisloPeriodika
5
n3:dodaniDat
n6:2004
n3:domaciTvurceVysledku
n7:1168800 n7:1231979
n3:druhVysledku
n4:J
n3:duvernostUdaju
n13:S
n3:entitaPredkladatele
n11:predkladatel
n3:idSjednocenehoVysledku
618837
n3:idVysledku
RIV/68378289:_____/03:04033512
n3:jazykVysledku
n8:eng
n3:klicovaSlova
magnetospheric physics; plasmasphere; wave propagation
n3:klicoveSlovo
n12:wave%20propagation n12:magnetospheric%20physics n12:plasmasphere
n3:kodStatuVydavatele
GB - Spojené království Velké Británie a Severního Irska
n3:kontrolniKodProRIV
[B3841D16C439]
n3:nazevZdroje
Advances in space research
n3:obor
n15:DG
n3:pocetDomacichTvurcuVysledku
2
n3:pocetTvurcuVysledku
3
n3:pocetUcastnikuAkce
0
n3:pocetZahranicnichUcastnikuAkce
0
n3:projekt
n5:OK%20162 n5:IAA3042703
n3:rokUplatneniVysledku
n6:2003
n3:svazekPeriodika
31
n3:tvurceVysledku
Chum, Jaroslav Shklyar, D. Jiříček, František
n3:zamer
n17:AV0Z3042911
s:issn
0273-1177
s:numberOfPages
6