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Statements

Subject Item
n2:RIV%2F68378289%3A_____%2F11%3A00396493%21RIV14-AV0-68378289
rdf:type
skos:Concept n10:Vysledek
dcterms:description
Whistler-mode chorus emissions are one of the most significant mechanisms causing the acceleration of electrons in the outer Van Allen radiation belt to relativistic energies. They consist of individual wave packets divided into two frequency bands separated close to the source region by a gap at 1/2 of the electron cyclotron frequency (fce). This configuration is called banded chorus and it is correlated with magnetic activity. Landau damping is one of the possible explanations describing the existence of the gap. On the other hand, the role of ducts in its formation was also discussed. We present several events of chorus combined with noisy or shapeless chorus-like emissions that are arranged in three or more frequency bands with two or more gaps and are observed mostly in a magnetic latitude range from 3 to 10 degrees on the both sides of the equator. We investigate possible influences of the magnetic local time (MLT), the Kp index, the McIlwain parameter and the plasma density on the formation of these multi-band emissions. Whistler-mode chorus emissions are one of the most significant mechanisms causing the acceleration of electrons in the outer Van Allen radiation belt to relativistic energies. They consist of individual wave packets divided into two frequency bands separated close to the source region by a gap at 1/2 of the electron cyclotron frequency (fce). This configuration is called banded chorus and it is correlated with magnetic activity. Landau damping is one of the possible explanations describing the existence of the gap. On the other hand, the role of ducts in its formation was also discussed. We present several events of chorus combined with noisy or shapeless chorus-like emissions that are arranged in three or more frequency bands with two or more gaps and are observed mostly in a magnetic latitude range from 3 to 10 degrees on the both sides of the equator. We investigate possible influences of the magnetic local time (MLT), the Kp index, the McIlwain parameter and the plasma density on the formation of these multi-band emissions.
dcterms:title
Multi-band Whistler-mode Chorus Emissions Observed by the Cluster Spacecraft Multi-band Whistler-mode Chorus Emissions Observed by the Cluster Spacecraft
skos:prefLabel
Multi-band Whistler-mode Chorus Emissions Observed by the Cluster Spacecraft Multi-band Whistler-mode Chorus Emissions Observed by the Cluster Spacecraft
skos:notation
RIV/68378289:_____/11:00396493!RIV14-AV0-68378289
n10:predkladatel
n11:ico%3A68378289
n3:aktivita
n4:S n4:Z
n3:aktivity
S, Z(AV0Z30420517)
n3:dodaniDat
n8:2014
n3:domaciTvurceVysledku
n13:9496726 Macúšová, Eva
n3:druhVysledku
n20:D
n3:duvernostUdaju
n14:S
n3:entitaPredkladatele
n9:predkladatel
n3:idSjednocenehoVysledku
214188
n3:idVysledku
RIV/68378289:_____/11:00396493
n3:jazykVysledku
n21:eng
n3:klicovaSlova
Cluster spacecraft; Whistler-mode chorus emissions
n3:klicoveSlovo
n16:Whistler-mode%20chorus%20emissions n16:Cluster%20spacecraft
n3:kontrolniKodProRIV
[7BDC450CBFBD]
n3:mistoKonaniAkce
Prague
n3:mistoVydani
Praha
n3:nazevZdroje
WDS'11 Proceedings of Contributed Papers: Part II – Physics of Plasmas and Ionized Media
n3:obor
n15:BL
n3:pocetDomacichTvurcuVysledku
2
n3:pocetTvurcuVysledku
2
n3:rokUplatneniVysledku
n8:2011
n3:tvurceVysledku
Santolík, Ondřej Macúšová, Eva
n3:typAkce
n5:WRD
n3:zahajeniAkce
2011-05-31+02:00
n3:zamer
n12:AV0Z30420517
s:numberOfPages
6
n17:hasPublisher
Matfyzpress
n19:isbn
978-80-7378-185-9