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Statements

Subject Item
n2:RIV%2F68378289%3A_____%2F14%3A00434199%21RIV15-AV0-68378289
rdf:type
skos:Concept n14:Vysledek
dcterms:description
Whistler-mode chorus emissions consist of individual wave packets exhibiting rising, falling tones or other spectral shapes (hooks or shapeless hiss) usually divided into two frequency bands separated by a gap at 1/2 of the electron cyclotron frequency (fce) close to the chorus source region. This configuration is often called banded chorus and it is correlated with the magnetic activity. Several theories have been published to explain how this specific configuration is generated. We present several tens of events of chorus emissions with more than two frequency bands and more than one gap that were found during more than 11 years of Cluster spacecraft measurements (from November 2000). Most of these “multi-banded emissions were observed within 10° of geomagnetic latitude, i.e., inside or very close to the chorus source region. Most of studied events propagate with oblique wave normal angles and were detected under disturbed geomagnetic conditions. Whistler-mode chorus emissions consist of individual wave packets exhibiting rising, falling tones or other spectral shapes (hooks or shapeless hiss) usually divided into two frequency bands separated by a gap at 1/2 of the electron cyclotron frequency (fce) close to the chorus source region. This configuration is often called banded chorus and it is correlated with the magnetic activity. Several theories have been published to explain how this specific configuration is generated. We present several tens of events of chorus emissions with more than two frequency bands and more than one gap that were found during more than 11 years of Cluster spacecraft measurements (from November 2000). Most of these “multi-banded emissions were observed within 10° of geomagnetic latitude, i.e., inside or very close to the chorus source region. Most of studied events propagate with oblique wave normal angles and were detected under disturbed geomagnetic conditions.
dcterms:title
Multi-banded structure of chorus-like emission Multi-banded structure of chorus-like emission
skos:prefLabel
Multi-banded structure of chorus-like emission Multi-banded structure of chorus-like emission
skos:notation
RIV/68378289:_____/14:00434199!RIV15-AV0-68378289
n3:aktivita
n15:I n15:P
n3:aktivity
I, P(7E12026)
n3:dodaniDat
n12:2015
n3:domaciTvurceVysledku
Macúšová, Eva n20:9496726
n3:druhVysledku
n5:D
n3:duvernostUdaju
n17:S
n3:entitaPredkladatele
n13:predkladatel
n3:idSjednocenehoVysledku
30935
n3:idVysledku
RIV/68378289:_____/14:00434199
n3:jazykVysledku
n4:eng
n3:klicovaSlova
cyclotrons; frequency measurement; magnetic confinement; magnetic separation; magnetosphere; physics; space vehicles
n3:klicoveSlovo
n10:frequency%20measurement n10:magnetic%20separation n10:magnetic%20confinement n10:physics n10:space%20vehicles n10:magnetosphere n10:cyclotrons
n3:kontrolniKodProRIV
[9BE4AF151044]
n3:mistoKonaniAkce
Beijing
n3:mistoVydani
New York
n3:nazevZdroje
General Assembly and Scientific Symposium (URSI GASS), 2014 XXXIth URSI
n3:obor
n7:BL
n3:pocetDomacichTvurcuVysledku
2
n3:pocetTvurcuVysledku
4
n3:projekt
n9:7E12026
n3:rokUplatneniVysledku
n12:2014
n3:tvurceVysledku
Pickett, J. S. Cornilleau-Wehrlin, N. Santolík, Ondřej Macúšová, Eva
n3:typAkce
n16:WRD
n3:zahajeniAkce
2014-08-16+02:00
s:numberOfPages
4
n21:doi
10.1109/URSIGASS.2014.6929889
n18:hasPublisher
IEEE
n19:isbn
978-1-4673-5225-3