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  • One of the objectives of the Cluster mission is to study sources of various electromagnetic waves using the four satellites. This paper describes the methods we have applied to data recorded from the STAFF spectrum analyser. This instrument provides the cross spectral matrix of three magnetic and two electric field components. This spectral matrix is analysed to determine, for each satellite, the direction of the wave normal relative to the Earth's magnetic field as a function of frequency and of time. Due to the Cluster orbit, chorus emissions are often observed close to perigee, and the data analysis determines the direction of these waves. Three events observed during different levels of magnetic activity are reported. It is shown that the component of the Poynting vector parallel to the magnetic field changes its sense when the satellites cross the magnetic equator, which indicates that the chorus waves propagate away from the equator. Detailed analysis indicates that the source is located in clos
  • One of the objectives of the Cluster mission is to study sources of various electromagnetic waves using the four satellites. This paper describes the methods we have applied to data recorded from the STAFF spectrum analyser. This instrument provides the cross spectral matrix of three magnetic and two electric field components. This spectral matrix is analysed to determine, for each satellite, the direction of the wave normal relative to the Earth's magnetic field as a function of frequency and of time. Due to the Cluster orbit, chorus emissions are often observed close to perigee, and the data analysis determines the direction of these waves. Three events observed during different levels of magnetic activity are reported. It is shown that the component of the Poynting vector parallel to the magnetic field changes its sense when the satellites cross the magnetic equator, which indicates that the chorus waves propagate away from the equator. Detailed analysis indicates that the source is located in clos (en)
Title
  • Source location of chorus emissions observed by Cluster.
  • Source location of chorus emissions observed by Cluster. (en)
skos:prefLabel
  • Source location of chorus emissions observed by Cluster.
  • Source location of chorus emissions observed by Cluster. (en)
skos:notation
  • RIV/68378289:_____/03:04030023!RIV/2004/AV0/A04004/N
http://linked.open.../vavai/riv/strany
  • 473;480
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • P(GA202/03/0832), P(ME 650), Z(AV0Z3042911), Z(MSM 113200004)
http://linked.open...iv/cisloPeriodika
  • N/A
http://linked.open...vai/riv/dodaniDat
http://linked.open...aciTvurceVysledku
http://linked.open.../riv/druhVysledku
http://linked.open...iv/duvernostUdaju
http://linked.open...titaPredkladatele
http://linked.open...dnocenehoVysledku
  • 627956
http://linked.open...ai/riv/idVysledku
  • RIV/68378289:_____/03:04030023
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • magnetospheric physics; space plasma physics (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • DE - Spolková republika Německo
http://linked.open...ontrolniKodProRIV
  • [ACBBFF036CCA]
http://linked.open...i/riv/nazevZdroje
  • Annales Geophysicae
http://linked.open...in/vavai/riv/obor
http://linked.open...ichTvurcuVysledku
http://linked.open...cetTvurcuVysledku
http://linked.open...ocetUcastnikuAkce
http://linked.open...nichUcastnikuAkce
http://linked.open...vavai/riv/projekt
http://linked.open...UplatneniVysledku
http://linked.open...v/svazekPeriodika
  • 21
http://linked.open...iv/tvurceVysledku
  • Parrot, M.
  • Santolík, Ondřej
  • Maksimovic, M.
  • Cornilleau-Wehrlin, N.
  • Harvey, C. C.
http://linked.open...n/vavai/riv/zamer
issn
  • 0992-7689
number of pages
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