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Description
  • This paper is related to the propagation characteristics of a chorus emission recorded simultaneously by the 4 satellites of the CLUSTER mission on 29 October 2001 between 01:00 and 05:00 UT. During this day, the spacecraft (SC) 1, 2, and 4 are relatively close to each other but SC3 has been delayed by half an hour. We use the data recorded aboard CLUSTER by the STAFF spectrum analyser. This instrument provides the cross spectral matrix of three magnetic and two electric field components. Dedicated software processes this spectral matrix in order to determine the wave normal directions relative to the Earth's magnetic field. This calculation is done for the 4 satellites at different times and different frequencies and allows us to check the directions of these waves. Measurements around the magnetic equator show that the parallel component of the Poynting vector changes its sign when the satellites cross the equator region. It indicates that the chorus waves propagate away from this region which is co
  • This paper is related to the propagation characteristics of a chorus emission recorded simultaneously by the 4 satellites of the CLUSTER mission on 29 October 2001 between 01:00 and 05:00 UT. During this day, the spacecraft (SC) 1, 2, and 4 are relatively close to each other but SC3 has been delayed by half an hour. We use the data recorded aboard CLUSTER by the STAFF spectrum analyser. This instrument provides the cross spectral matrix of three magnetic and two electric field components. Dedicated software processes this spectral matrix in order to determine the wave normal directions relative to the Earth's magnetic field. This calculation is done for the 4 satellites at different times and different frequencies and allows us to check the directions of these waves. Measurements around the magnetic equator show that the parallel component of the Poynting vector changes its sign when the satellites cross the equator region. It indicates that the chorus waves propagate away from this region which is co (en)
Title
  • Magnetospherically reflected chorus waves revealed by ray tracing with CLUSTER data.
  • Magnetospherically reflected chorus waves revealed by ray tracing with CLUSTER data. (en)
skos:prefLabel
  • Magnetospherically reflected chorus waves revealed by ray tracing with CLUSTER data.
  • Magnetospherically reflected chorus waves revealed by ray tracing with CLUSTER data. (en)
skos:notation
  • RIV/68378289:_____/03:04030022!RIV/2004/AV0/A04004/N
http://linked.open.../vavai/riv/strany
  • 1111;1120
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
  • 614145
http://linked.open...ai/riv/idVysledku
  • RIV/68378289:_____/03:04030022
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • magnetospheric physics; ionosphere; radio science (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • DE - Spolková republika Německo
http://linked.open...ontrolniKodProRIV
  • [ABFE52D506A1]
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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