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  • Radio spectra, observed during solar flares, are usually very complex (many bursts and fine structures). We have developed a new method to separate them into individual bursts and analyze them separately. The method is used in the analysis of the 0.8–2.0 GHz radio spectrum of the April 11, 2001 event, which was rich in drifting pulsating structures (DPSs). Using this method we showed that the complex radio spectrum consists of at least four DPSs separated with respect to their different frequency drifts (-115, -36, -23, and -11 MHz/s). These DPSs indicate a presence of at least four plasmoids expected to be formed in a flaring current sheet. These plasmoids produce the radio emission on close frequencies giving thus a mixture of superimposed DPSs observed in the radio spectrum.
  • Radio spectra, observed during solar flares, are usually very complex (many bursts and fine structures). We have developed a new method to separate them into individual bursts and analyze them separately. The method is used in the analysis of the 0.8–2.0 GHz radio spectrum of the April 11, 2001 event, which was rich in drifting pulsating structures (DPSs). Using this method we showed that the complex radio spectrum consists of at least four DPSs separated with respect to their different frequency drifts (-115, -36, -23, and -11 MHz/s). These DPSs indicate a presence of at least four plasmoids expected to be formed in a flaring current sheet. These plasmoids produce the radio emission on close frequencies giving thus a mixture of superimposed DPSs observed in the radio spectrum. (en)
Title
  • Separation of solar radio bursts in a complex spectrum
  • Separation of solar radio bursts in a complex spectrum (en)
skos:prefLabel
  • Separation of solar radio bursts in a complex spectrum
  • Separation of solar radio bursts in a complex spectrum (en)
skos:notation
  • RIV/67985815:_____/11:00360457!RIV12-AV0-67985815
http://linked.open...avai/predkladatel
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • P(IAA300030701), Z(AV0Z10030501)
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
  • 228914
http://linked.open...ai/riv/idVysledku
  • RIV/67985815:_____/11:00360457
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • Sun; flares; radio radiation (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...ontrolniKodProRIV
  • [72D8F938ED52]
http://linked.open...v/mistoKonaniAkce
  • Giardini Naxos
http://linked.open...i/riv/mistoVydani
  • Cambridge
http://linked.open...i/riv/nazevZdroje
  • Advances in Plasma Astrophysics
http://linked.open...in/vavai/riv/obor
http://linked.open...ichTvurcuVysledku
http://linked.open...cetTvurcuVysledku
http://linked.open...vavai/riv/projekt
http://linked.open...UplatneniVysledku
http://linked.open...iv/tvurceVysledku
  • Karlický, Marian
  • Jiřička, Karel
  • Mészárosová, Hana
  • Rybák, J.
http://linked.open...vavai/riv/typAkce
http://linked.open.../riv/zahajeniAkce
http://linked.open...n/vavai/riv/zamer
number of pages
http://purl.org/ne...btex#hasPublisher
  • Cambridge University Press
https://schema.org/isbn
  • 9780521197410
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