Observation of quasi-periodic pulsations in the solar flare SF 900610

O.V. Terekhov, A.V. Shevchenko, A.G. Kuz'min, S.Y. Sazonov, R.A. Sunyaev, Niels Lund

Research output: Contribution to journalJournal articleResearchpeer-review

Abstract

A quasi-periodic component was found at the maximum of the X-ray light curve for the June 10, 1990 solar flare detected by the Granat observatory. The pulsation period was 143.2 +/- 0.8 s. The intensity of the pulsing component is not constant; the maximum amplitude of the pulsations is similar to5% of the total flare intensity. An analysis of the data showed the characteristic size of the magnetic loop responsible for these pulsations to be similar to(1-3) x 10(10) cm.
Original languageEnglish
JournalAstronomy Letters-a Journal of Astronomy and Space Astrophysics
Volume28
Issue number6
Pages (from-to)397-400
ISSN1063-7737
Publication statusPublished - 2002

Keywords

  • magnetic loops
  • quasi-periodic pulsations
  • solar flares

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