Observation of quasi-periodic pulsations in the solar flare SF 900610 |
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Authors: | O V Terekhov A V Shevchenko A G Kuz’min S Yu Sazonov R A Sunyaev N Lund |
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Institution: | (1) Space Research Institute, Russian Academy of Sciences, ul. Profsoyuznaya 84/32, Moscow, 117810, Russia;(2) Danish Space Research Institute, Copenhagen, Denmark |
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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 ~5% of the total flare intensity. An analysis of the data showed the characteristic size of the magnetic loop responsible for these pulsations to be ~(1–3)×1010 cm. |
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Keywords: | solar flares quasi-periodic pulsations magnetic loops |
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