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 language | English |
|---|---|
| Journal | Astronomy Letters-a Journal of Astronomy and Space Astrophysics |
| Volume | 28 |
| Issue number | 6 |
| Pages (from-to) | 397-400 |
| ISSN | 1063-7737 |
| Publication status | Published - 2002 |
Keywords
- magnetic loops
- quasi-periodic pulsations
- solar flares
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