| Autor: |
Bakunin, L., Ledenev, V., Nefedyev, V., Potapov, N., Smolkov, G., Uralov, A., Chernov, G., Fomichev, V., Melnikov, V., Podstrigach, T., Epifanova, O., Khokhlov, A., Enome, Sh. |
| Zdroj: |
Solar Physics; Sep1991, Vol. 135 Issue 1, p107-129, 23p |
| Abstrakt: |
A complex analysis in different radio ranges of the evolutionary features of the 3 February, 1983 flare (05∶43-06∶19-08∶12 UT) has shown that the flare is a prolonged (∼ 15 hr) process of energy release and particle acceleration that gradually extends to still greater zones of the active region (AR) magnetosphere in both area and altitude. Observations from the Siberian Solar Radio Telescope obtained at λ = 5.2 cm indicate that the flare was preceded by quasi-periodical brightness enhancements with a period of 6-7 min of two sources of size 20″ and with a brightness temperature of ∼ 107 K. During the flare maximum phase, a type II burst with harmonic structure and the subsequent type FC II continuum with fine structure were both observed in the meter band. It has been found that zebra-structure appearances correlate with the Hα-flare kernel brightenings at loop tops. The observed characteristics of the type II burst and of the type FC II continuum treated in this paper are interpreted in terms of the complex flare flow structure, involving forward and backward shock waves. [ABSTRACT FROM AUTHOR] |
| Databáze: |
Complementary Index |
| Externí odkaz: |
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