An observational analysis of solar microflare phenomena of new type at decimeter wavelength.

Details An observational analysis of solar microflare phenomena of new type at decimeter wavelength. An observational analysis of solar microflare phenomena of new type at decimeter wavelength.

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996acaps..16..421x&link_type=abstract

Acta Astrophys. Sin., Vol. 16, No. 4, p. 421 - 427

Astronomy and Astrophysics

Astrophysics

1

Solar Flares: Radio Radiation, Solar Radio Bursts: Fine Structure

Scientific paper

The radio and optical properties of a group of short decimeter wave (1.42 MHz) solar microflares are presented. The event consists of 53 radio fast fine structure in a quasi-periodic pulsation train superimposed on the radio continuum emission. This event takes place in the active region 7646 where two newly emerging groups of small sunspots with complex polarities and multiple reconnection of multiplex cross magnetic loops may occur. The authors discuss qualitatively the mechanism of the occurrence and give support to the theoretical model of current loop explosive coalescence.

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