An analysis of fine structures in a solar radio burst at 10 cm and a coexisting hard X-ray flare

Details An analysis of fine structures in a solar radio burst at 10 cm and a coexisting hard X-ray flare An analysis of fine structures in a solar radio burst at 10 cm and a coexisting hard X-ray flare

Feb 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cha%26a..23..208t&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 23, Issue 2, p. 208-220.

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

The solar burst event of 1992-06-07 is analyzed in this paper using HXR material of the Yohkoh satellite and radio data at 2840 MHz observed at Beijing Astronomical Observatory. The results show that during the impulsive phase, the pulsational component had two time scales, a longer one of about 30s, and a shorter one of 1-4s. The pulsations on the longer scale are found to be correlated with a series of variations in the HXR images of the source region. A physical picture comprising loop-loop interaction and MHD oscillation modulation is presented.

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