The coronal oscillations revealed by solar hard X-ray bursts

Details The coronal oscillations revealed by solar hard X-ray bursts The coronal oscillations revealed by solar hard X-ray bursts

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986chjss...6q.169x&link_type=abstract

Chinese Journal of Space Science, vol. 6, no. 3, 1986, p. 169-176. In Chinese, with abstract in English.

Physics

Satellite-Borne Instruments, Solar Corona, Solar Flares, Solar Oscillations, Solar X-Rays, Solar Maximum Mission

Scientific paper

During the 21st solar activity cycle the HXRBS aboard SMM satellite and the HXM on HINOTORI spacecraft detected several thousand hard X-ray solar flares. Studies of the temporal properties of these events had revealed hundreds of examples of fast spikes with durations of less 1 sec. Some of these observations were analyzed, and it was found that they have four common characteristics. In particular, quasi-periodic oscillations suggested the possibility of existing oscillations in the corona. The characteristics of the oscillations were studied and their periods derived. The conditions of oscillation trapping are also discussed.

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