Observations of fine time structure in solar flare hard X-ray bursts

Details Observations of fine time structure in solar flare hard X-ray bursts Observations of fine time structure in solar flare hard X-ray bursts

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...86..367h&link_type=abstract

(Japan Society for the Promotion of Science and National Science Foundation, U.S.-Japan Seminar on the Recent Advances in the Un

Astronomy and Astrophysics

Astronomy

7

Fine Structure, Solar Flares, Solar X-Rays, Temporal Resolution, Bursts, Electron Acceleration, Spaceborne Astronomy

Scientific paper

Hard X-ray (⪆100 keV) time histories of solar flares which occurred on 1978 December 4 and 1979 February 18 are presented. The first flare was observed by 3 identical instruments from near-earth orbit (Prognoz 7) and interplanetary space (Venera 11 and 12). Fine time structure is present down to the 55 ms level for the e-folding rise and fall times. These data may be used to localize the emission region by the method of arrival time analysis.

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