A hard X-ray observation of a solar flare with 100 MS time resolution

Details A hard X-ray observation of a solar flare with 100 MS time resolution A hard X-ray observation of a solar flare with 100 MS time resolution

Apr 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...52..107h&link_type=abstract

Solar Physics, vol. 52, Apr. 1977, p. 107-116. Centre National d'Etudes Spatiales

Astronomy and Astrophysics

Astronomy

5

Solar Flares, Solar X-Rays, X Ray Astronomy, Atmospheric Scattering, Balloon-Borne Instruments, Collimators, Decimeter Waves, Solar Radio Bursts

Scientific paper

A solar flare which occurred on July 4, 1974, was observed in hard X-rays with a balloon-borne detector. When analyzed with a time resolution of 100 ms, four 2-sec-long spikes are observed, which are correlated with decimetric emission. Spectral analysis shows that the hardest X-rays were produced during the decay phase of the burst, when the microwave emission reached its peak, It is argued that the fine time structure could either be a bounce time effect or be due to the electron acceleration mechanism.

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