Temporal characteristics of solar hard X-ray/gamma-ray bursts observed by PHEBUS

Details Temporal characteristics of solar hard X-ray/gamma-ray bursts observed by PHEBUS Temporal characteristics of solar hard X-ray/gamma-ray bursts observed by PHEBUS

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993adspr..13..171t&link_type=abstract

Advances in Space Research, Volume 13, Issue 9, p. 171-174.

Computer Science

6

Scientific paper

The PHEBUS observations show that short duration hard X-ray/gamma-ray
bursts detected above ⋍ 70 keV generally exhibit subsecond time
structures. On the contrary, long duration events do not show fast time
variations and usually consist in ⋍ one minute duration peaks
superposed on a less intense and slowly varying component.

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