Time lags in hard X-ray emission from solar flares according to data from the Sneg-2M3 instruments

Details Time lags in hard X-ray emission from solar flares according to data from the Sneg-2M3 instruments Time lags in hard X-ray emission from solar flares according to data from the Sneg-2M3 instruments

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989kosis..27..907b&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 27, Nov.-Dec. 1989, p. 907-917. In Russian.

Physics

1

Satellite-Borne Instruments, Solar Flares, Solar X-Rays, Time Lag, Algorithms, Correlation, Magnetically Trapped Particles, Statistical Analysis

Scientific paper

The energy dependence of time lags arising in the electron trap models for solar hard X-ray bursts is investigated, and an algorithm for the statistical analysis of such time lags is proposed. An analysis is made of 80 flares detected with the Sneg-2M3 instruments on the Venera 13 and 14 probes. Statistically significant time lags were observed in two of these flares.

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