Gamma-ray bursts - Experimental data in support of a heliospheric origin

Details Gamma-ray bursts - Experimental data in support of a heliospheric origin Gamma-ray bursts - Experimental data in support of a heliospheric origin

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982kosis..20...89k&link_type=abstract

Kosmicheskie Issledovaniia, vol. 20, Jan.-Feb. 1982, p. 89-96. In Russian.

Physics

1

Celestial Sphere, Gamma Ray Bursts, Heliosphere, Solar Magnetic Field, Solar Radiation, Current Sheets, Galactic Radiation, Pair Production, Solar Activity Effects

Scientific paper

The distribution of approximately 70 gamma-ray bursts on the celestial sphere relative to the solar-equator plane is examined, and two basic burst characteristics are investigated: their pair production and their concentration toward the heliographic latitudes of + and 12, + and - 34, + and - 56, and - 79 deg. The analysis of the data suggests that the bursts have a heliospheric origin. The presence in the heliosphere of a current sheet on one of the heliolatitudes of burst concentration suggests that the latitudinal zonality in the distribution of bursts reflects the structure of the heliomagnetosphere and the large-scale solar magnetic field. In addition, it is suggested that the number of bursts depends on the phase of solar activity.

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