On the atmospheric optical and radio emission accompanying cosmic gamma-ray bursts

Details On the atmospheric optical and radio emission accompanying cosmic gamma-ray bursts On the atmospheric optical and radio emission accompanying cosmic gamma-ray bursts

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pazh...11..444v&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 11, June 1985, p. 444-447) Soviet Astronomy Letters (ISSN 0360-0327), vol. 11, May-June

Astronomy and Astrophysics

Astronomy

Earth Atmosphere, Gamma Ray Bursts, Light Emission, Radio Emission, Cerenkov Radiation, Radiation Effects

Scientific paper

The intensity of the atmospheric flashes that would be triggered by bursts of 0.01-10 MeV secondary gamma-ray photons is estimated to be comparable with the nightglow background whose intensity is below 5 x 10 to the -6th erg/cm s. Light flashes of this intensity can be detected with the large solar antenna arrays suggested for measuring the Cerenkov radiation from high-energy cosmic gamma rays. It is noted that due to their common generation mechanism, both optical and radio signals can be usefully incorporated in a program for detecting cosmic gamma-ray bursts.

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