Analysis of data from the Baksan underground scintillation telescope obtained during the solar flare of September 29, 1989

Details Analysis of data from the Baksan underground scintillation telescope obtained during the solar flare of September 29, 1989 Analysis of data from the Baksan underground scintillation telescope obtained during the solar flare of September 29, 1989

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ge%26ae..32..192a&link_type=abstract

Geomagnetizm i Aehronomiya (ISSN 0016-7940), vol. 32, no. 5, p. 192-195.

Astronomy and Astrophysics

Astronomy

1

Muons, Scintillation Counters, Solar Cosmic Rays, Solar Flares, Telescopes, Astronomical Observatories, Neutron Counters

Scientific paper

An increase in the muon count rate was recorded at the Baksan telescope
during the solar flare of September 29, 1989. The increase lagged 1.5 hr
behind the initial count rate increase of the neutron monitor, but
coincided with the count rate maximum. The recorded threshold energy of
the muons was 200 GeV.

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