Observation of solar neutrons by high-altitude neutron monitors

Details Observation of solar neutrons by high-altitude neutron monitors Observation of solar neutrons by high-altitude neutron monitors

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ge%26ae..27..375b&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 27, May-June 1987, p. 375-382. In Russian.

Physics

3

Flux Quantization, Radiation Measurement, Solar Neutrons, Gamma Rays, Radiation Measuring Instruments, Relativistic Particles, Solar Flares, Time Response

Scientific paper

Five-minute data from Alma-Ata and Lomnitski Shtit neutron monitors were used to search for cosmic-ray variations corresponding in time with the most intense phenomena in solar flares. A statistical analysis shows that the distribution of count-rate variations of high-altitude neutron monitors during a gamma-flare differs significantly from the distribution of variations in the preceding and subsequent periods. Observed count-rate increases are found to be due to solar-flare neutrons with energies greater than 300 MeV.

Affiliated with

Also associated with

No associations

Rating

Observation of solar neutrons by high-altitude neutron monitors does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Observation of solar neutrons by high-altitude neutron monitors, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observation of solar neutrons by high-altitude neutron monitors will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1817436