Observations of solar-cosmic-ray flares using a solar-longitudinal baseline

Details Observations of solar-cosmic-ray flares using a solar-longitudinal baseline Observations of solar-cosmic-ray flares using a solar-longitudinal baseline

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988izssr..52..818e&link_type=abstract

Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheskaia (ISSN 0367-6765), vol. 52, April 1988, p. 818-820. In Russian.

Astronomy and Astrophysics

Astronomy

Radiation Measurement, Solar Cosmic Rays, Solar Flares, Solar Protons, Flux Quantization, Longitude, Spaceborne Astronomy, Vega Project, Venera Satellites

Scientific paper

The longitudinal distribution of the solar proton flux injected by solar flares was investigated by the Venera 11 and 12 and the Vega 1 and 2 probes. The dependence of the relative flux on the relative solar longitude is evaluated, and the scheme of solar-cosmic-ray motion from a solar flare is depicted. It is shown that, in the case of the rapid arrival of the cosmic rays (collimiated propagation or diffusion), the longitude dependence of the maximum flux in the main direction is described by complex asymmetric curve, whose separate branches and parts can be approximated by an exponential curve.

Affiliated with

Also associated with

No associations

Rating

Observations of solar-cosmic-ray flares using a solar-longitudinal baseline 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 Observations of solar-cosmic-ray flares using a solar-longitudinal baseline, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observations of solar-cosmic-ray flares using a solar-longitudinal baseline will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-849359