Characteristics of the interplanetary medium and anisotropy of solar cosmic rays

Details Characteristics of the interplanetary medium and anisotropy of solar cosmic rays Characteristics of the interplanetary medium and anisotropy of solar cosmic rays

Aug 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ge%26ae..16..577v&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 16, July-Aug. 1976, p. 577-586. In Russian.

Physics

1

Interplanetary Medium, Solar Cosmic Rays, Solar Flares, Solar Wind, Anisotropy, Solar Electrons, Solar Protons

Scientific paper

Mars 4, 5, and 7 probes observed a solar cosmic ray event in September 1973 involving a flare-associated increase in cosmic ray intensity with prolonged negative anisotropy. A model for solar cosmic ray propagation in the interplanetary medium is developed which suggests that the rays are screened by regions in the solar equatorial plane and reflected at distances about 2 AU from the sun.

Affiliated with

Also associated with

No associations

Rating

Characteristics of the interplanetary medium and anisotropy of solar cosmic rays 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 Characteristics of the interplanetary medium and anisotropy of solar cosmic rays, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Characteristics of the interplanetary medium and anisotropy of solar cosmic rays will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1872775