Acceleration of cosmic rays by the stellar wind

Details Acceleration of cosmic rays by the stellar wind Acceleration of cosmic rays by the stellar wind

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984izyak..48.2066p&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Yakutsk, USSR, July 1984) Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheskai

Physics

Cosmic Rays, Particle Acceleration, Plasma-Particle Interactions, Stellar Winds, Electromagnetic Acceleration, Electromagnetic Wave Transmission, Heliosphere, Plasma-Electromagnetic Interaction, Proton Energy, Shock Waves, Solar Terrestrial Interactions, Standing Waves

Scientific paper

The method of generations is used to obtain a numerical solution to the
problem of the propagation and acceleration of cosmic rays in the
stellar wind, limited by a standing shock wave. In application to the
heliosphere, a calculation is made of the intensity of accelerated
protons near earth orbit in the 0.1-20 MeV energy range.

Affiliated with

Also associated with

No associations

Rating

Acceleration of cosmic rays by the stellar wind 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 Acceleration of cosmic rays by the stellar wind, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Acceleration of cosmic rays by the stellar wind will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1754456