Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ap%26ss..36..467s&link_type=abstract
Astrophysics and Space Science, vol. 36, Sept. 1975, p. 467-472.
Astronomy and Astrophysics
Astrophysics
4
Charged Particles, Cosmic Rays, Normal Shock Waves, Particle Acceleration, Supernova Remnants, Abundance, Energy Spectra, Magnetic Fields, Oblique Shock Waves, Particle Energy, Plasma Acceleration, Primary Cosmic Rays, Shock Fronts, Upstream
Scientific paper
The intensive acceleration of energetic charged particles in perpendicular shock waves (which has been known to take place in the interplanetary medium) is utilized to account for the energization of cosmic rays. It is proposed that cosmic rays can be accelerated up to energies between 10 to the 14th and 10 to the 15th power eV in successive perpendicular shock waves that appear inside supernova shells in our galaxy.
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