Energy changes of protons during their motion to the sun

Details Energy changes of protons during their motion to the sun Energy changes of protons during their motion to the sun

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ge%26ae..20..785g&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 20, Sept.-Oct. 1980, p. 785-789. In Russian.

Physics

Injection, Magnetic Effects, Particle Acceleration, Proton Energy, Solar Magnetic Field, Energy Spectra, Monte Carlo Method

Scientific paper

The Monte Carlo method is used to examine the behavior of protons injected toward the sun from within a distance of 1 AU from the sun. The effect of the radial magnetic field of the sun on the particles is considered. It is shown that most of the 1-MeV protons return to the place of injection (after wandering in interplanetary space) with an energy that is greater than the energy at injection. The remaining protons (15%) return with an energy less than that at injection.

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