Passage through the atmosphere of protons precipitating from the radiation belt

Details Passage through the atmosphere of protons precipitating from the radiation belt Passage through the atmosphere of protons precipitating from the radiation belt

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ge%26ae..26..214i&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 26, Mar.-Apr. 1986, p. 214-217. In Russian.

Physics

Proton Precipitation, Radiation Belts, Stratosphere Radiation, Midlatitude Atmosphere, Northern Hemisphere, Proton Energy, Sea Level, Southern Hemisphere, Vertical Distribution

Scientific paper

Calculations were made of the dependence of the energy of precipitating protons on height above sea level and the dependence of the mean energy of a proton and its dispersion at h = 30 km on longitude for the Northern and Southern Hemispheres at L = 2. Ionization losses and proton-nucleus inelastic interactions were taken into account, and a correction is made for the shift of the proton guiding center from the original field line. Attention is given to the feasibility of using high-altitude balloons to study the midlatitude precipitation of protons at energies above 100 MeV.

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