Computer Science
Scientific paper
Oct 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ge%26ae..22..711p&link_type=abstract
Geomagnetizm i Aeronomiia, vol. 22, Sept.-Oct. 1982, p. 711-715. In Russian.
Computer Science
Atmospheric Attenuation, Cosmic Rays, Galactic Radiation, Magnetic Moments, Radiation Absorption, Solar Activity Effects, Earth Atmosphere, Magnetic Effects, Primary Cosmic Rays, Solar Magnetic Field, Solar Terrestrial Interactions
Scientific paper
The paper examines data on the mean free path to absorption of the total ionizing component of cosmic rays in the atmosphere formed by primary particles with rigidities in the range 0.5-2.35 GV during the period 1961-1980. It is shown that this mean free path decreased by approximately 20% during 1972-1979 in comparison with 1961-1968. A decrease in the mean free path after the inversion of the solar magnetic field of 1968-1972 may be explained by an increase of the fraction of nuclei in the primary cosmic rays.
Pereiaslova N. K.
Pokrevskii P. E.
Stozhkov Iu. I.
No associations
LandOfFree
Absorption of fluxes of galactic cosmic rays in the atmosphere during 1961-1980 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 Absorption of fluxes of galactic cosmic rays in the atmosphere during 1961-1980, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Absorption of fluxes of galactic cosmic rays in the atmosphere during 1961-1980 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1030036