Computer Science
Scientific paper
Sep 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984kosis..22..756p&link_type=abstract
Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 22, Sept.-Oct. 1984, p. 756-762. In Russian.
Computer Science
Geomagnetic Pulsations, Magnetic Equator, Proton Belts, Proton Density (Concentration), Proton Energy, Energy Spectra, Power Spectra, Radial Distribution, Satellite Observation
Scientific paper
Satellite data on the spatial location of intensity peaks of radial profiles (Ljm) of protons in the energy range from 500 keV to 100 MeV near the geomagnetic equator are examined. These data are compared with calculations of Ljm(E), taking into account particle transport under the effect of geomagnetic-field fluctuations (GFF). Calculations and experimental data are shown to agree well for a GFF power spectrum having, along with the principal spectrum component Pm(nu) proportional to nu exp -p (where p is about 2), a dominant spectral component at the frequency nu in the mHz range.
Panasiuk M. I.
Sosnovets Eh. N.
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