Physics
Scientific paper
Mar 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984kosis..22..213v&link_type=abstract
Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 22, Mar.-Apr. 1984, p. 213-224. In Russian.
Physics
Energy Spectra, Equatorial Atmosphere, Ion Temperature, Radiation Belts, Solar Terrestrial Interactions, Helium Ions, Hydrogen Ions, Oxygen Ions, Solar Corona, Spectral Energy Distribution
Scientific paper
An analysis is made of differential energy spectra of H, He, C, and O ions with energies exceeding 1 MeV in the radiation belts at the geomagnetic equator in a magnetically quiet period. It is shown that at L of at least 4 the rigidity of the spectrum is a function of the ion charge state. The form of the ion spectrum is found to reflect charge states characteristic for coronal temperatures of 1-million to 2-million K. This finding is used to explain the existence of dominant streams of heavy ions in the radiation belts.
Panasiuk M. I.
Vlasova N. A.
No associations
LandOfFree
Equatorial energy distributions of ions of the earth's radiation belts as a function of the solar-corona temperature 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 Equatorial energy distributions of ions of the earth's radiation belts as a function of the solar-corona temperature, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Equatorial energy distributions of ions of the earth's radiation belts as a function of the solar-corona temperature will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1041707