Structure and dynamics of auroral protons and electrons with energies of tens and hundreds of keV studied on the basis of measurements on the Cosmos-900 satellite

Details Structure and dynamics of auroral protons and electrons with energies of tens and hundreds of keV studied on the basis of measurements on the Cosmos-900 satellite Structure and dynamics of auroral protons and electrons with energies of tens and hundreds of keV studied on the basis of measurements on the Cosmos-900 satellite

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981kosis..19...71k&link_type=abstract

Kosmicheskie Issledovaniia, vol. 19, Jan.-Feb. 1981, p. 71-75. In Russian.

Physics

Auroral Zones, Cosmos Satellites, Electron Flux Density, Magnetic Storms, Proton Flux Density, Electron Energy, Electron Precipitation, Energy Distribution, Proton Energy, Proton Precipitation

Scientific paper

The paper analyzes Cosmos-900 data on the distribution of protons with energies of 50-506 keV and electrons with energies of 50-210 keV in the auroral zone during the magnetic storm of December 11 to 12, 1977. Latitude profiles of proton and electron fluxes had a nonstationary multimaximum structure. Latitude distributions of protons in evening and postmidnight sectors had a two-maximum structure with a harder particle spectrum in the low-latitude region. Attention is given to the dynamics of the low-latitude and high-latitude boundaries of proton and electron precipitation in relation to magnetic conditions and local time.

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