Electron flux with electron energies above 40 MeV at altitudes of about 500 km in region where capture is possible and outside it when L is 3 or greater

Details Electron flux with electron energies above 40 MeV at altitudes of about 500 km in region where capture is possible and outside it when L is 3 or greater Electron flux with electron energies above 40 MeV at altitudes of about 500 km in region where capture is possible and outside it when L is 3 or greater

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985rpspr.......35k&link_type=abstract

In its USSR Rept.: Space (JPRS-USP-85-003) p 35 (SEE N85-25284 15-12) Transl. into ENGLISH from Kosmicheskiye Issled. (USSR),

Computer Science

Cosmic Rays, Electron Capture, Electron Flux Density, High Energy Electrons, Outer Radiation Belt, Cosmos 225 Satellite, Mirror Point, Particle Telescopes

Scientific paper

The electron flux for energies greater than 40 to 50 MeV at altitudes of 400 to 500 km in the capture region for a geometric shell parameter of L greater than 3, i.e., close to the outer belt boundary is compared with the electron flux outside the capture region when L greater than 3. Data from the Cosmos-225 (1968) were used. This data reduction was done because of the detection of electrons with energies above 40 MeV in the inner radiation belt and a report of an elevated electron flux in the outer belt. The analysis shows that electrons under these conditions have the same flux levels both inside and outside the possible capture regions. The maximum difference in the flux levels in these two regions cannot exceed about 80 m-2 x s-1 x sr-1.

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