Precipitation of energetic protons at high latitudes: dependence on the interplanetary magnetic field.

Details Precipitation of energetic protons at high latitudes: dependence on the interplanetary magnetic field. Precipitation of energetic protons at high latitudes: dependence on the interplanetary magnetic field.

Aug 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999kosis..37..339d&link_type=abstract

Kosmicheskie Issledovaniia, Tom 37, No. 4, p. 339 - 347

Physics

Aurorae: Interplanetary Magnetic Field

Scientific paper

The data of particle measurements onboard the low-orbit NOAA satellites are used to investigate the occurrence of energetic (>30 keV) proton precipitation at latitudes above 80° and the dynamics of the poleward boundary of the precipitation as a function of the interplanetary magnetic field (IMF). Similar dependencies have been established earlier at the same latitudes for polar-cap aurorae.

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