Ion Spectral Gaps as a Method for Checking the Existence of Quiet-Time Stationary Large-Scale Convection, Its Models, and Particle Source Localization in the Inner Magnetosphere: ION Spectrometer Observations on the Interball-2 Satellite

Details Ion Spectral Gaps as a Method for Checking the Existence of Quiet-Time Stationary Large-Scale Convection, Its Models, and Particle Source Localization in the Inner Magnetosphere: ION Spectrometer Observations on the Interball-2 Satellite Ion Spectral Gaps as a Method for Checking the Existence of Quiet-Time Stationary Large-Scale Convection, Its Models, and Particle Source Localization in the Inner Magnetosphere: ION Spectrometer Observations on the Interball-2 Satellite

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000cosre..38..491b&link_type=openurl

Cosmic Research, Vol. 38, No. 5, p.491

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