Intensity rises for electrons of energy greater than or equal to 40 keV due to quasisteady solar-wind plasma streams

Details Intensity rises for electrons of energy greater than or equal to 40 keV due to quasisteady solar-wind plasma streams Intensity rises for electrons of energy greater than or equal to 40 keV due to quasisteady solar-wind plasma streams

Mar 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975cosre..12..661z&link_type=associated

(Kosmicheskie Issledovaniia, vol. 12, Sept.-Oct. 1974, p. 725-730.) Cosmic Research, vol. 12, no. 5, Mar. 1975, p. 661-665. Tra

Physics

Electron Flux Density, Magnetohydrodynamic Flow, Shock Wave Propagation, Solar Wind, Electron Energy, Interplanetary Magnetic Fields, Kp Index, Proton Energy, Satellite Observation, Time Dependence

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