Wave-particle interactions at the magnetopause - Contributions to the dayside aurora

Details Wave-particle interactions at the magnetopause - Contributions to the dayside aurora Wave-particle interactions at the magnetopause - Contributions to the dayside aurora

Feb 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981georl...8..183t&link_type=abstract

Geophysical Research Letters, vol. 8, Feb. 1981, p. 183-186.

Physics

48

Auroras, Magnetopause, Plasma Waves, Plasma-Particle Interactions, Space Plasmas, Wave Interaction, Daytime, Magnetohydrodynamic Stability, Magnetosheath, Particle Energy, Particle Precipitation

Scientific paper

The observations on ISEE 1 and ISEE 2 correlate the presence of intense electromagnetic and electrostatic emissions with enhanced fluxes of 1-6 keV electrons at the earth's magnetopause. The measured proton to electron ratio in the 1-10 keV energy range indicates the presence of substantial fluxes of electrons at energies below 1 keV. The 1.3-1.7 keV proton flux was essentially unchanged as the spacecraft moved from the magnetosheath into the wave-particle layer at and inside the magnetopause. The consequences of the magnetopause wave-particle interactions reported are consistent with the known features of the dayside aurora.

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