Energetic /keV/ ions of ionospheric origin in the magnetosphere /A review/

Details Energetic /keV/ ions of ionospheric origin in the magnetosphere /A review/ Energetic /keV/ ions of ionospheric origin in the magnetosphere /A review/

Sep 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978ang....34..187p&link_type=abstract

Annales de Geophysique, vol. 34, July-Sept. 1978, p. 187-213.

Physics

Earth Ionosphere, Earth Magnetosphere, Energetic Particles, High Temperature Plasmas, Ionic Mobility, Atmospheric Composition, Energy Spectra, Ion Beams, Magnetic Storms, Oxygen Ions, Particle Acceleration, Polar Regions, Proton Precipitation, Ring Currents, Solar Wind

Scientific paper

Observations of precipitating ions during magnetic storms, upwardly accelerated ion beams at low and at high latitudes, and ring current composition are used to detail the current knowledge of magnetospheric ions which are of ionospheric origin (primarily O(plus) and H(plus), and to a smaller extent, He(plus) and O(plus plus)). These observations are correlated with theoretical acceleration and/or circulation mechanisms, such as ion-cyclotron wave-particle interactions, parallel electric fields, and adiabatic convection.

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