Variations of ion composition and electron density accompanying solar flares

Details Variations of ion composition and electron density accompanying solar flares Variations of ion composition and electron density accompanying solar flares

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980artsa..15...29d&link_type=abstract

Artificial Satellites, vol. 15, Jan. 1980, p. 29-51.

Computer Science

Atmospheric Ionization, Ion Production Rates, Ionospheric Composition, Ionospheric Electron Density, Ionospheric Ion Density, Solar Flares, Atmospheric Chemistry, Ionic Reactions, Photoionization, Solar X-Rays, Tables (Data), Ubv Spectra

Scientific paper

A sudden increase in solar ionizing radiation intensity and changes in the spectral structure of XUV radiation, accompanying a solar flare, produce substantial changes in ionospheric photochemical processes. In the present paper, an attempt is made to determine the changes in ion composition from an analysis of aeronomic processes, using Donnelly's (1976) ionospheric model of flare radiation. Under the assumption of quasi-stationarity, the ion and electron densities at heights between 70 and 300 km are calculated for several typical flare durations.

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