Winds, wind-shears and plasma densities during the initial phase of a magnetic storm from equatorial latitudes

Details Winds, wind-shears and plasma densities during the initial phase of a magnetic storm from equatorial latitudes Winds, wind-shears and plasma densities during the initial phase of a magnetic storm from equatorial latitudes

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989jatp...51..169s&link_type=abstract

Journal of Atmospheric and Terrestrial Physics (ISSN 0021-9169), vol. 51, March 1989, p. 169-177. Research supported by the Depa

Computer Science

Sound

3

Equatorial Regions, Magnetic Storms, Plasma Density, Wind Profiles, Wind Shear, Atmospheric Ionization, Electron Density (Concentration), Fabry-Perot Spectrometers, Rocket Sounding, Temperature Distribution

Scientific paper

A sodium vapor release experiment was performed at an equatorial rocket launching station during the initial phase of a magnetic storm. The formation of sharp layers of ionization can be explained by the electrodynamical processes associated with wind shears at a location close to the edge of the equatorial electrojet belt. The significance of the change in the neutral composition due to the enhanced neutral temperature and the low turbopause level is explored.

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