Ionospheric and thermospheric response over Millstone Hill to the May 30, 1984, annular solar eclipse

Details Ionospheric and thermospheric response over Millstone Hill to the May 30, 1984, annular solar eclipse Ionospheric and thermospheric response over Millstone Hill to the May 30, 1984, annular solar eclipse

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986jgr....91.1661r&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 91, Feb. 1, 1986, p. 1661-1670.

Physics

20

Ionospheric Electron Density, Ionospheric Ion Density, Solar Eclipses, Solar Terrestrial Interactions, Thermosphere, Atmospheric Circulation, Atmospheric Models, Atmospheric Temperature, Electron Energy, Ion Temperature, Time Dependence

Scientific paper

A procedure described in an earlier paper (Ridley et al., 1984) is used to calculate the thermospheric response to the May 30, 1984 annular solar eclipse. The time-dependent predictions of neutral temperature, winds, and composition over Millstone Hill are then used in an ionospheric code to calculate the time-dependent ionospheric response expected during the eclipse. These predictions were used to suggest an incoherent radar experiment for the eclipse. The model descriptions, calculational procedures, and predictions are presented.

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