Electron density changes during solar eclipse of 16 Feb. 1980 at Gauhati

Details Electron density changes during solar eclipse of 16 Feb. 1980 at Gauhati Electron density changes during solar eclipse of 16 Feb. 1980 at Gauhati

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ijrsp..11...96b&link_type=abstract

Indian Journal of Radio and Space Physics, vol. 11, June 1982, p. 96-99. Research supported by the University Grants Commission

Physics

Space Physics

1

Electron Density Profiles, Ionospheric Electron Density, Solar Eclipses, Ionograms, Photoionization

Scientific paper

True height electron density profiles are deduced from the ionograms taken at Gauhati (lat., 26 deg 10 min N; long. 91 deg 45 mine) on 16 Feb. 1980, a solar eclipse day. Constant electron density contours show a definite eclipse effect. A large increase in the height of the constant electron density levels, more pronounced at lower levels, is seen after first contact. The 'eclipse lag' is about 15 min at around 300 km. A long period wavelike oscillation observed at all electron density levels after the time of maximum obscuration could be eclipse generated.

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