Solar and lunar variations in TEC at low latitudes in India

Details Solar and lunar variations in TEC at low latitudes in India Solar and lunar variations in TEC at low latitudes in India

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985jatp...47..309r&link_type=abstract

Journal of Atmospheric and Terrestrial Physics (ISSN 0021-9169), vol. 47, April 1985, p. 309-317.

Physics

4

Earth-Moon System, F 2 Region, Ionospheric Electron Density, Lunar Tides, Solar Oscillations, Solar Terrestrial Interactions, Tropical Regions, Ats 6, Electrodynamics, India

Scientific paper

Total electron content data at Ootacamund (dip 6 deg N) during the second phase of the ATS-6 program are analyzed for solar and lunar variations. Both the lunar semimonthly and lunar semidiurnal tides at Ootacamund are smaller in magnitude than at stations near the Appleton anomaly crest. The phases of the lunar oscillations however are almost the same as that at tropical latitudes. Thus the lunar tides in total electron content and in maximum F2-region electron density at the equatorial station are not in phase and present problems for the simple electrodynamic theory.

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