Atmospheric Tides in the Ionosphere. II. Lunar Tidal Variations in the F Region Near the Magnetic Equator

Details Atmospheric Tides in the Ionosphere. II. Lunar Tidal Variations in the F Region Near the Magnetic Equator Atmospheric Tides in the Ionosphere. II. Lunar Tidal Variations in the F Region Near the Magnetic Equator

Jul 1947

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1947rspsa.190..273m&link_type=abstract

Proceedings of the Royal Society of London. Series A, Mathematical and Physical Sciences, Volume 190, Issue 1021, pp. 273-288

Physics

13

Scientific paper

Three years' data for the heights and critical frequencies of the F1 and F2 regions at Huancayo, Peru, are examined for lunar tides. Semi-diurnal lunar tides are found in all quantities save fF_{1}0. It is found that the lunar variation in the F2 region depends on solar time in both phase and amplitude. At certain solar epochs it attains very large amplitudes, up to 60 km. in hF_{2}max. and 28% in fF_{2}0. The theory of these variations, originated in a previous paper, is further developed.

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