The sunspot cycle and solar and lunar daily variations in H

Details The sunspot cycle and solar and lunar daily variations in H The sunspot cycle and solar and lunar daily variations in H

Dec 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972papge..98..146r&link_type=abstract

Pure and Applied Geophysics PAGEOPH, Volume 98, Issue 1, pp.146-152

Physics

Geophysics

4

Scientific paper

Results of sunspot cycle influence on solar and lunar ranges at a low latitude station, Alibag, outside the equatorial electrojet belt, show that the sunspot cycle association in solar ranges is three times that of the lunar ranges in the d- and j-seasons. This is in general agreement with the earlier results for non-polar latitude stations. The association with sunspot number of individual lunar amplitudes is greatest for lunar semidiurnal harmonic in the j-season. During this season, the sunspot cycle influence on lunar variations is more than that on solar variations, thereby indicating that the lunar current is situated at a level more favourable for sunspot cycle influence than the level of the current associated with solar variations. With the increase in solar activity a shift appears in the times of maxima of semidiurnal lunar variation towards a later lunar hour in e- and j-seasons and in the year.

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