On the existence of days with extraordinary geomagnetic lunar tide

Physics

Scientific paper

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Scientific paper

The lunar daily variation, L, in the geomagnetic horizontal field, H, at Huancayo on 2517 quiet days with disturbance character figure Cp [less-than-or-equals, slant] 0.5 has been analysed. On 487 individual days L has been separated from the diurnal variation. Classes of L are defined objectively and quantitatively and the definitions are applied to the study of the characteristics of L on the 487 days. It is found that the magnification of L tends to vary from hour to hour on the same day. The existence of Big L days near the December solstice has been confirmed and they are also found to occur near the Equinoxes. Days have been found on which the phase of L is completely reversed. Some of these days are shown on which the inversion of L conspicuously modifies the diurnal variations. These Inverse L days exist near the December solstice as well as near the Equinoxes and they are more numerous than Big L days. It is suggested that the extraordinary L effects are caused by modifications in the oscillations of the upper atmosphere.

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