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dc.contributor.authorRao, D.R.K.
dc.contributor.authorArora, B.R.
dc.date.accessioned2015-05-22T10:10:38Z
dc.date.accessioned2021-02-12T09:23:01Z-
dc.date.available2015-05-22T10:10:38Z
dc.date.available2021-02-12T09:23:01Z-
dc.date.issued1975
dc.identifier.citationGerlands Beitraege Geophysik, v.84/2, p.113-116, 1975.en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/132-
dc.description.abstractThe lunar semidiurnal term of the phase law tides in the horizontal intensity at Alibag is found to undergo a systematic decrease in amplitude with increase in magnetic activity. An examination of the results reported earlier for some stations and those of Alibag suggests that there is a general decrease of amplitude with increase in magnetic activity at stations where the lunar time of maximum is around the time of magnetospheric expansion for the lunar tide and an increase in amplitude for stations where the lunar time of maximum is around the time of magnetospheric contraction. In the partial tides, only the phase angle of the second harmonic shows a systematic decrease with increase in magnetic activity.en_US
dc.language.isoenen_US
dc.subjectDiurnal variationsen_US
dc.subjectFlux densityen_US
dc.subjectGeomagnetismen_US
dc.subjectLunar tidesen_US
dc.subjectMagnetic variationsen_US
dc.subjectMagnetospheric Instabilityen_US
dc.subjectHarmonic functionsen_US
dc.subjectLunar effectsen_US
dc.subjectolar activity effectsen_US
dc.subjectSolar wind velocityen_US
dc.titleOn the association of lunar daily variations in H at Alibag with the degree of magnetic activityen_US
dc.typeArticleen_US
dc.identifier.accession090645
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