The geomagnetic solar flare effect of 6 July 1968 and its implications

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4688

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DC Field	Value	Language
dc.contributor.author	Sastri, J. H	-
dc.date.accessioned	2009-07-30T10:09:48Z	-
dc.date.available	2009-07-30T10:09:48Z	-
dc.date.issued	1975-12	-
dc.identifier.citation	Annales de Geophysique, vol. 31, pp. 481 - 485	en
dc.identifier.issn	0003-4029	-
dc.identifier.uri	http://hdl.handle.net/2248/4688	-
dc.description.abstract	A study of the geomagnetic solar flare effect (SFE) of July 6, 1968, observed at five Indian magnetic observatories, lying in the longitude range 72-80 E, revealed that this SFE is characterized by a decrease in the H-component at electrojet stations and an increase in the H-component at stations outside the electrojet. Examination of relevant ionogram and magnetogram data recorded at Kodaikanal, a station under the electrojet, indicated the existence of a counter-electrojet just prior to and after the occurrence of SFE.	en
dc.language.iso	en	en
dc.publisher	European Geophysical Society	en
dc.relation.uri	http://adsabs.harvard.edu//abs/1975AnG....31..481S	en
dc.subject	Equatorial Electrojet	en
dc.subject	Geomagnetism	en
dc.subject	Magnetic Signatures	en
dc.subject	Solar Activity Effects	en
dc.subject	Solar Flares	en
dc.subject	Ionograms	en
dc.subject	Magnetic Measurement	en
dc.title	The geomagnetic solar flare effect of 6 July 1968 and its implications	en
dc.type	Article	en
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