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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4922
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dc.contributor.authorVats, H. O-
dc.contributor.authorChandra, H-
dc.contributor.authorDeshpande, M. R-
dc.contributor.authorRastogi, R. G-
dc.contributor.authorMurthy, B. S-
dc.contributor.authorJanve, A. V-
dc.contributor.authorRai, R. K-
dc.contributor.authorSingh, M-
dc.contributor.authorGurm, H. S-
dc.contributor.authorJain, A. R-
dc.date.accessioned2009-12-01T16:32:29Z-
dc.date.available2009-12-01T16:32:29Z-
dc.date.issued1978-03-
dc.identifier.citationNature, Vol. 272, No. 5651, pp. 345 - 346en
dc.identifier.issn0028-0836-
dc.identifier.urihttp://hdl.handle.net/2248/4922-
dc.descriptionRestricted Access-
dc.description.abstractGEOSTATIONARY satellites are able to monitor amplitude, phase, plane of polarisation (Faraday rotation) and group retardation of radio waves passing through the ionosphere with improved temporal resolution, although some of these parameters were earlier measured using orbiting satellites. An extensive experiment has been conducted on Faraday rotation measurements at a chain of stations covering a latitude region from the magnetic equator to 45°N dip (30°N geog.) in the Indian sub-continent using 140 MHz radio beacons received from ATS-6 satellite1. We report here the first evidence of an irregularity belt and its movement during a magnetic storm.en
dc.language.isoenen
dc.publisherNature Publishing Groupen
dc.relation.urihttp://www.nature.com/nature/journal/v272/n5651/abs/272345a0.htmlen
dc.rights© Nature Publishing Groupen
dc.subjectFaraday Effecten
dc.subjectIrregularitiesen
dc.subjectMagnetic Equatoren
dc.subjectMagnetic Stormsen
dc.subjectATS 6en
dc.subjectRadio Beaconsen
dc.subjectTraveling Ionospheric Disturbancesen
dc.titleEquatorial irregularity belt and its movement during a magnetic stormen
dc.typeArticleen
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