Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/277
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dc.contributor.authorRoy, M-
dc.date.accessioned2005-02-01T05:20:08Z-
dc.date.available2005-02-01T05:20:08Z-
dc.date.issued1980-03-
dc.identifier.citationBASI, Vol. 8, No. 1, pp. 15-20en
dc.identifier.urihttp://hdl.handle.net/2248/277-
dc.description.abstractThe enhanced radiation of the X-rays and the ultra-violets during a chromospheric flare can induce a qualitative change in the ionospheric current system. The observational results of this effect, popularly known as geomagnetic solar flare effect (s.f.e,), are briefly reviewsed. Various theoretical formulations to explain the morphological results are described. The success as well as the shortcomings of the various theories are pointed out.en
dc.format.extent735378 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectIonospheric Currentsen
dc.subjectSolar Flaresen
dc.titleIonospheric Currents Associated with Solar Flares: A Short Reviewen
dc.typeArticleen
Appears in Collections:BASI Publications

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