Ionospheric Currents Associated with Solar Flares: A Short Review

dc.contributor.author	Roy, M
dc.date.accessioned	2005-02-01T05:20:08Z
dc.date.available	2005-02-01T05:20:08Z
dc.date.issued	1980-03
dc.identifier.citation	BASI, Vol. 8, No. 1, pp. 15-20	en
dc.identifier.uri	http://hdl.handle.net/2248/277
dc.description.abstract	The 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.extent	735378 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Astronomical Society of India	en
dc.subject	Ionospheric Currents	en
dc.subject	Solar Flares	en
dc.title	Ionospheric Currents Associated with Solar Flares: A Short Review	en
dc.type	Article	en