Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/277
Full metadata record
DC Field | Value | Language |
---|---|---|
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 |
Appears in Collections: | BASI Publications |
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