Geomagnetic effects in the dark hemisphere associated with solar flares

dc.contributor.author	Sastri, J. H
dc.contributor.author	Murthy, B. S
dc.date.accessioned	2009-06-12T10:35:55Z
dc.date.available	2009-06-12T10:35:55Z
dc.date.issued	1975-01
dc.identifier.citation	Journal of Geomagnetism and Geoelectricity, Vol. 27, No. 1, pp. 67 - 73	en
dc.identifier.issn	0022-1392
dc.identifier.uri	http://hdl.handle.net/2248/4534
dc.description.abstract	Observational data are presented which show that geomagnetic effects occur in the dark hemisphere in association with solar flares. The characteristics of these events (referred to as NTSFEs) are found to be significantly different from those of solar flare effects (SFE) observed at the same station. NTSFEs are characterized by slower rise and slower decay compared to SFE events. Study of the characteristics of NTSFE events in relation to those of the associated solar X-ray flare events showed that the amplitude of the NTSFE is independent of the peak solar X-ray flux level in the two bands 1-8 A and 8-20 A.	en
dc.language.iso	en	en
dc.publisher	Japan Science and Technology Agency	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1975JGG....27...67S	en
dc.subject	Geomagnetism	en
dc.subject	Ionospheric Currents	en
dc.subject	Magnetic Variations	en
dc.subject	Solar Activity Effects	en
dc.subject	Solar Flares	en
dc.subject	Magnetic Induction	en
dc.subject	Solar X-Rays	en
dc.subject	Sunlight	en
dc.title	Geomagnetic effects in the dark hemisphere associated with solar flares	en
dc.type	Article	en