Effects of interplanetary transient disturbances on cosmic ray intensity in relation with solar wind plasma parameters

dc.contributor.author	Kaushik, S. C
dc.contributor.author	Shrivastava, P. K
dc.date.accessioned	2007-10-17T10:22:20Z
dc.date.available	2007-10-17T10:22:20Z
dc.date.issued	1999
dc.identifier.citation	BASI, Vol. 27, No. 1, pp. 85 - 90	en
dc.identifier.uri	http://hdl.handle.net/2248/1894
dc.description.abstract	Two types of interplanetary disturbances namely magnetic cloud events (MCE's) and bidirectional events (BDE's) are taken to study the short term change in solar wind plasma components as well as in cosmic ray intensity. These two types of disturbances are again separated into two categories : (i) coronal hole associated events (MCE's & BDE's), and (ii) without coronal hole associated events (MCE's & BDE's). Analysis of this research work indicates distinctly different effects on solar wind plasma velocity and cosmic ray intensity. Coronal holes associated BDE's are found significantly responsible for enhanced plasma velocity. Both disturances in either of the category produce short-term decrease in cosmic ray intensity.	en
dc.format.extent	419080 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1999BASI...27...85K	en
dc.subject	Interplanetary disturbance	en
dc.subject	Cosmic ray	en
dc.subject	Solar wind parameters	en
dc.title	Effects of interplanetary transient disturbances on cosmic ray intensity in relation with solar wind plasma parameters	en
dc.type	Article	en