The propagation of flare generated shock waves in self-gravitating solar atmosphere

Please use this identifier to cite or link to this item: http://www.repository.rmutt.ac.th/xmlui/handle/123456789/1322

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DC Field	Value	Language
dc.contributor.author	S. N. Ojha, Awaneesh Jee Srivastava
dc.date.accessioned	2014-02-12T04:01:48Z
dc.date.accessioned	2020-09-24T04:46:00Z	-
dc.date.available	2014-02-12T04:01:48Z
dc.date.available	2020-09-24T04:46:00Z	-
dc.date.issued	2014
dc.identifier.uri	http://www.repository.rmutt.ac.th/dspace/handle/123456789/1322	-
dc.description	The 15th International Conference of International Academy of Physical Sciences	en_US
dc.description.abstract	The effects of an interplanetary magnetic field on the propagation of the flare generated shock wave in a non-uniformly distributed solar self-gravitating atmosphere are investigated by using an approximate analytic method of Whitham. The expressions for the velocity of shock wave and for the other flow variables behind weak and strong shocks are derived and discussed.	en_US
dc.language.iso	en	en_US
dc.publisher	Rajamangala University of Technology Thanyaburi. Faculty of Sciences and Technology	en_US
dc.subject	propagation	en_US
dc.subject	flare generated	en_US
dc.subject	shock waves	en_US
dc.subject	self-gravitating	en_US
dc.subject	solar atmosphere	en_US
dc.title	The propagation of flare generated shock waves in self-gravitating solar atmosphere	en_US
dc.type	Other	en_US
Appears in Collections:	ประชุมวิชาการ (Proceedings - SCI)

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