Modelling of Plasma Structures in the Solar Atmosphere

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DC Field	Value	Language
dc.contributor.author	Krishan, V	-
dc.date.accessioned	2005-05-14T07:23:22Z	-
dc.date.available	2005-05-14T07:23:22Z	-
dc.date.issued	1984	-
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 4, pp. 43-46	en
dc.identifier.issn	0374-3632	-
dc.identifier.uri	http://hdl.handle.net/2248/394	-
dc.description.abstract	A maximal helicity principle is proposed to study the stability of plasma structures in the solar atmosphere. This principle derives from the statistical treatment of the magnetohydrodynamical turbulence. The steady state of the plasma system results from subjecting the system to the invariance of total energy, the magnetic helicity and toroidal and poloidal magnetic fluxes. The statistical distributions of the velocity and magnetic fields are formulated.	en
dc.format.extent	123212 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Plasma Structures-Velocity	en
dc.subject	Magnetic Fields	en
dc.subject	Solar Atmosphere	en
dc.title	Modelling of Plasma Structures in the Solar Atmosphere	en
dc.type	Article	en
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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