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Modelling of Plasma Structures in the Solar Atmosphere

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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

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