Modelling sunspot equilibrium through a solution of the time dependent MHD equations

dc.contributor.author	Gangadhara, R. T
dc.contributor.author	Hasan, S. S
dc.date.accessioned	2007-09-21T12:10:32Z
dc.date.available	2007-09-21T12:10:32Z
dc.date.issued	1996
dc.identifier.citation	BASI, Vol.24 No. 2 pp. 341-344	en
dc.identifier.uri	http://hdl.handle.net/2248/1819
dc.description.abstract	We numerically simulate the dynamical relaxation to equilibrium of a sunspot. Treating the sunspot as a thick axisymmetric flux tube in cylindrical geometry, we solve the time dependent MHD equation to examine the evolution of a sunspot towards equilibrium, starting from an arbitrary initial state.	en
dc.format.extent	305141 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/1996BASI...24..341G	en
dc.subject	Magnetohydrodynamics-Sun	en
dc.subject	Magnetic fields-Sun	en
dc.subject	Sunspots	en
dc.title	Modelling sunspot equilibrium through a solution of the time dependent MHD equations	en
dc.type	Article	en