Dynamics of magnetic and velocity fields in coronal loops

dc.contributor.author	Krishan, V
dc.contributor.author	Berger, M
dc.contributor.author	Priest, E. R
dc.date.accessioned	2009-12-03T11:15:09Z
dc.date.available	2009-12-03T11:15:09Z
dc.date.issued	1988-07
dc.identifier.citation	Altrock, Richard C. ed., Solar and stellar coronal structure and dynamics:A Festschrift in honor of Dr. John W-Evans: Proceedings of the Ninth Sacramento Peak Summer Symposium, Sunspot, NM 17 - 21, August, 1987, pp. 236 - 247	en
dc.identifier.uri	http://hdl.handle.net/2248/4929
dc.description.abstract	The coronal loop plasma is represented by a superposition of the three lowest order Chandrasekhar-Kendall modes. The temporal evolution of the velocity and magnetic field in each of these mode is determined using ideal MHD equations under two simplified cases viz (i) allowing small departures from the equilibrium and (ii) the pump approximation.	en
dc.language.iso	en	en
dc.publisher	National Solar Observatory	en
dc.rights	© National Solar Observatory	en
dc.subject	Dynamics	en
dc.subject	Magnetic and Velocity Fields	en
dc.subject	Coronal Loops	en
dc.subject	Solar Physics	en
dc.subject	Solar Corona	en
dc.title	Dynamics of magnetic and velocity fields in coronal loops	en
dc.type	Article	en