On the Out of Phase Appearance of Large-Scale Diffuse Magnetic Field of the Sun with Respect to Sunspots

dc.contributor.author	Dikpati, M
dc.contributor.author	Choudhuri, A. R
dc.date.accessioned	2008-07-16T06:36:48Z
dc.date.available	2008-07-16T06:36:48Z
dc.date.issued	1996-03
dc.identifier.citation	Astrophysics and Space Science, Vol. 243, No.1, pp. 169 - 172	en
dc.identifier.issn	0004-640X
dc.identifier.uri	http://hdl.handle.net/2248/2709
dc.description.abstract	We assume the large-scale diffuse magnetic field of the Sun to originate from the poloidal component of a dynamo operating at the base of the convection zone, whereas the sunspots are due to the toroidal component. The evolution of the poloidal component is studied to model the poleward migration of the diffuse field seen on the solar surface and the polar reversal at the time of sunspots maxima (Dikpati and Choudhuri 1994, 1995).	en
dc.format.extent	332466 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Kluwer Academic Publishers	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1996Ap%26SS.243..169D	en
dc.relation.uri	http://www.springerlink.com/content/u78p164358616632/	en
dc.subject	Sunspots	en
dc.subject	Solar magnetic field	en
dc.subject	Poloidal field	en
dc.title	On the Out of Phase Appearance of Large-Scale Diffuse Magnetic Field of the Sun with Respect to Sunspots	en
dc.type	Article	en