Large-scale flow patterns in the solar atmosphere

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3522

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DC Field	Value	Language
dc.contributor.author	Sivaraman, K. R	-
dc.date.accessioned	2008-09-10T12:08:06Z	-
dc.date.available	2008-09-10T12:08:06Z	-
dc.date.issued	1990	-
dc.identifier.citation	IAU Symposium, No. 142, pp. 101 - 105	en
dc.identifier.issn	0074-1809	-
dc.identifier.uri	http://hdl.handle.net/2248/3522	-
dc.description.abstract	One of the results of a study on the migration of H-alpha filaments, namely, the existence of meridional flow on the sun, is presented and extended to show the participation of this meridional flow in the solar cycle variation. The filament bands start their poleward migration with small speeds ranging from 5 to 20 m/s synchronously with the rising phase of the solar cycle. It is inferred from migration diagrams that during the years of the solar minimum, the filament bands do not show signs of a continuous migration toward the poles.	en
dc.language.iso	en	en
dc.publisher	International Astronomical Union	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1990IAUS..142..101S	en
dc.subject	Flow distribution	en
dc.subject	H Alpha line	en
dc.subject	Solar atmosphere	en
dc.subject	Solar cycles	en
dc.subject	Solar flares	en
dc.subject	Spectroheliographs	en
dc.subject	Flow velocity	en
dc.subject	Magnetic measurement	en
dc.subject	Solar magnetic field	en
dc.title	Large-scale flow patterns in the solar atmosphere	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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