Chromospheric inhomogeneities: origins and dynamics

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DC Field	Value	Language
dc.contributor.author	Venkatakrishnan, P	-
dc.date.accessioned	2009-10-16T11:19:25Z	-
dc.date.available	2009-10-16T11:19:25Z	-
dc.date.issued	1985-10-05	-
dc.identifier.citation	Current Science, Vol. 54, No. 19, pp. 959 - 963	en
dc.identifier.issn	0011-3891	-
dc.identifier.uri	http://hdl.handle.net/2248/4869	-
dc.description.abstract	Observations of the solar chromosphere in selected spectral lines reveal a large number of inhomogeneities. These inhomogeneities owe their origin to local a large enhancement of the Photospheric magnetic fields. The detection of chromospheric inhomogeneities in other sun-like stars can be considered as the evidence for magnetic structures in such stars. This article gives a brief description of solar chromospheric structures as well as the evidence for similar inhomogeneities in stellar chromospheres.	en
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences	en
dc.relation.uri	http://www.ias.ac.in/j_archive/currsci/54/vol54contents.html	en
dc.rights	© Indian Academy of Sciences	en
dc.subject	Chromospheric	en
dc.subject	In-homogeneities	en
dc.subject	Dynamics	en
dc.title	Chromospheric inhomogeneities: origins and dynamics	en
dc.type	Article	en
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