K2V/K2R asymmetries in the sun and stars

dc.contributor.author	Sivaraman, K. R
dc.date.accessioned	2008-12-19T14:32:09Z
dc.date.available	2008-12-19T14:32:09Z
dc.date.issued	1982-03
dc.identifier.citation	Astrophysical Journal, Part 1, Vol. 254, pp. 814 - 815	en
dc.identifier.issn	0004-637X
dc.identifier.uri	http://hdl.handle.net/2248/4146
dc.description.abstract	The K2V/K2R asymmetry in the self-reversed emission peaks of the Ca II K line in the sun is the result of the redward displacement of K3. This redward displacement is explained as caused by the dark condensations in K3 and not due to the supergranulation flow pattern. Arguments are presented to show that such asymmetries in the spectra of stars provide evidence for the presence of these structures in their chromospheres	en
dc.language.iso	en	en
dc.publisher	The American Astronomical Society	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1982ApJ...254..814S	en
dc.rights	©The American Astronomical Society	en
dc.subject	Calcium, Chromosphere	en
dc.subject	Emission Spectra	en
dc.subject	K Lines	en
dc.subject	Red Shift	en
dc.subject	Solar Spectra	en
dc.subject	Stellar Spectra	en
dc.subject	Visible Spectrum	en
dc.subject	Asymmetry	en
dc.subject	Optical Emission	en
dc.subject	Spectroscopy	en
dc.title	K2V/K2R asymmetries in the sun and stars	en
dc.type	Article	en