Coronal heating and chromospheric energy density: An observational association

dc.contributor.author	Venkatakrishnan, P
dc.date.accessioned	2008-07-09T08:09:51Z
dc.date.available	2008-07-09T08:09:51Z
dc.date.issued	1993-12
dc.identifier.citation	Solar physics , Vol. 148, No. 2, pp. 233 - 238	en
dc.identifier.uri	http://hdl.handle.net/2248/2593
dc.description.abstract	The time-averaged equivalent width of the He 1 10830 Angstrom line is seen to be correlated with the time-averaged line width. This correlation is interpreted as evidence for the association of the chromospheric energy density with the heating of overlying corona	en
dc.format.extent	632711 bytes
dc.format.mimetype	application/pdf
dc.language.iso		en
dc.publisher	Springer	en
dc.relation.uri	http://www.springerlink.com/content/t54171037r3p4566/	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1993SoPh..148..233V	en
dc.subject	Chromosphere	en
dc.subject	Corona	en
dc.title	Coronal heating and chromospheric energy density: An observational association	en
dc.type	Article	en