The Kitt Peak Coronal Velocity Experiment

dc.contributor.author	Livingston, W
dc.contributor.author	Harvey, J
dc.contributor.author	Doe, L. A
dc.contributor.author	Gillespie, B
dc.contributor.author	Ladd, G
dc.date.accessioned	2005-02-03T02:57:37Z
dc.date.available	2005-02-03T02:57:37Z
dc.date.issued	1980-06
dc.identifier.citation	BASI, Vol. 8, Nos. 2&3, pp. 43-47	en
dc.identifier.uri	http://hdl.handle.net/2248/282
dc.description.abstract	Multi-slit spectra of (Fe XIV 5303) plus neon comparisons were successfully obtained on February 16, 1980 at the Japal-Rangapur site. The objective is to confirm our previous results of March 1970 and June 1973, viz. that the corona is remarkably quiescent (random velocities = 0.5 Km/s r.m.s.) and that the majority of detected flows at 0.3 - 1.0 Ro are directed towards the Sun.	en
dc.format.extent	1161387 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Tata Institute of Fundamental Research, Bombay	en
dc.subject	Coronal Velocity	en
dc.subject	Kitt Peak Coronal Velocity Experiment	en
dc.title	The Kitt Peak Coronal Velocity Experiment	en
dc.type	Article	en