Interferometric Eclipse Observations of Coronal Fe XIV Emission

dc.contributor.author	Smartt, R. N
dc.contributor.author	Zirker, J. B
dc.contributor.author	Mauter, H. A
dc.date.accessioned	2005-02-03T03:54:13Z
dc.date.available	2005-02-03T03:54:13Z
dc.date.issued	1980-06
dc.identifier.citation	BASI, Vol. 8, Nos. 2&3, pp. 59-61	en
dc.identifier.uri	http://hdl.handle.net/2248/284
dc.description.abstract	An experiment carried out during the February 16, 1980 total solar eclipse to measure velocities and intensity distributions associated with coronal loops is described. The optical instrumentation used consisted of a 30-cm aperture Cassegrain telescope, a solid fabry-Perot etalon, ancillary optical components and a motor-driven camera. During totality, the green corona was photographed both with and without the etalon in thte system; the first maximum of the etalon beyond the limb was recorded on three frames. A preliminary discussion of the data is presented.	en
dc.format.extent	1357711 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Tata Institute of Fundamental Research, Bombay	en
dc.subject	Coronal Emission	en
dc.subject	Interferometric Eclipse Observations	en
dc.subject	Coronal Fe XIV Emission	en
dc.title	Interferometric Eclipse Observations of Coronal Fe XIV Emission	en
dc.type	Article	en