High Resolution Coronal Intensity and Polarization Measurements

dc.contributor.author	Streete, John. L
dc.contributor.author	Lacey, Leon. B
dc.date.accessioned	2005-02-03T06:41:39Z
dc.date.available	2005-02-03T06:41:39Z
dc.date.issued	1980-12
dc.identifier.citation	BASI, Vol. 8, No. 4, pp. 141-143	en
dc.identifier.uri	http://hdl.handle.net/2248/299
dc.description.abstract	The total eclipse of February 16, 1980 was successfully photographed with the High Altitude Observatory's coronal camera from a site in Palem, India. The purpose of the experiment was to obtain, with high spatial resolution, polarization and intensity measurements of the corona to about 3.5 Radius. The exposures are now processed, raster scanned, digitized and stored on magnetic tape, and we are in the process of obtaining the final photometric calibration of the exposures.	en
dc.format.extent	1285917 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Astronomical Society of India	en
dc.subject	Coronal Intensity	en
dc.subject	Polarization Measurements	en
dc.subject	Total Solar Eclipse	en
dc.title	High Resolution Coronal Intensity and Polarization Measurements	en
dc.type	Article	en