Fabry-Perot interferometric observations of the coronal red and green lines during the 1983 Indonesian eclipse

dc.contributor.author	Chandrasekhar, T
dc.contributor.author	Ashok, N. M
dc.contributor.author	Desai, J. N
dc.contributor.author	Pasachoff, J. M
dc.contributor.author	Sivaraman, K. R
dc.date.accessioned	2009-01-16T14:15:41Z
dc.date.available	2009-01-16T14:15:41Z
dc.date.issued	1984-02
dc.identifier.citation	Applied Optics , Vol. 23, pp. 508 - 511	en
dc.identifier.issn	0003-6935
dc.identifier.uri	http://hdl.handle.net/2248/4265
dc.description	Restricted Access
dc.description.abstract	A dual-channel Fabry-Perot interferometric system was used to study simultaneously the coronal emission lines at 5303 Å (Fe XIV) and at 6374 Å (Fe X). Initial results indicate an emission corona confined largely within 1.2 R_sun;. Doppler temperatures derived from the width of the 5303-Å line appear to be appreciably lower than similar temperatures determined during the solar-maximum eclipse of 1980.	en
dc.language.iso	en	en
dc.publisher	Optical society of America	en
dc.relation.uri	http://www.opticsinfobase.org/abstract.cfm?id=27279	en
dc.rights	© Optical Society of America	en
dc.subject	Fabry-Perot Interferometers	en
dc.subject	Solar Corona	en
dc.subject	Solar Eclipses	en
dc.subject	Solar Instruments	en
dc.subject	Solar Spectra	en
dc.subject	Collimation	en
dc.subject	Emission Spectra	en
dc.subject	Image Filters	en
dc.title	Fabry-Perot interferometric observations of the coronal red and green lines during the 1983 Indonesian eclipse	en
dc.type	Article	en