HiRES - A high-resolution stigmatic extreme ultraviolet spectroheliometer for studies of the fine-scale structure of the solar chromosphere, transition region, and corona

Timothy, J. G; Berger, T. E; Morgan, J. S; Walker, A. B. C; Jain, S. K; Saxena, A. K; Bhattacharyya, J. C; Huber, M. C. E; Tondello, G; Naletto, G

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3058

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DC Field	Value	Language
dc.contributor.author	Timothy, J. G	-
dc.contributor.author	Berger, T. E	-
dc.contributor.author	Morgan, J. S	-
dc.contributor.author	Walker, A. B. C	-
dc.contributor.author	Jain, S. K	-
dc.contributor.author	Saxena, A. K	-
dc.contributor.author	Bhattacharyya, J. C	-
dc.contributor.author	Huber, M. C. E	-
dc.contributor.author	Tondello, G	-
dc.contributor.author	Naletto, G	-
dc.date.accessioned	2008-08-08T05:59:34Z	-
dc.date.available	2008-08-08T05:59:34Z	-
dc.date.issued	1991-08	-
dc.identifier.citation	Optical Engineering , Vol. 30, No.8, pp. 1142 - 1149	en
dc.identifier.issn	0091-3286	-
dc.identifier.uri	http://hdl.handle.net/2248/3058	-
dc.description	Restricted Access	-
dc.description.abstract	HiRES is a high-resolution stigmatic EUV spectroheliometer whose 45-cm Gregory telescope is coupled to a spectrometer employing a single toroidal diffraction grating and an imaging pulse-counting multianode microchannel array detector system. This spectroheliometer will be used in conjunction with plasma-diagnostic techniques to study the temperature, density, and velocity structures of specific features in the outer solar atmosphere.	en
dc.format.extent	3894 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	SPIE	en
dc.subject	Chromosphere	en
dc.subject	Extreme ultraviolet radiation	en
dc.subject	Rocket-borne instruments	en
dc.subject	Solar corona	en
dc.subject	Spectroheliographs	en
dc.subject	Ultraviolet spectroscopy	en
dc.subject	Calibrating	en
dc.subject	High resolution	en
dc.title	HiRES - A high-resolution stigmatic extreme ultraviolet spectroheliometer for studies of the fine-scale structure of the solar chromosphere, transition region, and corona	en
dc.type	Article	en
Appears in Collections:	IIAP Publications J.C.Bhattacharyya (1982 - 1990)

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