On the detectibility of HeH(+) in the solar photospheric spectrum

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1590

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DC Field	Value	Language
dc.contributor.author	Sinha, K	-
dc.date.accessioned	2007-05-17T05:09:17Z	-
dc.date.available	2007-05-17T05:09:17Z	-
dc.date.issued	1994	-
dc.identifier.citation	BASI, Vol. 22, No. 2, pp. 143-147	en
dc.identifier.uri	http://hdl.handle.net/2248/1590	-
dc.description.abstract	In a recent publication of the Bulletin of the Astronomical Society of India, the possibility of detection of the (1-0) vibration-rotation lines of HeH(+) molecules in the solar photospheric spectrum has been suggested. Taking cue, the Photometric Atlas of the solar Spectrum from 1850 to 10,000 1 cm was scanned for the suggested lines in the present preliminary ivestigation. It is tentatively concluded that (1) it seems rather difficult to detect the HeH(+) lines and (2) observations from above the terrestrial atmosphere may be required for firm conclusions	en
dc.format.extent	325702 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Photospheric spectrum	en
dc.subject	Photospheric atlas	en
dc.title	On the detectibility of HeH(+) in the solar photospheric spectrum	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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