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On the detectibility of HeH⁺ in the solar photospheric spectrum

Show simple item record Sinha, K. 2010-01-08T05:39:14Z 2010-01-08T05:39:14Z 1994
dc.identifier.citation This article downloded from ADS Free Online Journal en_US
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 cm⁻¹ was scanned for the suggested lines in the present preliminary investigation. It is tentatively concluded that (i) it seems rather difficult to detect the HeH⁺ lines and (ii) observations from above the terrestrial atmosphere may be required for firm conclusion. en_US
dc.language.iso en_US en_US
dc.relation.ispartofseries basi22-143
dc.subject Photospheric spectrum, Photospheric atlas, Ionic molecules en_US
dc.title On the detectibility of HeH⁺ in the solar photospheric spectrum en_US
dc.type Article en_US

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