✦ LIBER ✦

On the possibility of faint molecular lines of PO, PH, MgH+, and CN in the solar spectrum

✍ Scribed by K. Sinha; B. M. Tripathi; R. M. Atalla; P. D. Singh

Publisher: Springer
Year: 1988
Tongue: English
Weight: 334 KB
Volume: 115
Category: Article
ISSN: 0038-0938
DOI: 10.1007/bf00148724

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✦ Synopsis

Equivalent width calculations for some electronic and vibration-rotation transitions of the molecules PO, PH, MgH +, and CN have been carried out for a few umbral, photospheric, and facular model atmospheres. It appears that a few weak lines of these molecules might show up in the umbral spectrum. Le Blanc bands of CN are too weak for detection in the solar spectrum.

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