✦ LIBER ✦

Possibility of24MgH+in the solar atmosphere-high resolution rotation-vibration spectra

✍ Scribed by P. D. Singh; W. J. Maciel

Publisher: Springer
Year: 1976
Tongue: English
Weight: 531 KB
Volume: 49
Category: Article
ISSN: 0038-0938
DOI: 10.1007/bf00162446

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✦ Synopsis

High resolution rotation-vibration spectra of Av = 1 and 2 sequences of 24MgH + are obtained by a differencing process invoking the known structures of electronic bands observed in the region 214-340nm. A reversal of R branch (band head formation) is noticed in each of the rotation-vibration bands. The J= l--~J= 0 transition is predicted to be at 376098, 365301, 354286 and 342981 MHz for v = 0,1,2 and 3, respectively, in the ground electronic state 12s The equilibrium rotational constants Be, ae and re for the XI~ + state are found 6.4637 cm -1, 0.1899cm -1 and 1.6421 ,~, respectively.

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