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Possibility of 24MgH+ in the solar atmosphere-high resolution rotation-vibration spectra (1976)

Singh, P. D. ; Maciel, W. J.

Springer

Solar physics 49 (1976), S. 217-230

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ISSN: 1573-093X

Source: Springer Online Journal Archives 1860-2000

Topics: Physics

Notes: Abstract High resolution rotation-vibration spectra of Δv = 1 and 2 sequences of 24MgH+ are obtained by a differencing process invoking the known structures of electronic bands observed in the region 214–340 nm. A reversal of R branch (band head formation) is noticed in each of the rotation-vibration bands. The J = 1 → 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 1∑+. The equilibrium rotational constants B e, α e and r e for the X 1•E+ state are found 6.4637cm−1, 0.1899 cm−1 1.6421 Å, respectively.

Type of Medium: Electronic Resource

URL: http://dx.doi.org/10.1007/BF00162446

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