On the presence of SH in the sunspot spectrum

Author:

Joshi G. C.,Pande M. C.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference23 articles.

1. Dieke, G. H. and Crosswhite, H. M.: 1962, J. Quant. Spectrosc. Radiat. Transfer 2, 97.

2. Gingerich, O., Noyes, R. W., Kalkofen, W., and Cunny, Y.: 1971, Solar Phys. 18, 347.

3. Glushko, V. P., Gurevich, L. V., Khachkuruzov, G. A., Veits, I. V., and Medvedyev, V. A.: 1962, Termodinamicheskiye Svojstva Individual'nykh Veshchestv, Izd. A.N.S.S.S.R., Moskva, Vol. 2, p. 534.

4. Golden, S. A.: 1967, J. Quant. Spectrosc. Radiat. Transfer 7, 225.

5. Hall, D. N. B.: 1970, Ph.D. Thesis, Harvard Univ. Cambridge, Mass., U.S.A.

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1. The 2020 release of the ExoMol database: Molecular line lists for exoplanet and other hot atmospheres;Journal of Quantitative Spectroscopy and Radiative Transfer;2020-11

2. On SH Molecules in Umbral Spectra;Solar Physics;2015-11

3. Detection of the mercapto radical SH in the solar atmosphere;Astronomy & Astrophysics;2002-05

4. Molecules in the Sun;Publications of the Astronomical Society of Australia;1991

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