SH on the sun

Sinha, K.; Joshi, G. C.; Pande, M. C.
URI: http://hdl.handle.net/123456789/844
Date: 1976

Abstract:

The theoretical estimates of the abundances and intensities of the fraunhofer lines for various atomic and molecular species facilitate identification and clarify the role of blending produced by the nearby lines in the solar spectrum.

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