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Diagnostic Tools for Sunspots: the Molecules C2, Mg H and Ti O

Published online by Cambridge University Press:  03 August 2017

K Sinha*
Affiliation:
U.P. State Observatory, Manora Peak, Naini tal - 263 129, India

Abstract

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The aim of the present communication is to draw attention to the value of simultaneous observations of sunspot umbrae and the quiet Sun in selected molecular lines. It is felt that such observations may lead to an array of sunspot models which account for sunspot sizes, magnetic field strengths, and the solar activity cycle.

Type
Part 5: Magnetic Fields and Infrared Magnetometry
Copyright
Copyright © Kluwer 1994 

References

Lambert, D.L., Mallia, E.A., and Petford, A.D.: 1971, Monthly Notices Roy. Astron. Soc. 154, 265.CrossRefGoogle Scholar
Maltby, P., Avrett, E.H., Carlsson, M., Kjeldseth-Moe, O., Kurucz, R.L., and Loeser, R.: 1986, Astrophys. J. 306, 306, 284.Google Scholar
Minnaert, M.: 1953, in Kuiper, G.P. (ed.) The Sun, University of Chicago Press, Chicago, p. 126.Google Scholar
Sinha, K.: 1984, Bull. Astron. Soc. India 12, 172.Google Scholar
Sinha, K., and Tripathi, B.M.: 1991a, Bull. Astron. Soc. India 19, 13.Google Scholar
Sinha, K. and Tripathi, B.M.: 1991b, Bull. Astron. Soc. India 19, 23.Google Scholar
Sobotka, M.: 1985, Soviet Ast. 29, 576.Google Scholar
Sotirovski, P.: 1971, Astron. Astrophys. 14, 319.Google Scholar
Stankiewicz, A.: 1967, Acta Astr. 17, 341.Google Scholar