Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981jkas...14...79l&link_type=abstract
Journal of the Korean Astronomical Society, vol. 14, no. 2, p. 79-87
Astronomy and Astrophysics
Astronomy
1
Scientific paper
Theoretical profiles of selected rotational lines of C_2, CH, TiO and MgH are computed by using the current models of sunspot umbrae and penumbrae. It is found that the lines of the diatomic carbides are enhanced in penumbrae relative to umbrae, while MgH lined are more strongly enhanced in umbrae and the quiet photosphere. The results are discussed with respect to selecting lines suitable for studying the structure of sunspots.
Lee Michael H.
Lee Yong Bok
Yun Hong Sik
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