Hostname: page-component-78c5997874-m6dg7 Total loading time: 0 Render date: 2024-11-17T16:17:26.620Z Has data issue: false hasContentIssue false

Magnetic Splitting of Molecular Lines in Sunspots

Published online by Cambridge University Press:  13 May 2016

S. V. Berdyugina
Affiliation:
Astronomy Division, University of Oulu, Finland
C. Frutiger
Affiliation:
Institut für Astronomie, ETHZ, Zürich, Switzerland
S. K. Solanki
Affiliation:
Max-Plank-Institut für Aeronomie, Katlenburg-Lindau, Germany

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We investigate the magnetic sensitivity of molecular lines observed in sunspot umbrae and briefly discuss their major differences compared to atomic lines.

Type
Session III: Active Region Structure and Dynamics
Copyright
Copyright © Astronomical Society of the Pacific 2001 

References

Frutiger, C., Solanki, S.K., Fligge, M., Bruls, J.H.M.J. 2000, A&A, 358, 1109.Google Scholar
Harvey, J.W. 1973, Sol. Phys., 28, 43.Google Scholar
Harvey, J.W. 1985, in NASA Marshall Space Flight Center Meas. of Solar Vector Magnetic Fields, p. 109.Google Scholar
Herzberg, G. 1950, Molecular Spectra and Molecular Structure. I. Spectra of Diatomic Molecules, NY.Google Scholar
Illing, R.M.E. 1981, ApJ, 248, 358.Google Scholar
Nicholson, S.B. 1938, PASP, 50, 224.Google Scholar
Rüedi, I., Solanki, S.K., Livingston, W., Harvey, J. 1995, A&AS, 113, 91.Google Scholar
Schadee, A. 1978, JQSRT 19, 517.Google Scholar
Solanki, S.K., Rüedi, I., Livingston, W. 1992, A&A, 263, 312.Google Scholar