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  New molecular indicators of sunspot magnetic fields: Infrared OH lines.

Berdyugina, S. V., Solanki, S. K., & Lagg, A. (2003). New molecular indicators of sunspot magnetic fields: Infrared OH lines. In A. A. Pevtsov, & H. Uitenbroek (Eds.), Current theoretical models and future high resolution solar observations: Preparing for ATST, ASP Conference Series, Vol. 286, held 11-15 March 2002 at NSO, Sunspot, New Mexico, USA (pp. 299). San Francisco, CA, USA: Astronomical Society of the Pacific.

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 Creators:
Berdyugina, S. V., Author
Solanki, S. K.1, 2, Author           
Lagg, A.1, 2, Author           
Affiliations:
1Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832289              
2MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832291              

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 MPIS_GROUPS: Sun and Heliosphere
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 Dates: 2003
 Publication Status: Issued
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: -
 Identifiers: ISBN: 1-58381-129-X
BibTex Citekey: Berdyugina:2003-129
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Title: Current theoretical models and future high resolution solar observations: Preparing for ATST, ASP Conference Series, Vol. 286, held 11-15 March 2002 at NSO, Sunspot, New Mexico, USA
Source Genre: Proceedings
 Creator(s):
Pevtsov, A. A., Editor
Uitenbroek, H., Editor
Affiliations:
-
Publ. Info: San Francisco, CA, USA : Astronomical Society of the Pacific
Pages: - Volume / Issue: - Sequence Number: - Start / End Page: 299 Identifier: -