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Conference Paper

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

MPS-Authors
/persons/resource/persons104218

Solanki,  S. K.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

/persons/resource/persons104044

Lagg,  A.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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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.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0014-EE99-7
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