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Journal Article

Why solar magnetic flux concentrations are bright in molecular bands

MPS-Authors
http://pubman.mpdl.mpg.de/cone/persons/resource/persons104196

Schüssler,  M.
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;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons104273

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

http://pubman.mpdl.mpg.de/cone/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;

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Citation

Schüssler, M., Shelyag, S., Berdyugina, S., Vögler, A., & Solanki, S. K. (2003). Why solar magnetic flux concentrations are bright in molecular bands. Astrophysical Journal, 597, L173-L176.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0014-EE55-0
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