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Comparison of far-ultraviolet emission lines formed in coronal holes and the quiet Sun

MPS-Authors
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;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons104197

Schühle,  U.
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/persons104293

Wilhelm,  K.
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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Citation

Stucki, K., Solanki, S. K., Schühle, U., Rüedi, I., Wilhelm, K., Stenflo, J. O., et al. (2000). Comparison of far-ultraviolet emission lines formed in coronal holes and the quiet Sun. Astronomy and Astrophysics, 363, 1145-1154.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0014-E141-F
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