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Relationship between line shift and intensity inside coronal holes

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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/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;

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Stucki, K., Solanki, S. K., Rüedi, I., & Schühle, U. (1999). Relationship between line shift and intensity inside coronal holes. In J.-C. Vial, & B. Kaldeich-Schürmann (Eds.), Proc. 8th SOHO Workshop `Plasma Dynamics and Diagnostics in the Solar Transition Region and Corona', Paris, France, 22-25 June 1999 (pp. 633-637). Noordwijk: ESA Publ. Div.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0014-DE71-7
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