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Conference Paper

Stellar irradiance variations caused by magnetic activity: the influence of an inclined rotation axis

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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/persons104262

Unruh,  Y. C.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Citation

Knaack, R., Fligge, M., Solanki, S. K., & Unruh, Y. C. (2001). Stellar irradiance variations caused by magnetic activity: the influence of an inclined rotation axis. In G. Mathys, S. K. Solanki, & D. T. Wickramasinghe (Eds.), Magnetic Fields Across the Hertzsprung-Russell Diagram (pp. 227-230). San Francisco/CA: Astronomical Society of the Pacific.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0014-E809-C
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