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

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.

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 Creators:
Knaack, R., Author
Fligge, M., Author
Solanki, S. K.1, 2, Author           
Unruh, Y. C.1, Author           
Affiliations:
1Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832289              
2MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832291              

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 MPIS_GROUPS: Sun and Heliosphere
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 Dates: 2001
 Publication Status: Issued
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: -
 Identifiers: BibTex Citekey: Knaack:2001-116
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Title: Magnetic Fields Across the Hertzsprung-Russell Diagram
Source Genre: Proceedings
 Creator(s):
Mathys, G., Editor
Solanki, S. K.1, 2, Editor           
Wickramasinghe, D. T., Editor
Affiliations:
1 Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832289            
2 MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832291            
Publ. Info: San Francisco/CA : Astronomical Society of the Pacific
Pages: - Volume / Issue: - Sequence Number: - Start / End Page: 227 - 230 Identifier: -