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Conference Paper

Magnetic source of the solar cycle variation of the Mn I 539.4 nm line

MPS-Authors
/persons/resource/persons103879

Danilovic,  S.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
IMPRS on Physical Processes in the Solar System and Beyond, Max Planck Institute for Solar System Research, Max Planck Society;

/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;

/persons/resource/persons104034

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

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Citation

Danilovic, S., Solanki, S. K., Livingston, W., Krivova, N. A., & Vince, I. (2007). Magnetic source of the solar cycle variation of the Mn I 539.4 nm line. In F. Kneer, K. G. Puschmann, & A. D. Wittmann (Eds.), Modern solar facilities-Advanced Solar Science (pp. 189-192). Göttingen: Universitätsverlag Göttingen.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0014-FE63-B
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