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On the relation between continuum brightness and magnetic field in solar active regions

MPS-Authors
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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;

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Röhrbein,  D.
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;

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Cameron,  R. H.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Schüssler,  M.
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

Danilovic, S., Röhrbein, D., Cameron, R. H., & Schüssler, M. (2013). On the relation between continuum brightness and magnetic field in solar active regions. Astronomy and Astrophysics, 550: A118. doi:10.1051/0004-6361/201219726.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0015-0A72-C
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