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Thermal-magnetic relation of a sunspot as inferred from inversion of 1.5 μm spectral data

MPS-Authors
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Mathew,  S. K.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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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;

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Lagg,  A.
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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Krupp,  N.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Woch,  J.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Citation

Mathew, S. K., Solanki, S. K., Lagg, A., Collados, M., Berdyugina, S., Frutiger, C., et al. (2002). Thermal-magnetic relation of a sunspot as inferred from inversion of 1.5 μm spectral data. In H. Sawaya-Lacoste (Ed.), SOLMAG 2002, Proceedings of the Magnetic Coupling of the Solar Atmosphere, Euroconference and IAU Colloquium 188, (pp. 501-504). Noordwijk: ESA Publ. Div.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0014-EC0F-2
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