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Conference Paper

Modeling the Fine Structure of a Sunspot Penumbra through the Inversion of Stokes Profiles

MPS-Authors
http://pubman.mpdl.mpg.de/cone/persons/resource/persons103843

Borrero,  J. M.
IMPRS on Physical Processes in the Solar System and Beyond, Max Planck Institute for Solar System Research, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons104044

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;

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;

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Citation

Borrero, J. M., Lagg, A., Solanki, S. K., Frutiger, C., Collados, M., & Bellot Rubio, L. R. (2003). Modeling the Fine Structure of a Sunspot Penumbra through the Inversion of Stokes Profiles. In A. A. Pevtsov, & H. Uitenbroek (Eds.), Current Theoretical Models and Future High Resolution Solar Observations: Preparing for ATST (pp. 235).


Cite as: http://hdl.handle.net/11858/00-001M-0000-0014-F1E1-8
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