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Three-dimensional magnetic field topology in a region of solar coronal heating

MPS-Authors
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;

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/persons104296

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

http://pubman.mpdl.mpg.de/cone/persons/resource/persons104038

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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Citation

Solanki, S. K., Lagg, A., Woch, J., Krupp, N., & Collados, M. (2003). Three-dimensional magnetic field topology in a region of solar coronal heating. Nature, 425, 692-695. doi:10.1038/nature02035.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0014-EE43-7
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