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Magnetic Stereoscopy of Coronal Loops in NOAA 8891

MPS-Authors
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Feng,  L.
IMPRS on Physical Processes in the Solar System and Beyond, 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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Wiegelmann,  T.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Inhester,  B.
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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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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Ruan,  P.
IMPRS on Physical Processes in the Solar System and Beyond, Max Planck Institute for Solar System Research, Max Planck Society;

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Citation

Feng, L., Wiegelmann, T., Inhester, B., Solanki, S. K., Gan, W. Q., & Ruan, P. (2007). Magnetic Stereoscopy of Coronal Loops in NOAA 8891. Solar Physics, 241, 235-249. doi:10.1007/s11207-007-0370-z.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0014-FCE2-3
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