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Loop morphology and flows and their relation to the magnetic field

MPS-Authors
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Teriaca,  L.
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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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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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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Curdt,  W.
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

Teriaca, L., Wiegelmann, T., Lagg, A., Solanki, S. K., Curdt, W., Sekii, T., et al. (2008). Loop morphology and flows and their relation to the magnetic field. In S. Matthews, J. M. Davis, & L. K. Harra (Eds.), First Results from Hinode (pp. 196).


Cite as: http://hdl.handle.net/11858/00-001M-0000-0014-FFD1-B
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