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The Role of Active Region Loop Geometry. II. Symmetry Breaking in Three-Dimensional Active Region: Why are Vertivcal Kink Oscillations Observed so Rarely?

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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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Selwa, M., Solanki, S. K., & Ofmann, L. (2011). The Role of Active Region Loop Geometry. II. Symmetry Breaking in Three-Dimensional Active Region: Why are Vertivcal Kink Oscillations Observed so Rarely? Astrophysical Journal, 728: 87. doi:10.1088/0004-637X/728/2/87.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0015-0685-4
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