Rayleigh-Taylor Type Instabilities in the Reconnection Exhaust Jet as a 
Mechanism for Supra-Arcade Downflows in the Sun

Guo, L.-J.; Huang, Y.-M.; Bhattacharjee, A.; Innes, D. E.

doi:10.1088/2041-8205/796/2/L29

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Rayleigh-Taylor Type Instabilities in the Reconnection Exhaust Jet as a Mechanism for Supra-Arcade Downflows in the Sun

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

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Innes, D. E.
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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Guo, L.-J., Huang, Y.-M., Bhattacharjee, A., & Innes, D. E. (2014). Rayleigh-Taylor Type Instabilities in the Reconnection Exhaust Jet as a Mechanism for Supra-Arcade Downflows in the Sun. Astrophysical Journal, 796(2): L29. doi:10.1088/2041-8205/796/2/L29.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0027-7C3E-3

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