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  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. (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.

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 Creators:
Guo, L.-J.1, Author           
Huang, Y.-M., Author
Bhattacharjee, A., Author
Innes, D. E.1, 2, Author           
Affiliations:
1Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832289              
2MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832291              

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 MPIS_GROUPS: Sun and Heliosphere
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 Dates: 2014
 Publication Status: Issued
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 Rev. Type: Peer
 Identifiers: DOI: 10.1088/2041-8205/796/2/L29
BibTex Citekey: Guo:2014-267
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Title: Astrophysical Journal
Source Genre: Journal
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Pages: - Volume / Issue: 796 (2) Sequence Number: L29 Start / End Page: - Identifier: -