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IRIS Si IV Line Profiles: An Indication for the Plasmoid Instability During Small-scale Magnetic Reconnection on the Sun

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Innes,  Davina
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,  Lijia
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Innes, D., Guo, L., Huang, Y.-M., & Bhattacharjee, A. (2015). IRIS Si IV Line Profiles: An Indication for the Plasmoid Instability During Small-scale Magnetic Reconnection on the Sun. Astrophysical Journal, 813, 86-96. doi:10.1088/0004-637X/813/2/86.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0029-B726-6
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