The origin of underdense plasma downflows associated with magnetic reconnection in solar flares
Author:
Publisher
Springer Science and Business Media LLC
Subject
Astronomy and Astrophysics
Link
https://www.nature.com/articles/s41550-021-01570-2.pdf
Reference66 articles.
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2. Haggerty, C. C. et al. The reduction of magnetic reconnection outflow jets to sub-Alfvénic speeds. Phys. Plasmas 25, 102120 (2018).
3. McKenzie, D. E. & Hudson, H. S. X-ray observations of motions and structure above a solar flare arcade. Astrophys. J. 519, L93–L96 (1999).
4. Savage, S. L., McKenzie, D. E. & Reeves, K. K. Re-interpretation of supra-arcade downflows in solar flares. Astrophys. J. Lett. 747, L40 (2012).
5. Savage, S. L. & McKenzie, D. E. Quantitative examination of a large sample of supra-arcade downflows in eruptive solar flares. Astrophys. J. 730, 98 (2011).
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