Journal
JOURNAL OF PLASMA PHYSICS
Volume 83, Issue 5, Pages -Publisher
CAMBRIDGE UNIV PRESS
DOI: 10.1017/S0022377817000666
Keywords
astrophysical plasmas; fusion plasma; space plasma physics
Categories
Funding
- NSF [AGS-1460037]
- NASA [NNX16AG76G, NNX16AG75G, NNX15AW58G]
- NASA [904132, NNX16AG75G, NNX16AG76G, 904779] Funding Source: Federal RePORTER
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A long-standing problem in magnetic reconnection is to explain why it tends to proceed at or below a normalized rate of 0.1. This article gives a review of observational and numerical evidence for this rate and discusses recent theoretical work addressing this problem. Some remaining open questions are summarized.
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