Whistler Mode Based Explanation for the Fast Reconnection Rate Measured in the MIT Versatile Toroidal Facility
Creators
- 1. Electrical and Computer Engineering, University of Alabama, Huntsville, Alabama 35899 (United States)
Description
Despite the widely discussed role of whistler waves in mediating magnetic reconnection (MR), the direct connection between such waves and the MR has not been demonstrated by comparing the characteristic temporal and spatial features of the waves and the MR process. Using the whistler wave dispersion relation, we theoretically predict the experimentally measured rise time (τrise) of a few microseconds for the fast rising MR rate in the Versatile Toroidal Facility at MIT. The rise time is closely given by the inverse of the frequency bandwidth of the whistler waves generated in the evolving current sheet. The wave frequencies lie much above the ion cyclotron frequency, but they are limited to less than 0.1% of the electron cyclotron frequency in the argon plasma. The maximum normalized MR rate R=0.35 measured experimentally is precisely predicted by the angular dispersion of the whistler waves.
Additional details
Identifiers
Publishing Information
- Journal Title
- Physical Review Letters
- Journal Volume
- 107
- Journal Issue
- 24
- Journal Page Range
- p. 245003-245003.4
- ISSN
- 0031-9007
- CODEN
- PRLTAO
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 43091209
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY; S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- ARGON; CYCLOTRON FREQUENCY; DISPERSION RELATIONS; ELECTRONS; MAGNETIC RECONNECTION; PLASMA; PULSE RISE TIME; WHISTLER INSTABILITY; WHISTLERS
- Descriptors DEC
- ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; ELEMENTS; FERMIONS; FLUIDS; GASES; INSTABILITY; LEPTONS; NOISE; NONMETALS; PLASMA INSTABILITY; PLASMA MACROINSTABILITIES; RADIATIONS; RADIO NOISE; RADIOWAVE RADIATION; RARE GASES; TIMING PROPERTIES
Optional Information
- Notes
- (c) 2011 American Institute of Physics