Journal article
The reduction of magnetic reconnection outflow jets to sub-Alfvenic speeds
Physics of plasmas, Vol.25(10), 102120
10/01/2018
DOI: 10.1063/1.5050530
Abstract
The outflow velocity of jets produced by collisionless magnetic reconnection is shown to be reduced by the ion exhaust temperature in fully kinetic particle in cell simulations and in situ satellite observations. We derive a scaling relationship for the outflow velocity based on the upstream Alfven speed and the parallel ion exhaust temperature, which is verified in kinetic simulations and observations. The outflow speed reduction is shown to be due to the firehose instability criterion, and so, for large enough guide fields, this effect is suppressed and the outflow speed reaches the upstream Alfven speed based on the reconnecting component of the magnetic field. Published by AIP Publishing.
Details
- Title: Subtitle
- The reduction of magnetic reconnection outflow jets to sub-Alfvenic speeds
- Creators
- Colby C. Haggerty - University of ChicagoMichael A. Shay - University of DelawareAlexandros Chasapis - University of DelawareTai D. Phan - University of California, BerkeleyJames F. Drake - University of Maryland, College ParkKittipat Malakit - Thammasat UniversityPaul A. Cassak - West Virginia UniversityRungployphan Kieokaew - University of ExeterLawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC)
- Resource Type
- Journal article
- Publication Details
- Physics of plasmas, Vol.25(10), 102120
- DOI
- 10.1063/1.5050530
- ISSN
- 1070-664X
- eISSN
- 1089-7674
- Publisher
- AIP Publishing
- Number of pages
- 6
- Grant note
- Faculty of Science at Mahidol University RTA5980003 / Thailand Research Fund; Thailand Research Fund (TRF) AGS-1460130; AGS-1460037 / NSF; National Science Foundation (NSF) NNX08A083G; NNX14AC39G; NNX15AW58G; NNX16AF75G; NNX16AG76G; NNX17AI25G / NASA; National Aeronautics & Space Administration (NASA)
- Language
- English
- Date published
- 10/01/2018
- Academic Unit
- Physics and Astronomy
- Record Identifier
- 9985224320002771
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