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Aspects of Collisionless Magnetic Reconnection in Asymmetric SystemsAsymmetric reconnection is being investigated by means of particle-in-cell simulations. The research has two foci: The direction of the reconnection line in configurations with nonvanishing magnetic fields; and the question why reconnection can be faster if a guide field is added to an otherwise unchanged asymmetric configuration. We find that reconnection prefers a direction, which maximizes the available magnetic energy, and show that this direction coincides with the bisection of the angle between the asymptotic magnetic fields. Regarding the difference in reconnection rates between planar and guide field models, we demonstrate that a guide field can provide essential confinement for particles in the reconnection region, which the weaker magnetic field in one of the inflow directions cannot necessarily provide.


Document ID
20150017061
Acquisition Source
Goddard Space Flight Center
Document Type
Preprint (Draft being sent to journal)
Authors
Hesse, Michael
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Aunai, Nicolas
(Oak Ridge Associated Universities Greenbelt, MD, United States)
Zenitani, Seiji
(National Astronomical Observatory Gunma, Japan)
Kuznetsova, Masha
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Birn, Joachim
(Space Science Inst. Boulder, CO, United States)
Date Acquired
September 4, 2015
Publication Date
May 15, 2013
Subject Category
Solar Physics
Report/Patent Number
GSFC-E-DAA-TN7398
Funding Number(s)
CONTRACT_GRANT: NNH06CC03B
Distribution Limits
Public
Copyright
Public Use Permitted.
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