Publication: Driving reconnection in sheared magnetic configurations with forced fluctuations
Issued Date
2018-02-01
Resource Type
ISSN
10897674
1070664X
1070664X
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2-s2.0-85042235876
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Mahidol University
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SCOPUS
Bibliographic Citation
Physics of Plasmas. Vol.25, No.2 (2018)
Suggested Citation
Peera Pongkitiwanichakul, Kirit D. Makwana, David Ruffolo Driving reconnection in sheared magnetic configurations with forced fluctuations. Physics of Plasmas. Vol.25, No.2 (2018). doi:10.1063/1.5014026 Retrieved from: https://repository.li.mahidol.ac.th/handle/123456789/47369
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Title
Driving reconnection in sheared magnetic configurations with forced fluctuations
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Abstract
© 2018 Author(s). We investigate reconnection of magnetic field lines in sheared magnetic field configurations due to fluctuations driven by random forcing by means of numerical simulations. The simulations are performed with an incompressible, pseudo-spectral magnetohydrodynamics code in 2D where we take thick, resistively decaying, current-sheet like sheared magnetic configurations which do not reconnect spontaneously. We describe and test the forcing that is introduced in the momentum equation to drive fluctuations. It is found that the forcing does not change the rate of decay; however, it adds and removes energy faster in the presence of the magnetic shear structure compared to when it has decayed away. We observe that such a forcing can induce magnetic reconnection due to field line wandering leading to the formation of magnetic islands and O-points. These reconnecting field lines spread out as the current sheet decays with time. A semi-empirical formula is derived which reasonably explains the formation and spread of O-points. We find that reconnection spreads faster with stronger forcing and longer correlation time of forcing, while the wavenumber of forcing does not have a significant effect. When the field line wandering becomes large enough, the neighboring current sheets with opposite polarity start interacting, and then the magnetic field is rapidly annihilated. This work is useful to understand how forced fluctuations can drive reconnection in large scale current structures in space and astrophysical plasmas that are not susceptible to reconnection.