Kinetic evolution of the Orszag‐Tang vortex is studied using collisionless hybrid simulations based on particle in cell ions and fluid electrons. In magnetohydrodynamics (MHD) this configuration leads rapidly to broadband turbulence. An earlier study [1] estimated the dissipation in the system. A comparison of MHD & hybrid simulations showed similar behavior at large scales but substantial differences at small scales. The hybrid magnetic energy spectrum shows a break at the scale where Hall term in the Ohm’s law becomes important. The protons heat perpendicularly and most of the energy is dissipated through magnetic interactions. Here, the space time structure of the system is studied using frequency‐wavenumber (k‐ω) decomposition. No clear resonances appear, ruling out the cyclotron resonances as a likely candidate for the perpendicular heating. The only distinguishable wave modes present, which constitute a small percentage of total energy, are magnetosonic modes.
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25 March 2010
TWELFTH INTERNATIONAL SOLAR WIND CONFERENCE
21–26 June 2009
Saint‐Malo, (France)
Research Article|
March 25 2010
Orszag Tang vortex—Kinetic study of a turbulent plasma
T. N. Parashar;
T. N. Parashar
aDepartment of Physics & Astronomy, 217 Sharp Lab, University of Delaware, Newark, Delaware 19716, USA
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S. Servidio;
S. Servidio
aDepartment of Physics & Astronomy, 217 Sharp Lab, University of Delaware, Newark, Delaware 19716, USA
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M. A. Shay;
M. A. Shay
aDepartment of Physics & Astronomy, 217 Sharp Lab, University of Delaware, Newark, Delaware 19716, USA
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W. H. Matthaeus;
W. H. Matthaeus
aDepartment of Physics & Astronomy, 217 Sharp Lab, University of Delaware, Newark, Delaware 19716, USA
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P. A. Cassak
P. A. Cassak
aDepartment of Physics & Astronomy, 217 Sharp Lab, University of Delaware, Newark, Delaware 19716, USA
bDepartment of Physics, Hodges Hall, Box 6315, West Virginia University, Morgantown, WV 26506
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AIP Conf. Proc. 1216, 304–307 (2010)
Citation
T. N. Parashar, S. Servidio, M. A. Shay, W. H. Matthaeus, P. A. Cassak; Orszag Tang vortex—Kinetic study of a turbulent plasma. AIP Conf. Proc. 25 March 2010; 1216 (1): 304–307. https://doi.org/10.1063/1.3395861
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