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Numerical comparison between a gyrofluid and gyrokinetic model investigating collisionless magnetic reconnection
- Source :
- Physics of Plasmas, Physics of plasmas 21 (2014): 062106. doi:10.1063/1.4882679, info:cnr-pdr/source/autori:O. Zacharias (1); L. Comisso (2,3); D. Grasso (2,3); R. Kleiber (1); M. Borchardt (1); R. Hatzky (4)/titolo:Numerical comparison between a gyrofluid and gyrokinetic model investigating collisionless magnetic reconnection/doi:10.1063%2F1.4882679/rivista:Physics of plasmas/anno:2014/pagina_da:062106/pagina_a:/intervallo_pagine:062106/volume:21
- Publication Year :
- 2014
-
Abstract
- The first detailed comparison between gyrokinetic and gyrofluid simulations of collisionless magnetic reconnection has been carried out. Both the linear and nonlinear evolution of the collisionless tearing mode have been analyzed. In the linear regime, we have found a good agreement between the two approaches over the whole spectrum of linearly unstable wave numbers, both in the drift kinetic limit and for finite ion temperature. Nonlinearly, focusing on the small-$\Delta '$ regime, with $\Delta '$ indicating the standard tearing stability parameter, we have compared relevant observables such as the evolution and saturation of the island width, as well as the island oscillation frequency in the saturated phase.The results are basically the same, with small discrepancies only in the value of the saturated island width for moderately high values of $\Delta '$. Therefore, in the regimes investigated here, the gyrofluid approach can describe the collisionless reconnection process as well as the more complete gyrokinetic model.<br />Comment: Accepted for publication on Physics of Plasmas
- Subjects :
- Physics
Oscillation
FOS: Physical sciences
Observable
Magnetic reconnection
Computational Physics (physics.comp-ph)
Condensed Matter Physics
Kinetic energy
Physics - Plasma Physics
Plasma Physics (physics.plasm-ph)
Astrophysics - Solar and Stellar Astrophysics
Physics::Plasma Physics
Quantum electrodynamics
Tearing
Physics::Space Physics
Wavenumber
Limit (mathematics)
Saturation (chemistry)
Physics - Computational Physics
Solar and Stellar Astrophysics (astro-ph.SR)
collisionless magnetic reconnection
Subjects
Details
- ISSN :
- 1070664X
- Database :
- OpenAIRE
- Journal :
- Physics of Plasmas
- Accession number :
- edsair.doi.dedup.....d658691b411bea5267bf9d23c2478bed
- Full Text :
- https://doi.org/10.1063/1.4882679