Numerical comparison between a gyrofluid and gyrokinetic model investigating 
collisionless magnetic reconnection

Zacharias, O.; Comisso, L.; Grasso, D.; Kleiber, R.; Borchardt, M.; Hatzky, R.

doi:10.1063/1.4882679

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Journal Article

Numerical comparison between a gyrofluid and gyrokinetic model investigating collisionless magnetic reconnection

MPS-Authors

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Zacharias, O.
Stellarator Theory (ST), Max Planck Institute for Plasma Physics, Max Planck Society;

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Kleiber, R.
Stellarator Theory (ST), Max Planck Institute for Plasma Physics, Max Planck Society;

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Borchardt, M.
Stellarator Theory (ST), Max Planck Institute for Plasma Physics, Max Planck Society;

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Hatzky, R.
Numerical Methods in Plasma Physics (NMPP), Max Planck Institute for Plasma Physics, Max Planck Society;

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Zacharias, O., Comisso, L., Grasso, D., Kleiber, R., Borchardt, M., & Hatzky, R. (2014). Numerical comparison between a gyrofluid and gyrokinetic model investigating collisionless magnetic reconnection. Physics of Plasmas, 21: 062106. doi:10.1063/1.4882679.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0025-0BC8-0

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