TY - JOUR
T1 - Energy transfer and electron energization in collisionless magnetic reconnection for different guide-field intensities
AU - Pucci, F.
AU - Usami, S.
AU - Ji, H.
AU - Guo, X.
AU - Horiuchi, R.
AU - Okamura, S.
AU - Fox, W.
AU - Jara-Almonte, J.
AU - Yamada, M.
AU - Yoo, J.
N1 - Funding Information:
F. Pucci would like to thank Dr. R. Kumar, Dr. D. Del Sarto, and Dr. M. Innocenti for interesting discussions on the interpretation of energy partition and electron temperature. This simulation work was performed by means of the Plasma Simulator at the National Institute for Fusion Science (NIFS) with the support and under the auspices of the NIFS Collaboration Research Program (NIFS17KNSS085). This work was supported by the Strategic International Research Exchange Promotion Program in the National Institutes of Natural Sciences, Japan; Grant-in-Aid from the Japan Society for the Promotion of Science (JSPS) Fellows 15J03758; Grant-in-Aid for Scientific Research 15H05750; the Max-Planck Princeton Center for Plasma Physics, funded by the U.S. Department of Energy under Contract No. DE-AC0204CH11466; and NASA under Agreement Nos. NNH15AB29I and NNH14AX631.
Publisher Copyright:
© 2018 Author(s).
PY - 2018/12/1
Y1 - 2018/12/1
N2 - Electron dynamics and energization are one of the key components of magnetic field dissipation in collisionless reconnection. In 2D numerical simulations of magnetic reconnection, the main mechanism that limits the current density and provides an effective dissipation is most probably the electron pressure tensor term, which has been shown to break the frozen-in condition at the x-point. In addition, the electron-meandering-orbit scale controls the width of the electron dissipation region, where the electron temperature has been observed to increase both in recent Magnetospheric Multiple-Scale (MMS) observations and in laboratory experiments, such as the Magnetic Reconnection Experiment (MRX). By means of two-dimensional full-particle simulations in an open system, we investigate how the energy conversion and particle energization depend on the guide field intensity. We study the energy transfer from the magnetic field to the plasma in the vicinity of the x-point and close downstream regions, and E·J and the threshold guide field separating two regimes where either the parallel component, E||J||, or the perpendicular component, E⊥·J⊥, dominate the energy transfer, confirming recent MRX results and also consistent with MMS observations. We calculate the energy partition between fields and kinetic and thermal energies of different species, from electron to ion scales, showing that there is no significant variation for different guide field configurations. Finally, we study possible mechanisms for electron perpendicular heating by examining electron distribution functions and self-consistently evolved particle orbits in high guide field configurations.
AB - Electron dynamics and energization are one of the key components of magnetic field dissipation in collisionless reconnection. In 2D numerical simulations of magnetic reconnection, the main mechanism that limits the current density and provides an effective dissipation is most probably the electron pressure tensor term, which has been shown to break the frozen-in condition at the x-point. In addition, the electron-meandering-orbit scale controls the width of the electron dissipation region, where the electron temperature has been observed to increase both in recent Magnetospheric Multiple-Scale (MMS) observations and in laboratory experiments, such as the Magnetic Reconnection Experiment (MRX). By means of two-dimensional full-particle simulations in an open system, we investigate how the energy conversion and particle energization depend on the guide field intensity. We study the energy transfer from the magnetic field to the plasma in the vicinity of the x-point and close downstream regions, and E·J and the threshold guide field separating two regimes where either the parallel component, E||J||, or the perpendicular component, E⊥·J⊥, dominate the energy transfer, confirming recent MRX results and also consistent with MMS observations. We calculate the energy partition between fields and kinetic and thermal energies of different species, from electron to ion scales, showing that there is no significant variation for different guide field configurations. Finally, we study possible mechanisms for electron perpendicular heating by examining electron distribution functions and self-consistently evolved particle orbits in high guide field configurations.
UR - http://www.scopus.com/inward/record.url?scp=85058057679&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85058057679&partnerID=8YFLogxK
U2 - 10.1063/1.5050992
DO - 10.1063/1.5050992
M3 - Article
AN - SCOPUS:85058057679
SN - 1070-664X
VL - 25
JO - Physics of Plasmas
JF - Physics of Plasmas
IS - 12
M1 - 122111
ER -