Super-Alfvénic Propagation and Damping of Reconnection Onset Signatures
Abstract
The quadrupolar out-of-plane Hall magnetic leld generated during collisionless reconnection propagates away from the x line as a kinetic Alfvén wave (KAW). While it has been shown that this KAW carries substantial Poynting flux and propagates super-Alfvenically, how this KAW damps as it propagates away from the x line is not well understood. In this study, this damping is examined using kinetic particle-in-cell simulations of antiparallel symmetric magnetic reconnection in a one-dimensional current sheet equilibrium. In the reconnection simulations, the KAW wave vector has a typical magnitude comparable to an inverse fluid Larmor radius (effectively an inverse ion Larmor radius) and a direction of 85–89°relative to the local magnetic field. We find that the damping of the reconnection KAW is consistent with linear Landau damping results from a numerical Vlasov dispersion solver. This knowledge allows us to generalize our damping predictions to regions in the magnetotail and solar corona where the magnetic geometry can be approximated as a current sheet. For the magneto tail, the KAW from reconnection will not damp away before propagating the approximately 20 Earth radii associated with global magneto tail distances. For the solar corona, on the other hand, these KAWs will completely damp before reachingmore »
- Authors:
-
- Univ. of Delaware, Newark, DE (United States). Dept. of Physics and Astronomy
- Univ. of Maryland, College Park, MD (United States)
- West Virginia Univ., Morgantown, WV (United States)
- Space Science Inst., Boulder, CO (United States)
- Publication Date:
- Research Org.:
- Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC)
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 1461626
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Journal of Geophysical Research. Space Physics
- Additional Journal Information:
- Journal Volume: 123; Journal Issue: 1; Journal ID: ISSN 2169-9380
- Publisher:
- American Geophysical Union
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS
Citation Formats
Sharma Pyakurel, P., Shay, M. A., Haggerty, C. C., Parashar, T. N., Drake, J. F., Cassak, P. A., and Gary, S. Peter. Super-Alfvénic Propagation and Damping of Reconnection Onset Signatures. United States: N. p., 2017.
Web. doi:10.1002/2017JA024606.
Sharma Pyakurel, P., Shay, M. A., Haggerty, C. C., Parashar, T. N., Drake, J. F., Cassak, P. A., & Gary, S. Peter. Super-Alfvénic Propagation and Damping of Reconnection Onset Signatures. United States. https://doi.org/10.1002/2017JA024606
Sharma Pyakurel, P., Shay, M. A., Haggerty, C. C., Parashar, T. N., Drake, J. F., Cassak, P. A., and Gary, S. Peter. Tue .
"Super-Alfvénic Propagation and Damping of Reconnection Onset Signatures". United States. https://doi.org/10.1002/2017JA024606. https://www.osti.gov/servlets/purl/1461626.
@article{osti_1461626,
title = {Super-Alfvénic Propagation and Damping of Reconnection Onset Signatures},
author = {Sharma Pyakurel, P. and Shay, M. A. and Haggerty, C. C. and Parashar, T. N. and Drake, J. F. and Cassak, P. A. and Gary, S. Peter},
abstractNote = {The quadrupolar out-of-plane Hall magnetic leld generated during collisionless reconnection propagates away from the x line as a kinetic Alfvén wave (KAW). While it has been shown that this KAW carries substantial Poynting flux and propagates super-Alfvenically, how this KAW damps as it propagates away from the x line is not well understood. In this study, this damping is examined using kinetic particle-in-cell simulations of antiparallel symmetric magnetic reconnection in a one-dimensional current sheet equilibrium. In the reconnection simulations, the KAW wave vector has a typical magnitude comparable to an inverse fluid Larmor radius (effectively an inverse ion Larmor radius) and a direction of 85–89°relative to the local magnetic field. We find that the damping of the reconnection KAW is consistent with linear Landau damping results from a numerical Vlasov dispersion solver. This knowledge allows us to generalize our damping predictions to regions in the magnetotail and solar corona where the magnetic geometry can be approximated as a current sheet. For the magneto tail, the KAW from reconnection will not damp away before propagating the approximately 20 Earth radii associated with global magneto tail distances. For the solar corona, on the other hand, these KAWs will completely damp before reaching the distances comparable to the flare loop length.},
doi = {10.1002/2017JA024606},
journal = {Journal of Geophysical Research. Space Physics},
number = 1,
volume = 123,
place = {United States},
year = {Tue Dec 05 00:00:00 EST 2017},
month = {Tue Dec 05 00:00:00 EST 2017}
}
Web of Science
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Works referencing / citing this record:
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