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Title: 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 » the distances comparable to the flare loop length.« less

Authors:
ORCiD logo [1]; ORCiD logo [1]; ORCiD logo [1]; ORCiD logo [1]; ORCiD logo [2]; ORCiD logo [3]; ORCiD logo [4]
  1. Univ. of Delaware, Newark, DE (United States). Dept. of Physics and Astronomy
  2. Univ. of Maryland, College Park, MD (United States)
  3. West Virginia Univ., Morgantown, WV (United States)
  4. 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}
}

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Works referenced in this record:

Electron Trapping in Shear Alfvén Waves that Power the Aurora
journal, January 2009


Current disruption in the Earth's magnetosphere: Observations and models
journal, June 1996

  • Lui, A. T. Y.
  • Journal of Geophysical Research: Space Physics, Vol. 101, Issue A6
  • DOI: 10.1029/96JA00079

Development of parallel electric fields at the plasma sheet boundary layer: PARALLEL ELECTRIC FIELD AT PSBL
journal, January 2011

  • Lysak, Robert L.; Song, Yan
  • Journal of Geophysical Research: Space Physics, Vol. 116, Issue A1
  • DOI: 10.1029/2010JA016424

Tail Reconnection Triggering Substorm Onset
journal, August 2008


Auroral ion acceleration in dispersive Alfvén waves
journal, January 2004


Laminar wave-train structure of collisionless magnetic slow shocks
journal, May 1971


Impulsive Phase Flare Energy Transport by Large‐Scale Alfvén Waves and the Electron Acceleration Problem
journal, March 2008

  • Fletcher, L.; Hudson, H. S.
  • The Astrophysical Journal, Vol. 675, Issue 2
  • DOI: 10.1086/527044

On the kinetic dispersion relation for shear Alfvén waves
journal, March 1996

  • Lysak, Robert L.; Lotko, William
  • Journal of Geophysical Research: Space Physics, Vol. 101, Issue A3
  • DOI: 10.1029/95JA03712

Neutral line model of substorms: Past results and present view
journal, June 1996

  • Baker, D. N.; Pulkkinen, T. I.; Angelopoulos, V.
  • Journal of Geophysical Research: Space Physics, Vol. 101, Issue A6
  • DOI: 10.1029/95JA03753

Comment on "Tail Reconnection Triggering Substorm Onset"
journal, June 2009


Three-dimensional particle simulations of collisionless magnetic reconnection
journal, January 2002


The Global Morphology of Wave Poynting Flux: Powering the Aurora
journal, January 2003


Response to Comment on "Tail Reconnection Triggering Substorm Onset"
journal, June 2009


Propagation of Alfvén waves in the magnetotail during substorms
journal, January 2009


Propagation speed of rotation signals for field lines undergoing magnetic reconnection
journal, October 2013

  • Lapenta, Giovanni; Goldman, Martin; Newman, David
  • Physics of Plasmas, Vol. 20, Issue 10
  • DOI: 10.1063/1.4825132

Role of Dispersive Waves in Collisionless Magnetic Reconnection
journal, October 2001


Equatorward moving auroral signatures of a flow burst observed prior to auroral onset
journal, January 2009

  • Kepko, L.; Spanswick, E.; Angelopoulos, V.
  • Geophysical Research Letters, Vol. 36, Issue 24
  • DOI: 10.1029/2009GL041476

Do magnetospheric shear Alfvén waves generate sufficient electron energy flux to power the aurora?: ELECTRON ACCELERATION
journal, July 2010

  • Watt, C. E. J.; Rankin, R.
  • Journal of Geophysical Research: Space Physics, Vol. 115, Issue A7
  • DOI: 10.1029/2009JA015185

Wave-particle energy exchange directly observed in a kinetic Alfvén-branch wave
journal, March 2017

  • Gershman, Daniel J.; F-Viñas, Adolfo; Dorelli, John C.
  • Nature Communications, Vol. 8, Issue 1
  • DOI: 10.1038/ncomms14719

Super-Alfvénic Propagation of Substorm Reconnection Signatures and Poynting Flux
journal, August 2011


Ion temperature effects on magnetotail Alfvén wave propagation and electron energization: ION TEMPERATURE EFFECTS ON ALFVÉN WAVES
journal, July 2015

  • Damiano, P. A.; Johnson, J. R.; Chaston, C. C.
  • Journal of Geophysical Research: Space Physics, Vol. 120, Issue 7
  • DOI: 10.1002/2015JA021074

Ion gyroradius effects on particle trapping in kinetic Alfvén waves along auroral field lines: PARTICLE TRAPPING IN KAWS
journal, November 2016

  • Damiano, P. A.; Johnson, J. R.; Chaston, C. C.
  • Journal of Geophysical Research: Space Physics, Vol. 121, Issue 11
  • DOI: 10.1002/2016JA022566

Theory of Space Plasma Microinstabilities
book, January 2009


Works referencing / citing this record:

Transition from ion-coupled to electron-only reconnection: Basic physics and implications for plasma turbulence
journal, August 2019

  • Sharma Pyakurel, P.; Shay, M. A.; Phan, T. D.
  • Physics of Plasmas, Vol. 26, Issue 8
  • DOI: 10.1063/1.5090403