Measurement of the Magnetic Reconnection Rate in the Earth's Magnetotail
Abstract
In the Earth's magnetotail, magnetic reconnection releases stored magnetic energy and drives magnetospheric convection. The rate at which magnetic flux is transferred from the reconnection inflow to outflow regions is determined by the reconnection electric field Er, which is often referred to as the unnormalized reconnection rate. To better quantify the efficiency of reconnection, this electric field Er is often normalized by the characteristic Alfvén speed and the reconnecting magnetic field. This parameter is generally called the normalized or dimensionless reconnection rate R. In this paper, we employ a two–dimensional fully kinetic simulation to model a magnetotail reconnection event with weak geomagnetic activity (<200 nT of the AE index) observed by the Magnetospheric Multiscale (MMS) mission on 11 July 2017. We obtain R and Er from direct measurements in the diffusion region and indirect measurements of the rate at the separatrix using a recently proposed remote sensing technique. The measured normalized rate for this MMS event is R ~0.15–0.2, consistent with theoretical and simulation models of fast collisionless reconnection. This corresponds to an unnormalized rate of Er ~2–3 mV/m. Based on quantitative consistencies between the simulation and the MMS observations, we conclude that our estimates of the reconnection rates aremore »
- Authors:
-
- Austrian Academy of Sciences, Graz (Austria)
- Austrian Academy of Sciences, Graz (Austria); Univ. of New Hampshire, Durham, NH (United States)
- Dartmouth College, Hanover, NH (United States)
- Univ. Kebangsaan Malaysia, Bangi (Malaysia)
- JAXA, Sagamihara (Japan)
- Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
- Univ. of Bergen, Bergen (Norway); Southwest Research Institute, San Antonio, TX (United States)
- Univ. of New Hampshire, Durham, NH (United States); Southwest Research Institute, San Antonio, TX (United States)
- Southwest Research Institute, San Antonio, TX (United States)
- NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)
- Publication Date:
- Research Org.:
- Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
- Sponsoring Org.:
- National Aeronautics and Space Administration (NASA); USDOE
- OSTI Identifier:
- 1483547
- Report Number(s):
- LA-UR-18-28888
Journal ID: ISSN 2169-9380
- Grant/Contract Number:
- 89233218CNA000001
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Journal of Geophysical Research. Space Physics
- Additional Journal Information:
- Journal Volume: 123; Journal Issue: 11; Journal ID: ISSN 2169-9380
- Publisher:
- American Geophysical Union
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 58 GEOSCIENCES; magnetic reconnection; reconnection rate; MMS; magnetotail; PIC simulation; geomagnetic activity
Citation Formats
Nakamura, Takuma K. M., Genestreti, K. J., Liu, Yi -Hsin, Nakamura, R., Teh, W. -L., Hasegawa, H., Daughton, William Scott, Hesse, M., Torbert, R. B., Burch, J. L., and Giles, B. L. Measurement of the Magnetic Reconnection Rate in the Earth's Magnetotail. United States: N. p., 2018.
Web. doi:10.1029/2018JA025713.
Nakamura, Takuma K. M., Genestreti, K. J., Liu, Yi -Hsin, Nakamura, R., Teh, W. -L., Hasegawa, H., Daughton, William Scott, Hesse, M., Torbert, R. B., Burch, J. L., & Giles, B. L. Measurement of the Magnetic Reconnection Rate in the Earth's Magnetotail. United States. https://doi.org/10.1029/2018JA025713
Nakamura, Takuma K. M., Genestreti, K. J., Liu, Yi -Hsin, Nakamura, R., Teh, W. -L., Hasegawa, H., Daughton, William Scott, Hesse, M., Torbert, R. B., Burch, J. L., and Giles, B. L. Sat .
"Measurement of the Magnetic Reconnection Rate in the Earth's Magnetotail". United States. https://doi.org/10.1029/2018JA025713. https://www.osti.gov/servlets/purl/1483547.
@article{osti_1483547,
title = {Measurement of the Magnetic Reconnection Rate in the Earth's Magnetotail},
author = {Nakamura, Takuma K. M. and Genestreti, K. J. and Liu, Yi -Hsin and Nakamura, R. and Teh, W. -L. and Hasegawa, H. and Daughton, William Scott and Hesse, M. and Torbert, R. B. and Burch, J. L. and Giles, B. L.},
abstractNote = {In the Earth's magnetotail, magnetic reconnection releases stored magnetic energy and drives magnetospheric convection. The rate at which magnetic flux is transferred from the reconnection inflow to outflow regions is determined by the reconnection electric field Er, which is often referred to as the unnormalized reconnection rate. To better quantify the efficiency of reconnection, this electric field Er is often normalized by the characteristic Alfvén speed and the reconnecting magnetic field. This parameter is generally called the normalized or dimensionless reconnection rate R. In this paper, we employ a two–dimensional fully kinetic simulation to model a magnetotail reconnection event with weak geomagnetic activity (<200 nT of the AE index) observed by the Magnetospheric Multiscale (MMS) mission on 11 July 2017. We obtain R and Er from direct measurements in the diffusion region and indirect measurements of the rate at the separatrix using a recently proposed remote sensing technique. The measured normalized rate for this MMS event is R ~0.15–0.2, consistent with theoretical and simulation models of fast collisionless reconnection. This corresponds to an unnormalized rate of Er ~2–3 mV/m. Based on quantitative consistencies between the simulation and the MMS observations, we conclude that our estimates of the reconnection rates are reasonably accurate. Here, given that past studies have found Er of the order ~10 mV/m during strong geomagnetic substorms, these results indicate that the local Er in magnetotail reconnection may be an important parameter controlling the amplitude of geomagnetic disturbances.},
doi = {10.1029/2018JA025713},
journal = {Journal of Geophysical Research. Space Physics},
number = 11,
volume = 123,
place = {United States},
year = {Sat Sep 15 00:00:00 EDT 2018},
month = {Sat Sep 15 00:00:00 EDT 2018}
}
Web of Science
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