Global three-dimensional simulation of Earth's dayside reconnection using a two-way coupled magnetohydrodynamics with embedded particle-in-cell model: initial results: 3D MHD-EPIC simulation of magnetosphere
Abstract
Abstract We perform a three‐dimensional (3‐D) global simulation of Earth's magnetosphere with kinetic reconnection physics to study the flux transfer events (FTEs) and dayside magnetic reconnection with the recently developed magnetohydrodynamics with embedded particle‐in‐cell model. During the 1 h long simulation, the FTEs are generated quasi‐periodically near the subsolar point and move toward the poles. We find that the magnetic field signature of FTEs at their early formation stage is similar to a “crater FTE,” which is characterized by a magnetic field strength dip at the FTE center. After the FTE core field grows to a significant value, it becomes an FTE with typical flux rope structure. When an FTE moves across the cusp, reconnection between the FTE field lines and the cusp field lines can dissipate the FTE. The kinetic features are also captured by our model. A crescent electron phase space distribution is found near the reconnection site. A similar distribution is found for ions at the location where the Larmor electric field appears. The lower hybrid drift instability (LHDI) along the current sheet direction also arises at the interface of magnetosheath and magnetosphere plasma. The LHDI electric field is about 8 mV/m, and its dominant wavelength relative to themore »
- Authors:
-
- Univ. of Michigan, Ann Arbor, MI (United States). Center for Space Environment Modeling
- West Virginia Univ., Morgantown, WV (United States). Dept. of Physics and Astronomy
- Center for Space Environment Modeling, University of Michigan, Ann Arbor MI USA
- KTH Royal Inst. of Technology, Stockholm (Sweden)
- Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
- Publication Date:
- Research Org.:
- Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
- Sponsoring Org.:
- National Science Foundation (NSF); USDOE
- OSTI Identifier:
- 1394984
- Alternate Identifier(s):
- OSTI ID: 1485749
- Report Number(s):
- LA-UR-17-25622
Journal ID: ISSN 2169-9380
- Grant/Contract Number:
- AC52-06NA25396; ACI-1640510
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Journal of Geophysical Research. Space Physics
- Additional Journal Information:
- Journal Volume: 122; Journal Issue: 10; Journal ID: ISSN 2169-9380
- Publisher:
- American Geophysical Union
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 58 GEOSCIENCES; Heliospheric and Magnetospheric Physics
Citation Formats
Chen, Yuxi, Tóth, Gábor, Cassak, Paul, Jia, Xianzhe, Gombosi, Tamas I., Slavin, James A., Markidis, Stefano, Peng, Ivy Bo, Jordanova, Vania K., and Henderson, Michael G. Global three-dimensional simulation of Earth's dayside reconnection using a two-way coupled magnetohydrodynamics with embedded particle-in-cell model: initial results: 3D MHD-EPIC simulation of magnetosphere. United States: N. p., 2017.
Web. doi:10.1002/2017JA024186.
Chen, Yuxi, Tóth, Gábor, Cassak, Paul, Jia, Xianzhe, Gombosi, Tamas I., Slavin, James A., Markidis, Stefano, Peng, Ivy Bo, Jordanova, Vania K., & Henderson, Michael G. Global three-dimensional simulation of Earth's dayside reconnection using a two-way coupled magnetohydrodynamics with embedded particle-in-cell model: initial results: 3D MHD-EPIC simulation of magnetosphere. United States. https://doi.org/10.1002/2017JA024186
Chen, Yuxi, Tóth, Gábor, Cassak, Paul, Jia, Xianzhe, Gombosi, Tamas I., Slavin, James A., Markidis, Stefano, Peng, Ivy Bo, Jordanova, Vania K., and Henderson, Michael G. Mon .
"Global three-dimensional simulation of Earth's dayside reconnection using a two-way coupled magnetohydrodynamics with embedded particle-in-cell model: initial results: 3D MHD-EPIC simulation of magnetosphere". United States. https://doi.org/10.1002/2017JA024186. https://www.osti.gov/servlets/purl/1394984.
@article{osti_1394984,
title = {Global three-dimensional simulation of Earth's dayside reconnection using a two-way coupled magnetohydrodynamics with embedded particle-in-cell model: initial results: 3D MHD-EPIC simulation of magnetosphere},
author = {Chen, Yuxi and Tóth, Gábor and Cassak, Paul and Jia, Xianzhe and Gombosi, Tamas I. and Slavin, James A. and Markidis, Stefano and Peng, Ivy Bo and Jordanova, Vania K. and Henderson, Michael G.},
abstractNote = {Abstract We perform a three‐dimensional (3‐D) global simulation of Earth's magnetosphere with kinetic reconnection physics to study the flux transfer events (FTEs) and dayside magnetic reconnection with the recently developed magnetohydrodynamics with embedded particle‐in‐cell model. During the 1 h long simulation, the FTEs are generated quasi‐periodically near the subsolar point and move toward the poles. We find that the magnetic field signature of FTEs at their early formation stage is similar to a “crater FTE,” which is characterized by a magnetic field strength dip at the FTE center. After the FTE core field grows to a significant value, it becomes an FTE with typical flux rope structure. When an FTE moves across the cusp, reconnection between the FTE field lines and the cusp field lines can dissipate the FTE. The kinetic features are also captured by our model. A crescent electron phase space distribution is found near the reconnection site. A similar distribution is found for ions at the location where the Larmor electric field appears. The lower hybrid drift instability (LHDI) along the current sheet direction also arises at the interface of magnetosheath and magnetosphere plasma. The LHDI electric field is about 8 mV/m, and its dominant wavelength relative to the electron gyroradius agrees reasonably with Magnetospheric Multiscale (MMS) observations.},
doi = {10.1002/2017JA024186},
journal = {Journal of Geophysical Research. Space Physics},
number = 10,
volume = 122,
place = {United States},
year = {Mon Sep 18 00:00:00 EDT 2017},
month = {Mon Sep 18 00:00:00 EDT 2017}
}
Web of Science
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