Research output: Contribution to journal › Article › peer-review
The Inertia-Based Model for Reconstruction of the Electron Diffusion Region. / Korovinskiy, D. B.; Kiehas, S. A.; Panov, E. V.; Semenov, V. S.; Erkaev, N. V.; Divin, A. V.; Kubyshkin, I. V.
In: journal of geophysical research: Space Physics, Vol. 126, No. 5, e2020JA029045, 05.2021.Research output: Contribution to journal › Article › peer-review
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TY - JOUR
T1 - The Inertia-Based Model for Reconstruction of the Electron Diffusion Region
AU - Korovinskiy, D. B.
AU - Kiehas, S. A.
AU - Panov, E. V.
AU - Semenov, V. S.
AU - Erkaev, N. V.
AU - Divin, A. V.
AU - Kubyshkin, I. V.
N1 - Publisher Copyright: © 2021. American Geophysical Union. All Rights Reserved.
PY - 2021/5
Y1 - 2021/5
N2 - The present study is focused on the problem of reconstruction of the magnetic configuration in the magnetic reconnection electron diffusion region (EDR). The problem is addressed in the frame of electron magnetohydrodynamics with kept electron inertia term. We introduce the new reconstruction model independent of divergence of the electron pressure tensor and reconnection electric field. The model is tested on the magnetotail reconnection event of July 11, 2017 observed by the Magnetospheric Multiscale (MMS) spacecraft in the course of crossing the very core part of the reconnection region, the internal EDR. This new model demonstrates considerably better accuracy of the longitudinal electron velocity reconstruction due to the lower sensitivity to the configuration deviation from the two-dimensional time-independent model adopted in our study. We suggest also a new technique to estimate the guide field, implementing the reconstruction of magnetic potential of the in-plane magnetic field and relying on symmetric properties of magnetic reconnection.
AB - The present study is focused on the problem of reconstruction of the magnetic configuration in the magnetic reconnection electron diffusion region (EDR). The problem is addressed in the frame of electron magnetohydrodynamics with kept electron inertia term. We introduce the new reconstruction model independent of divergence of the electron pressure tensor and reconnection electric field. The model is tested on the magnetotail reconnection event of July 11, 2017 observed by the Magnetospheric Multiscale (MMS) spacecraft in the course of crossing the very core part of the reconnection region, the internal EDR. This new model demonstrates considerably better accuracy of the longitudinal electron velocity reconstruction due to the lower sensitivity to the configuration deviation from the two-dimensional time-independent model adopted in our study. We suggest also a new technique to estimate the guide field, implementing the reconstruction of magnetic potential of the in-plane magnetic field and relying on symmetric properties of magnetic reconnection.
KW - MAGNETIC RECONNECTION
KW - MAGNETOTAIL
KW - MAGNETOPAUSE
KW - SPACECRAFT
UR - http://www.scopus.com/inward/record.url?scp=85107039602&partnerID=8YFLogxK
UR - https://www.mendeley.com/catalogue/09ca3612-24fb-3218-a71b-29de0df7c6bf/
U2 - 10.1029/2020ja029045
DO - 10.1029/2020ja029045
M3 - Article
AN - SCOPUS:85107039602
VL - 126
JO - Journal of Geophysical Research: Space Physics
JF - Journal of Geophysical Research: Space Physics
SN - 2169-9380
IS - 5
M1 - e2020JA029045
ER -
ID: 84911293