TY - JOUR
T1 - Fundamental Understanding of Magnetic Reconnection via Spiral CT Scan. VI. Parallel Electric Field and Electron Acceleration
AU - Fu, H. S.
AU - Wang, Z.
AU - Cao, J. B.
N1 - Publisher Copyright:
© 2026. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the https://creativecommons.org/licenses/by/4.0/. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
PY - 2026/5/10
Y1 - 2026/5/10
N2 - For the first time, we reveal the distribution of parallel electric fields and suprathermal electrons around a reconnection X-line by using the spiral CT scan technique, which is a novel technique analogous to that in the hospital. This X-line was detected by the Magnetospheric Multiscale (MMS) mission at the magnetopause and has been widely believed to host an antiparallel reconnection without guide fields. With the help of such an advanced technique, we find that (1) suprathermal electrons exist mainly near the X-point and in the magnetosphere-side inflow region, but are sparse in the magnetosheath-side inflow region and near the separatrix; (2) parallel electric fields are strong near the X-point and in the magnetosphere-side inflow region, but are weak in the magnetosheath-side inflow region; (3) near the separatrix, electric fields are dominantly perpendicular rather than parallel; (4) both the enhancement of suprathermal electrons and parallel electric fields near the X-point are within a scale of 10 km (0.1 di); (5) the distribution of suprathermal electrons is different from the distribution of electron temperature, meaning that suprathermal electrons and thermal electrons have different behaviors near the reconnection site; (6) however, the distributions of suprathermal electrons and parallel electric fields are quite similar, indicating that the parallel electric fields may be responsible for suprathermal electron acceleration during reconnection. These results greatly improve our understanding of the electron acceleration during magnetic reconnection.
AB - For the first time, we reveal the distribution of parallel electric fields and suprathermal electrons around a reconnection X-line by using the spiral CT scan technique, which is a novel technique analogous to that in the hospital. This X-line was detected by the Magnetospheric Multiscale (MMS) mission at the magnetopause and has been widely believed to host an antiparallel reconnection without guide fields. With the help of such an advanced technique, we find that (1) suprathermal electrons exist mainly near the X-point and in the magnetosphere-side inflow region, but are sparse in the magnetosheath-side inflow region and near the separatrix; (2) parallel electric fields are strong near the X-point and in the magnetosphere-side inflow region, but are weak in the magnetosheath-side inflow region; (3) near the separatrix, electric fields are dominantly perpendicular rather than parallel; (4) both the enhancement of suprathermal electrons and parallel electric fields near the X-point are within a scale of 10 km (0.1 di); (5) the distribution of suprathermal electrons is different from the distribution of electron temperature, meaning that suprathermal electrons and thermal electrons have different behaviors near the reconnection site; (6) however, the distributions of suprathermal electrons and parallel electric fields are quite similar, indicating that the parallel electric fields may be responsible for suprathermal electron acceleration during reconnection. These results greatly improve our understanding of the electron acceleration during magnetic reconnection.
KW - Plasma physics (2089)
KW - Solar magnetic reconnection (1504)
KW - Space plasmas (1544)
UR - https://www.scopus.com/pages/publications/105037980360
U2 - 10.3847/1538-4357/ae5e63
DO - 10.3847/1538-4357/ae5e63
M3 - 文章
AN - SCOPUS:105037980360
SN - 0004-637X
VL - 1002
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 2
ER -