TY - JOUR
T1 - Fundamental Understanding of Magnetic Reconnection via Spiral CT Scan. VII. Energy Conversion
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 - 2026/6/20
Y1 - 2026/6/20
N2 - For the first time, we reveal the distribution of energy conversion (J · E′) around a reconnection X-line, by using the spiral CT scan technique, which is a novel technique analogous to that used in hospitals. This X-line was detected by the Magnetospheric Multiscale mission at the terrestrial magnetopause and has been widely believed to host a non-guide-field reconnection. With the help of such an advanced technique, we find that the energy conversion is strong near the X-point and in the magnetosphere-side inflow region, but is weak in the magnetosheath-side inflow region and at the separatrix. Such distribution is quite similar to the parallel-electric-field distribution, indicating that parallel electric fields may be responsible for the energy conversion. Surprisingly, the magnetic reconnection converts magnetic energy to particle energy in the inflow region (J · E′ > 0) but inversely converts particle energy to magnetic energy near the X-point (J · E′ < 0). This upends the conventional wisdom that magnetic reconnection only converts magnetic energy to particle energy. Quantitatively, we find that the net energy conversion by magnetic reconnection is (Binflow2 − Boutflow2)/2μ0.
AB - For the first time, we reveal the distribution of energy conversion (J · E′) around a reconnection X-line, by using the spiral CT scan technique, which is a novel technique analogous to that used in hospitals. This X-line was detected by the Magnetospheric Multiscale mission at the terrestrial magnetopause and has been widely believed to host a non-guide-field reconnection. With the help of such an advanced technique, we find that the energy conversion is strong near the X-point and in the magnetosphere-side inflow region, but is weak in the magnetosheath-side inflow region and at the separatrix. Such distribution is quite similar to the parallel-electric-field distribution, indicating that parallel electric fields may be responsible for the energy conversion. Surprisingly, the magnetic reconnection converts magnetic energy to particle energy in the inflow region (J · E′ > 0) but inversely converts particle energy to magnetic energy near the X-point (J · E′ < 0). This upends the conventional wisdom that magnetic reconnection only converts magnetic energy to particle energy. Quantitatively, we find that the net energy conversion by magnetic reconnection is (Binflow2 − Boutflow2)/2μ0.
KW - Plasma physics (2089)
KW - Solar magnetic reconnection (1504)
KW - Space plasmas (1544)
UR - https://www.scopus.com/pages/publications/105041664998
U2 - 10.3847/1538-4357/ae743b
DO - 10.3847/1538-4357/ae743b
M3 - 文章
AN - SCOPUS:105041664998
SN - 0004-637X
VL - 1004
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 2
M1 - 174
ER -