TY - JOUR
T1 - Super-efficient Electron Acceleration by an Isolated Magnetic Reconnection
AU - Fu, H. S.
AU - Xu, Y.
AU - Vaivads, A.
AU - Khotyaintsev, Y. V.
N1 - Publisher Copyright:
© 2019. The American Astronomical Society. All rights reserved.
PY - 2019/1/10
Y1 - 2019/1/10
N2 - Magnetic reconnection - the process typically lasting for a few seconds in space - is able to accelerate electrons. However, the efficiency of the acceleration during such a short period is still a puzzle. Previous analyses, based on spacecraft measurements in the Earth's magnetotail, indicate that magnetic reconnection can enhance electron fluxes up to 100 times. This efficiency is very low, creating an impression that magnetic reconnection is not good at particle acceleration. By analyzing Cluster data, we report here a remarkable magnetic reconnection event during which electron fluxes are enhanced by 10,000 times. Such acceleration, 100 times more efficient than those in previous studies, is caused by the betatron mechanism. Both reconnection fronts and magnetic islands contribute to the acceleration, with the former being more prominent.
AB - Magnetic reconnection - the process typically lasting for a few seconds in space - is able to accelerate electrons. However, the efficiency of the acceleration during such a short period is still a puzzle. Previous analyses, based on spacecraft measurements in the Earth's magnetotail, indicate that magnetic reconnection can enhance electron fluxes up to 100 times. This efficiency is very low, creating an impression that magnetic reconnection is not good at particle acceleration. By analyzing Cluster data, we report here a remarkable magnetic reconnection event during which electron fluxes are enhanced by 10,000 times. Such acceleration, 100 times more efficient than those in previous studies, is caused by the betatron mechanism. Both reconnection fronts and magnetic islands contribute to the acceleration, with the former being more prominent.
KW - acceleration of particles
KW - magnetic reconnection
UR - https://www.scopus.com/pages/publications/85060198327
U2 - 10.3847/2041-8213/aafa75
DO - 10.3847/2041-8213/aafa75
M3 - 文章
AN - SCOPUS:85060198327
SN - 2041-8205
VL - 870
JO - Astrophysical Journal Letters
JF - Astrophysical Journal Letters
IS - 2
M1 - L22
ER -