In-situ evidence of electron energization in the electron diffusion region of magnetotail reconnection
arXiv:1602.08482 · doi:10.1002/2015JA022040
Abstract
Magnetic reconnection is an explosive energy-release process in laboratory, space and astrophysical plasmas. While magnetic fields can `break' and `reconnect' in a very small region called the electron diffusion region (EDR), there have been conflicting theories as to whether this region can be a place of rapid energization of plasmas. Here we report a fortuitous encounter of the EDR by THEMIS in the Earth's magnetotail where significant heating and demagnetization of electrons were observed. Additional energization was observed on both sides (immediate upstream and downstream) of the EDR, leading to a total of more than an order of magnitude energization across this region. The results demonstrate that, despite its minuscule size, the EDR does indeed contribute to the overall process of electron energization via magnetic reconnection.
arXiv comment10 pages, 7 figures; accepted by Journal of Geophysical Research
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Cited by in corpus (5)
- Electron-Scale Dynamics of the Diffusion Region during Symmetric Magnetic Reconnection in Space
- Electron Power-Law Spectra in Solar and Space Plasmas
- The Acceleration of Charged Particles and Formation of Power-law Energy Spectra in Nonrelativistic Magnetic Reconnection
- Particle dynamics in the electron current layer in collisionless magnetic reconnection
- Using the maximum entropy distribution to describe electrons in reconnecting current sheets