Processes setting the structure of the electron distribution function within the exhausts of anti-parallel reconnection
- Univ. of Wisconsin, Madison, WI (United States). Dept. of Physics
- Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
In situ spacecraft observations within the exhausts of magnetic reconnection document a large variation in the velocity space structure of the electron distribution function. Multiple mechanisms help govern the underlying electron dynamics, yielding a range of signatures for collisionless reconnection. These signatures include passing beams of electrons separated by well-defined boundaries from betatron heated/cooled trapped electrons. The present study emphasizes how localized regions of non-adiabatic electron dynamics can mix electrons across the trapped/passing boundaries and impact the form of the electron distributions in the full width of the exhaust. Here, while our study is based on 2D simulations, the described principles shaping the velocity space distributions also apply to 3D geometries making our findings relevant to spacecraft observation of reconnection in the Earth's magnetosphere.
- Research Organization:
- Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
- Sponsoring Organization:
- National Aeronautics and Space Administration (NASA); National Science Foundation (NSF); USDOE
- Grant/Contract Number:
- AC52-06NA25396; NNX14AC68G; NNX14AL38G
- OSTI ID:
- 1475335
- Report Number(s):
- LA-UR-17-27438
- Journal Information:
- Physics of Plasmas, Vol. 23, Issue 12; ISSN 1070-664X
- Publisher:
- American Institute of Physics (AIP)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
Web of Science
Energy transfer and electron energization in collisionless magnetic reconnection for different guide-field intensities
|
journal | December 2018 |
Inner and outer electron diffusion region of antiparallel collisionless reconnection: Density dependence
|
journal | October 2019 |
Energy transfer and electron energization in collisionless magnetic reconnection for different guide-field intensities | text | January 2018 |
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