Abstract
In Innocenti et al. (2015) we have observed and characterized for the first time Petschek-like switch-off slow shock/rotational discontinuity (SO-SS/RD) compound structures in a 2-D fully kinetic simulation of collisionless magnetic reconnection. Observing these structures in the solar wind or in the magnetotail would corroborate the possibility that Petschek exhausts develop in collisionless media as a result of single X point collisionless reconnection. Here we highlight their signatures in simulations with the aim of easing their identification in observations. The most notable signatures include a four-peaked ion current profile in the out-of-plane direction, associated ion distribution functions, increased electron and ion anisotropy downstream the SS, and increased electron agyrotropy downstream the RDs.
| Original language | English |
|---|---|
| Pages (from-to) | 3447-3455 |
| Number of pages | 9 |
| Journal | Geophysical Research Letters |
| Volume | 44 |
| Issue number | 8 |
| DOIs | |
| Publication status | Published - 28 Apr 2017 |
| Externally published | Yes |
Keywords
- Hall reconnection
- Petschek exhaust
- anisotropy and agyrotropy
- ion distribution functions
- magnetic reconnection
- slow shock/rotational discontinuity
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