Supermagnetosonic jets behind a collisionless quasi-parallel shock
H. Hietala (1), T. V. Laitinen (2), K. Andr\'eeov\'a (3), R. Vainio, (1), A. Vaivads (2), M. Palmroth (3), T. I. Pulkkinen (3), H. E. J. Koskinen, (1, 3), E. A. Lucek (4), H. R\`eme (5, 6) ((1) Department of, Physics, University of Helsinki, Helsinki, Finland

TL;DR
This paper reports on the discovery and analysis of supermagnetosonic jets behind collisionless quasi-parallel shocks, revealing a new generation mechanism involving shock curvature and secondary shock formation, with implications for plasma environments.
Contribution
It introduces a novel generation mechanism for supermagnetosonic jets in collisionless shocks based on spacecraft observations and shock curvature effects.
Findings
Identification of supermagnetosonic jets in the downstream region.
Detection of a secondary shock front within the sheath.
Proposed mechanism linking shock curvature to jet formation.
Abstract
The downstream region of a collisionless quasi-parallel shock is structured containing bulk flows with high kinetic energy density from a previously unidentified source. We present Cluster multi-spacecraft measurements of this type of supermagnetosonic jet as well as of a weak secondary shock front within the sheath, that allow us to propose the following generation mechanism for the jets: The local curvature variations inherent to quasi-parallel shocks can create fast, deflected jets accompanied by density variations in the downstream region. If the speed of the jet is super(magneto)sonic in the reference frame of the obstacle, a second shock front forms in the sheath closer to the obstacle. Our results can be applied to collisionless quasi-parallel shocks in many plasma environments.
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