Space Sci Rev (2018) 214:81 https://doi.org/10.1007/s11214-018-0516-3 Jets Downstream of Collisionless Shocks Ferdinand Plaschke1,2 · Heli Hietala3 · Martin Archer4 · Xóchitl Blanco-Cano5 · Primož Kajdicˇ5 · Tomas Karlsson6 · Sun Hee Lee7 · Nojan Omidi8 · Minna Palmroth9,10 · Vadim Roytershteyn11 · Daniel Schmid12 · Victor Sergeev13 · David Sibeck7 Received: 19 December 2017 / Accepted: 2 June 2018 / Published online: 21 June 2018 © The Author(s) 2018 Abstract The magnetosheath flow may take the form of large amplitude, yet spatially local- ized, transient increases in dynamic pressure, known as “magnetosheath jets” or “plasmoids” among other denominations. Here, we describe the present state of knowledge with respect to such jets, which are a very common phenomenon downstream of the quasi-parallel bow shock. We discuss their properties as determined by satellite observations (based on both case and statistical studies), their occurrence, their relation to solar wind and foreshock con- ditions, and their interaction with and impact on the magnetosphere. As carriers of plasma and corresponding momentum, energy, and magnetic flux, jets bear some similarities to bursty bulk flows, which they are compared to. Based on our knowledge of jets in the near Earth environment, we discuss the expectations for jets occurring in other planetary and B F. Plaschke
[email protected] 1 Space Research Institute, Austrian Academy of Sciences, Graz, Austria 2 Present address: Institute of Physics, University of Graz, Graz, Austria 3 Department of