Simulations of collisionless shocksA problem of critical importance to space and astrophysics is the existence and properties of high-Mach-number shocks. In this letter the results of simulations of perpendicular shocks with Alfven Mach number 22 are presented. It is shown that the shock structure is a sensitive function of resistivity, becoming turbulent when the resistivity is too low. The problem of electron heating, and the extension of the results to higher Mach numbers are discussed.
Document ID
19870024491
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Quest, K. B. (Los Alamos National Laboratory NM, United States)