Rankine-Hugoniot relations in turbulent shocks

A collisionless shock is often regarded as a discontinuity with a plasma flow across it. Plasma parameters before the shock (upstream) and behind the shock (downstream) are related by the Rankine-Hugoniot relations (RH) which essentially are the mass, momentum, and energy conservation laws. Standard...

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Main Author: Michael Gedalin
Format: Article
Language:English
Published: Frontiers Media S.A. 2023-12-01
Series:Frontiers in Physics
Subjects:
Online Access:https://www.frontiersin.org/articles/10.3389/fphy.2023.1325995/full
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author Michael Gedalin
author_facet Michael Gedalin
author_sort Michael Gedalin
collection DOAJ
description A collisionless shock is often regarded as a discontinuity with a plasma flow across it. Plasma parameters before the shock (upstream) and behind the shock (downstream) are related by the Rankine-Hugoniot relations (RH) which essentially are the mass, momentum, and energy conservation laws. Standard RH assume the upstream and downstream regions are uniform, that is, the fluctuations of the plasma parameters and magnetic field are negligible. Observations show that there exist shocks in which these fluctuations remain large well behind the shock. The pressure and energy of these fluctuations have to be included in the total pressure and energy. Here we lay down a basis of theory taking into account persisting non-negligible turbulence. The theory is applied to the case where only downstream magnetic turbulence is substantial. It is shown that the density and magnetic field compression ratios may significantly deviate from those predicted by the standard RH. Thus, turbulent effects should be taken into account in observational data analyses.
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spelling doaj.art-d7ce93fde366497c882b1cbdd3865fbe2023-12-20T08:38:29ZengFrontiers Media S.A.Frontiers in Physics2296-424X2023-12-011110.3389/fphy.2023.13259951325995Rankine-Hugoniot relations in turbulent shocksMichael GedalinA collisionless shock is often regarded as a discontinuity with a plasma flow across it. Plasma parameters before the shock (upstream) and behind the shock (downstream) are related by the Rankine-Hugoniot relations (RH) which essentially are the mass, momentum, and energy conservation laws. Standard RH assume the upstream and downstream regions are uniform, that is, the fluctuations of the plasma parameters and magnetic field are negligible. Observations show that there exist shocks in which these fluctuations remain large well behind the shock. The pressure and energy of these fluctuations have to be included in the total pressure and energy. Here we lay down a basis of theory taking into account persisting non-negligible turbulence. The theory is applied to the case where only downstream magnetic turbulence is substantial. It is shown that the density and magnetic field compression ratios may significantly deviate from those predicted by the standard RH. Thus, turbulent effects should be taken into account in observational data analyses.https://www.frontiersin.org/articles/10.3389/fphy.2023.1325995/fullcollisionless shocksplanetary bow shocksturbulenceparticle accelerationinterplanetary shock
spellingShingle Michael Gedalin
Rankine-Hugoniot relations in turbulent shocks
Frontiers in Physics
collisionless shocks
planetary bow shocks
turbulence
particle acceleration
interplanetary shock
title Rankine-Hugoniot relations in turbulent shocks
title_full Rankine-Hugoniot relations in turbulent shocks
title_fullStr Rankine-Hugoniot relations in turbulent shocks
title_full_unstemmed Rankine-Hugoniot relations in turbulent shocks
title_short Rankine-Hugoniot relations in turbulent shocks
title_sort rankine hugoniot relations in turbulent shocks
topic collisionless shocks
planetary bow shocks
turbulence
particle acceleration
interplanetary shock
url https://www.frontiersin.org/articles/10.3389/fphy.2023.1325995/full
work_keys_str_mv AT michaelgedalin rankinehugoniotrelationsinturbulentshocks