A possible link between turbulence and plasma heating
arXiv:2108.01376 · doi:10.3847/1538-4357/ac1942
Abstract
Numerical simulations and experimental results have shown that current sheets formation in space plasmas can be associated with enhanced vorticity. Also, in simulations the generation of such structures is associated with strong plasma heating. Here, we compare four-point measurements in the terrestrial magnetosheath turbulence from the Multiscale magnetospheric mission (MMS) of the flow vorticity and the magnetic field curlometer versus their corresponding one-point proxies PVI(V) and PVI(B) based on the Partial Variance of Increments (PVI) method. We show that the one-point proxies are sufficiently precise in identifying not only the generic features of the current sheets and vortices statistically, but also their appearance in groups associated with plasma heating. The method has been further applied to the region of the turbulent sheath of an interplanetary coronal mass ejection (ICME) observed at L1 by WIND spacecraft. We observe current sheets and vorticity associated heating in larger groups (blobs), which so far have not been considered in the literature on turbulent data analysis. The blobs represent extended spatial regions of activity with enhanced regional correlations between the occurrence of conditioned currents and vorticity, which at the same time are also correlated with enhanced temperatures. This heating mechanism is substantially different from the plasma heating in the vicinity of the ICME shock, where plasma beta is strongly fluctuating and there is no vorticity. The proposed method describes a new pathway for linking the plasma heating and plasma turbulence, and it is relevant to in-situ observations when only single spacecraft measurements are available.
arXiv comment21 pages, 7 figures
References in corpus (21)
- Evidence for Electron Landau Damping in Space Plasma Turbulence
- Energy transfer, pressure tensor and heating of kinetic plasma
- Intermittent Dissipation and Local Heating in the Solar Wind
- Electrons in the Young Solar Wind: First Results from the Parker Solar Probe
- Electron scale structures and magnetic reconnection signatures in the turbulent magnetosheath
- Alfven Wave Turbulence and Perpendicular Ion Temperatures in Coronal Holes
- Turbulence-driven ion beams in the magnetospheric Kelvin-Helmholtz instability
- Pressure anisotropy and small spatial scales induced by velocity shear
- The Complex Structure of Magnetic Field Discontinuities in the Turbulent Solar Wind
- Identification of Magnetic Flux Ropes from Parker Solar Probe Observations during the First Encounter
- Differential kinetic dynamics and heating of ions in the turbulent solar wind
- Whistler wave generation by halo electrons in the solar wind
- Turbulence Transport Modeling and First Orbit Parker Solar Probe (PSP) Observations
- Scale dependence of energy transfer in turbulent plasma
- On the statistical properties of turbulent energy transfer rate in the inner Heliosphere
- Velocity-Space Cascade in Magnetized Plasmas: Numerical Simulations
- Alternative high plasma beta regimes of electron heat-flux instabilities in the solar wind
- On the deviation from Maxwellian of the ion velocity distribution functions in the turbulent magnetosheath
- Turbulence-generated proton-scale structures in the terrestrial magnetosheath
- MMS Observations of Whistler and Lower Hybrid Drift Waves Associated with Magnetic Reconnection in the Turbulent Magnetosheath
- Nonlinear evolution of electron shear flow instabilities in the presence of an external guide magnetic field