Citation

BibTex format

@article{Adhikari:2021:10.1103/PhysRevE.104.065206,
author = {Adhikari, S and Parashar, TN and Shay, MA and Matthaeus, WH and Pyakurel, PS and Fordin, S and Stawarz, JE and Eastwood, JP},
doi = {10.1103/PhysRevE.104.065206},
journal = {Physical Review E: Statistical, Nonlinear, and Soft Matter Physics},
title = {Energy transfer in reconnection and turbulence},
url = {http://dx.doi.org/10.1103/PhysRevE.104.065206},
volume = {104},
year = {2021}
}

RIS format (EndNote, RefMan)

TY  - JOUR
AB - Reconnection and turbulence are two of the most commonly observed dynamical processes in plasmas, but their relationship is still not fully understood. Using 2.5D kinetic particle-in-cell simulations of both strong turbulence and reconnection, we compare the cross-scale transfer of energy in the two systems by analyzing the generalization of the von Kármán Howarth equations for Hall magnetohydrodynamics, a formulation that subsumes the third-order law for steady energy transfer rates. Even though the large scale features are quite different, the finding is that the decomposition of the energy transfer is structurally very similar in the two cases. In the reconnection case, the time evolution of the energy transfer also exhibits a correlation with the reconnection rate. These results provide explicit evidence that reconnection dynamics fundamentally involves turbulence-like energy transfer.
AU - Adhikari,S
AU - Parashar,TN
AU - Shay,MA
AU - Matthaeus,WH
AU - Pyakurel,PS
AU - Fordin,S
AU - Stawarz,JE
AU - Eastwood,JP
DO - 10.1103/PhysRevE.104.065206
PY - 2021///
SN - 1539-3755
TI - Energy transfer in reconnection and turbulence
T2 - Physical Review E: Statistical, Nonlinear, and Soft Matter Physics
UR - http://dx.doi.org/10.1103/PhysRevE.104.065206
UR - http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000753842400003&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=1ba7043ffcc86c417c072aa74d649202
UR - https://journals.aps.org/pre/abstract/10.1103/PhysRevE.104.065206
UR - http://hdl.handle.net/10044/1/95457
VL - 104
ER -