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dc.contributor.authorLapenta, G.
dc.contributor.authorBerchem, J.
dc.contributor.authorEl-Alaoui, M.
dc.contributor.authorWalker, R.
dc.contributor.authorAravindakshan, H.
dc.contributor.authorReisinger, N.
dc.contributor.authorPucci, F.
dc.contributor.authorArrò, G.
dc.contributor.authorBacchini, F.
dc.date2025
dc.date.accessioned2025-11-04T13:44:16Z
dc.date.available2025-11-04T13:44:16Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/14393
dc.descriptionWe present a method to visualize and analyze turbulence within macroscopic flows that feature complex structures not determined by the turbulence itself. We introduce a technique to shift to a Lagrangian frame that captures the macroscopic scales not part of the turbulent cascade. We then study turbulence within this frame that is comoving with the large-scale nonturbulent flow. The method is applied to Particle-in-Cell simulations of astrophysical plasma. Specifically, we use two cases to illustrate the new method. First, we consider a magnetic perturbation in the solar wind interacting with the bow shock, magnetosheath, and magnetopause in the dayside of the Earth. Second, we consider an Earthward flow generated by magnetic reconnection in the magnetotail. In these cases we show how the Lagrangian frame can be used to distinguish turbulent fluctuations from the macroscopic flow structures due to the evolution of the system caused by macroscopic forcing.
dc.languageeng
dc.titleA Lagrangian-frame technique for investigating plasma turbulence in complex underlying system-scale structures
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freeSpace plasma
dc.subject.freeLagrangian frame
dc.subject.freeKinetic modeling
dc.subject.freePlanetary magnetospheres
dc.source.titleFundamental Plasma Physics
dc.source.volume15
dc.source.pageA100099
Orfeo.peerreviewedYes
dc.identifier.doi10.1016/j.fpp.2025.100099
dc.identifier.url


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