Comparing turbulence in a Kelvin–Helmholtz instability region across the terrestrial magnetopause

Autor: Federico Fraternale, Paulina Quijia, C. L. Vásconez, Emiliya Yordanova, Silvia Perri, Raffaele Marino, Luca Sorriso-Valvo, Julia E. Stawarz

Publikováno v: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 503 (4), pp.4815-4827. ⟨10.1093/MNRAS/STAB319⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 503 (4), pp.4815-4827. ⟨10.1093/mnras/stab319⟩
Monthly notices of the Royal Astronomical Society (Online) 503 (2021): 4815–4827. doi:10.1093/mnras/stab319
info:cnr-pdr/source/autori:Quijia, P.; Fraternale, F.; Stawarz, J.E.; Vasconez, C.L.; Perri, S.; Marino, R.; Yordanova, E.; Sorriso-Valvo, L./titolo:Comparing turbulence in a Kelvin-Helmholtz instability region across the terrestrial magnetopause/doi:10.1093%2Fmnras%2Fstab319/rivista:Monthly notices of the Royal Astronomical Society (Online)/anno:2021/pagina_da:4815/pagina_a:4827/intervallo_pagine:4815–4827/volume:503

The properties of turbulence observed within the plasma originating from the magnetosheath and the magnetospheric boundary layer, which have been entrained within vortices driven by the Kelvin–Helmholtz Instability (KHI), are compared. The goal of

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4a74064e9e7064d3c19bf1d62049b7f1
https://doi.org/10.1093/mnras/stab319