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  5. Coexistence of Plasmoid and Kelvin-Helmholtz Instabilities in Collisionless Plasma Turbulence
 

Coexistence of Plasmoid and Kelvin-Helmholtz Instabilities in Collisionless Plasma Turbulence

Journal
THE ASTROPHYSICAL JOURNAL  
Date Issued
2022
Author(s)
BORGOGNO, Dario  
•
Grasso, Daniela
•
Achilli, Beatrice
•
Romé, Massimiliano
•
Comisso, Luca
DOI
10.3847/1538-4357/ac582f
Abstract
The plasmoid formation in collisionless plasmas, where magnetic reconnection within turbulence may take place driven by the electron inertia, is analyzed. We find a complex situation in which, due to the presence of strong velocity shears, the typical plasmoid formation, observed to influence the energy cascade in the magnetohydrodynamic context, has to coexist with the Kelvin-Helmholtz (KH) instability. We find that the current density layers may undergo the plasmoid or the KH instability depending on the local values of the magnetic and velocity fields. The competition among these instabilities affects not only the evolution of the current sheets, that may generate plasmoid chains or KH-driven vortices, but also the energy cascade, that is different for the magnetic and kinetic spectra.
Volume
929
Issue
1
Start page
62
Uri
http://hdl.handle.net/20.500.12386/36457
Url
https://iopscience.iop.org/article/10.3847/1538-4357/ac582f
https://api.elsevier.com/content/abstract/scopus_id/85128818550
Issn Identifier
0004-637X
Rights
open.access
File(s)
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Borgogno_2022_ApJ_929_62 (7).pdf

Description
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Size

1.76 MB

Format

Adobe PDF

Checksum (MD5)

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