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pro vyhledávání: '"Yauheni Huliuta"'
Publikováno v:
The Astrophysical Journal, Vol 970, Iss 1, p 3 (2024)
The dispersion relation of the magnetized Kelvin–Helmholtz (KH) instability driven by shear flow with zero thickness of the shear layer is derived theoretically based on a set of magnetohydrodynamic equations in the presence of a transverse magneti
Externí odkaz:
https://doaj.org/article/ba8b9f43649a4dc3bb94a6ee59d2f73d