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Autor:
Jago Edyvean, Tulasi N. Parashar, Tom Simpson, James Juno, Gian Luca Delzanno, Fan Guo, Oleksandr Koshkarov, William H Matthaeus, Michael Shay, Yan Yang
Publikováno v:
The Astrophysical Journal, Vol 972, Iss 2, p 173 (2024)
Understanding plasma turbulence requires a synthesis of experiments, observations, theory, and simulations. In the case of kinetic plasmas such as the solar wind, the lack of collisions renders the fluid closures such as viscosity meaningless and one
Externí odkaz:
https://doaj.org/article/76c986da482a449498f0e2c4f142a2bf