A hybrid gyrokinetic ion and isothermal electron fluid code for astrophysical plasma
This paper describes a new code for simulating astrophysical plasmas that solves a hybrid model composed of gyrokinetic ions (GKI) and an isothermal electron fluid (ITEF) [A. Schekochihin et al., Astrophys. J. Suppl. \textbf{182}, 310 (2009)]. This model captures ion kinetic effects that are importa...
主要な著者: | Kawazura, Y, Barnes, M |
---|---|
フォーマット: | Journal article |
出版事項: |
Elsevier
2018
|
類似資料
-
Ion versus electron heating in compressively driven astrophysical gyrokinetic turbulence
著者:: Kawazura, Y, 等
出版事項: (2020) -
Ion versus Electron Heating in Compressively Driven Astrophysical Gyrokinetic Turbulence
著者:: Y. Kawazura, 等
出版事項: (2020-12-01) -
AstroGK: Astrophysical gyrokinetics code
著者:: Numata, R, 等
出版事項: (2010) -
Astrophysical gyrokinetics: turbulence in pressure-anisotropic plasmas at ion scales and beyond
著者:: Kunz, MW, 等
出版事項: (2018) -
Astrophysical gyrokinetics: kinetic and fluid turbulent cascades in
magnetized weakly collisional plasmas
著者:: Schekochihin, A, 等
出版事項: (2007)