Astrophysical gyrokinetics: Basic equations and linear theory
Magnetohydrodynamic (MHD) turbulence is encountered in a wide variety of astrophysical plasmas, including accretion disks, the solar wind, and the interstellar and intracluster medium. On small scales, this turbulence is often expected to consist of highly anisotropic fluctuations with frequencies s...
| Egile Nagusiak: | , , , , , |
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| Formatua: | Journal article |
| Hizkuntza: | English |
| Argitaratua: |
2006
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