TL;DR
This paper reviews the current state of magnetohydrodynamic (MHD) turbulence research, including theoretical models, numerical simulations, and applications to astrophysics and solar science, highlighting recent advances and methodologies.
Contribution
It provides a comprehensive overview of MHD turbulence theories, numerical methods, and their applications, integrating recent developments in Alfvenic turbulence, dynamos, and supersonic regimes.
Findings
Summarizes key turbulence models and wave modes.
Discusses numerical techniques for MHD turbulence.
Highlights applications in astrophysics and solar science.
Abstract
We review the current status of research in MHD turbulence theory and numerical experiments and their applications to astrophysics and solar science. We introduce general tools for studying turbulence, basic turbulence models, MHD equations and their wave modes. Subsequently, we cover the theories and numerics of Alfvenic turbulence, imbalanced turbulence, small-scale dynamos and models and numerics for supersonic MHD turbulence.
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