arXiv (All)
open access
Hall-MHD in driven turbulence FLASH simulations
The origin of magnetic fields in turbulent astrophysical systems has long been a central problem in plasma astrophysics. Fluctuation dynamos are a class of field amplification mechanisms that occur in turbulent magnetohydrodynamics whereby stochastically forced motions of plasma at sufficiently high
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- The role of different nonlinearities and potential vorticity conservation in two-dimensional fluid ITG models#821349
- Effects of Alfvénicity on the Compressible Energy Cascade in Magnetohydrodynamic Solar Wind Turbulence: Evidence from Parker Solar Probe, Solar Orbiter, and WIND observations#1142164
- Turbulent wall-bounded flow of weakly shear-thinning fluid: Phenomenological modeling of eddy viscosity and law of the wall#354141
- The driving mode of turbulence in disc galaxy simulations with adaptive mesh refinement#1084935
- Why MHD turbulence forms sheets: energy conversion and cascade geometry#1051900
Record · ID 925545
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive