arXiv (All)
open access
Divergence-free magnetohydrodynamics on a moving mesh
Magnetic fields are ubiquitous in the Universe and play an important role in many astrophysical processes, such as star formation and the evolution of galaxies. Hydrodynamical simulation methods that account for ideal magnetohydrodynamics (MHD) are however challenged by the need to achieve numerical
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
- PHASE: Multi-Regime Modeling of Incompressible Magnetohydrodynamics#1141924
- Magnetohydrodynamics of charged interstellar dust. Multifluid models and study of the linear modes#818766
- Magnetohydrodynamics of charged interstellar dust. Multifluid models and study of the linear modes#808774
- Phlegethon: a fully compressible magnetohydrodynamic code for simulations in stellar astrophysics#1129223
- Stellar streams for Galactic and cosmic archaeology#374399
Record · ID 1130831
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