arXiv (All)
open access
Effects of Synchrotron Self-Absorption on Polarization Diagnostics of MHD Turbulence
Synchrotron polarization is a powerful tool for diagnosing magnetohydrodynamic (MHD) turbulence, yet prior analyses are confined to the optically thin regime, neglecting the effects of synchrotron self-absorption (SSA). Here, we incorporate SSA into the radiative transfer of polarized synchrotron em
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
- Stellar flare detection and characterization in ZTF High-cadence light curves#1050515
- Effective-frequency shear organizes chaotic response under higher-order coupling#1198899
- Genesis and evolution of velocity gradients in near-field spatially developing turbulence#1311587
- Post-merger rotational evolution of magnetised single hot subdwarfs results in slow rotation due to magnetic braking#1354360
- Joint Line Intensity Recovery from Multi-Tracer Cross-Correlations#1355387
Record · ID 1456519
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