arXiv (All)
open access
Kappa distributions in the framework of superstatistics
The kappa distribution of velocities appears routinely in the study of collisionless plasmas present in Earth's magnetosphere, the solar wind among other contexts where particles are unable to reach thermal equilibrium. Originally justified through the use of Tsallis' non-extensive statistics, nowad
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
- Investigating in the laboratory particle-magnetized plasma energy exchange processes relevant for astrophysics#1066184
- A Momentum-Regulated Model For Star Formation Efficiency in Giant Molecular Clouds#793771
- A Momentum-Regulated Model For Star Formation Efficiency in Giant Molecular Clouds#789766
- Coronal Mass Ejections from Young Suns: An Observational View through the Solar-Stellar Connection#1013876
- Molecules in the shadows of the protoplanetary disk HD 143006: Evidence for C/O $\gtrsim 1$ from simultaneously modeling fourteen ALMA lines#1062326
Record · ID 987450
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