arXiv (OAI Expanded)
open access
A self-consistent solar coronal heating model by Alfvenic waves
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
- A self-consistent solar coronal heating model by Alfvenic waves#612643
- Cascade models of anisotropic turbulence in magnetized plasma of solar wind#997302
- Sunspot fluctuations in two‐sector models: New results with additively separable preferences#284238
- A 22 yr Cycle of the Network Topology of Solar Active Regions#400835
- Solar Magnetic Configuration Control over Radiation Belt Electrons#792322
Record · ID 611166
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