HAL (France)
open access
Energetic particles accelerated via turbulent magnetic reconnection in protoplanetary discs - I. Ionisation rates
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
- On Characteristics of the Fluctuation Concentration Field of the Diffusion of Matter from a Continuous Point Source in Grid Turbulence#22485
- Direct Four-Spacecraft Measurement of Reconnection Exhaust Thickness in the Solar Wind#925453
- Direct Four-Spacecraft Measurement of Reconnection Exhaust Thickness in the Solar Wind#921217
- Sea surface wakes observed by spaceborne SAR in the offshore wind farms#357005
- Probing into the aging dynamics of biomass burning aerosol by using satellite measurements of aerosol optical depth and carbon monoxide#142438
Record · ID 317474
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