DORAS
metadata only
Sulfur fractionation in coronal plumes as observed by Solar Orbiter/Spectral Imaging of the Coronal Environment
Coronal plumes are bright, narrow structures rooted in coronal holes that contribute to the solar wind. Their composition, particularly elemental fractionation as a function of first ionization potential (FIP), provides diagnostics of plasma properties and magnetic connectivity. Earlier plume studie
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
- R Coronae Borealis fadings: a dusty gas cloud eclipse model#1119430
- Promise and pitfalls of plasma emission as an exo-space-weather tool#1123323
- The Seasonal Sun.#333094
- Spectro-Polarimetric Observations of TeV Sources (SPOTS): first results#383757
- Conspicuous Gas, Cryptic Dust: Spectroscopy and Chromaticity of Complex Periodic Variables#819606
Record · ID 921700
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