HAL (France)
open access
Ly α Emissions from Titan’s Atmosphere and Exosphere
Abstract From 2004 to 2017, the Cassini/UVIS instrument observed Titan’s Ly α airglow from Titan’s atmosphere and exosphere, helping to characterize Titan’s H population. Most Ly α observations remain unanalyzed. Using data from the T10 Titan flyby, we analyze Ly α signal profiles from observations
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
- Current Status, Trends, and Future Directions in Chilean Air Quality: A Data-Driven Perspective#1225873
- Chang'e 7 Lunar Lander Optical Camera-Telescope: Optical Astronomy from the Moon#659354
- Chang'e 7 Lunar Lander Optical Camera-Telescope: Optical Astronomy from the Moon#657218
- A New Data Set to Keep a Sharper Eye on Land-Air Exchanges#614761
- Limb Asymmetries on WASP-39b: A Multi-GCM Comparison of Chemistry, Clouds, and Hazes#1296366
Record · ID 1449264
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