arXiv (All)
open access
A First Global Full-Vector Coronal Magnetic Field Inference Using MLSO CoMP and UCoMP Observations
Building on recent advances in coronal spectropolarimetry, seismology, and magnetic-field inferences of Z. Yang et al. (2024) and A. R. Paraschiv (2026), we present the first application of the CLEDB IQUD inversion methodology to Mauna Loa Solar Observatory CoMP and UCoMP observations. Using spectro
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
- Estudios teóricos sobre el espectro de líneas de la corona solar, II: (Continuación)#1089264
- Coronal Green-Line Emission During a Solar Prominence Eruption: Spectroscopic Evidence of Its Correspondence with the EUV Late Phase#1078235
- "Photon Aging" versus "Space Expansion": A Meta–Monist Re-reading of Cosmic Redshift#109577
- Models of the Transition Region between Chromosphere and Corona#284660
- Models of the Transition Region between Chromosphere and Corona#284612
Record · ID 1129701
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