arXiv (All)
open access
Apparent magnetic field decay in a solar flare from Zeeman splitting of the Mg 12.32 microns observations
The magnetic field is the most fundamental observable in solar physics, while solar flares are the most violent, rapid magnetic energy-release events in the solar atmosphere. Decades of observations and theory have sketched the framework of flare evolution and magnetic-field-related physical process
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
- The Gannon Storm: Citizen science observations during the geomagnetic superstorm of 10 May 2024#1354611
- Investigating the inferred spatiotemporal evolution of magnetic fields during an X1-class flare#1033900
- Coherent radio bursts, polarity reversal, and quiescent emission from the M4V dwarf WW PsA#1202374
- The "Other" Centuries-Long Record of Solar Magnetic Activity Cycles: Lessons From the Stars#1037156
- Stellar flare detection and characterization in ZTF High-cadence light curves#1050515
Record · ID 1455983
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