arXiv (OAI Expanded)
open access
Triple coronal hard X-ray source observed by STIX during a failed filament eruption
{Observations reveal hard X-ray sources in the solar corona with morphologies and locations distinct from typical solar flares. One expected mechanisms for hard X-ray (HXR) production in the solar corona is eruptions of various types. Failed eruptions are promising targets for detecting non-flare-re
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
- Cycle Variation in the Occurrence of Great Soft X-ray Solar Flares#987183
- A high-frequency type II radio burst associated with an X2.3 class flare#792382
- A high-frequency type II radio burst associated with an X2.3 class flare#788382
- The analysis and the three-dimensional, forward-fit modeling of the hard x-ray and the microwave emissions of major solar flares#641337
- Dual Signatures of Bursty Star Formation in High-Redshift UV Luminosity Functions#1037114
Record · ID 1122854
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