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Astrophyzix.com is the publication of the Astrophyzix Digital Observatory, offering unpaywalled, evidence‑driven analysis and real‑time monitoring of PHAs and NEOs. Our tracking consoles and reporting systems use and provide access to official NASA CNEOS Scout, JPL CAD, NeoWs, JPL SBDB, Horizons and NOAA observational datasets, peer‑reviewed sources, and high‑precision numerical methods (IEEE‑754 Float64, RKN4). Designed for students, educators, researchers, and the public, every console is uniquely designed and engineered by the Astrophyzix Digital Observatory. Our research notes and papers can be found at Astrophyzix.Academia.Edu

Showing posts with label Peer Reviewed. Show all posts
Showing posts with label Peer Reviewed. Show all posts

Saturday, 7 February 2026

Solar Flares Explained: Magnetic Reconnection, Energy Release, and Effects on Earth and The Peer Reviewed Physics Behind Them

Written by: Astrophyzix Science Communication

Article type: Explainer, Evidence-Based

Solar flare physics

Introduction 

Solar flares are among the most energetic phenomena in the solar system, representing rapid and intense releases of magnetic energy from the Sun’s atmosphere. These events can heat plasma to tens of millions of kelvin, accelerate particles to relativistic speeds, and emit radiation across the entire electromagnetic spectrum. Although they occur on the Sun, solar flares can directly affect Earth’s space environment and modern technological systems.

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