Solar physics
Magnetic Reconnection
The process by which oppositely directed magnetic field lines break and reconnect, converting stored magnetic energy explosively into heat, light, and fast particles. Reconnection powers solar flares and helps launch coronal mass ejections, and is a fundamental plasma process seen throughout the Universe.
Highlights
- ›Releases magnetic energy — the engine of solar flares
The Sun, its layers & phenomena
Across solar physics
Knowledge connections
- Associated withThe Sun
- Associated withThe Solar Corona
- Associated withSolar Flare
- Associated withCoronal Mass Ejection (CME)
- Associated withNanoflare Heating
Sources
The primary and reference sources this topic draws on.
- NASANational Aeronautics and Space Administration
Mission data, planetary science, space telescopes, and public-domain imagery.
Most NASA-produced imagery is in the public domain; individual items are checked for usage terms before publication.