A Model for the Solar Flare,
Abstract
It is suggested that many solar flares occur due to an interaction between newly emerging magnetic flux and an active region filament. A current sheet forms between the new and old flux and, when its electric current density exceeds a critical value, rapid magnetic fields reconnection takes place. Electrons are then accelerated to high energies and follow the magnetic field lines down to the chromosphere where they produce several (typically three) bright H alpha knots. Magnetic energy is continuously released as reconnected prominence fields are allowed to untwist. Two ribbons of H alpha emission are produced by one or more of three mechanisms: energetic particles, thermal conduction or shocks due to infalling material.
Document Details
- Document Type
- Technical Report
- Publication Date
- Jul 10, 1975
- Accession Number
- ADA013776
Entities
People
- D. M. Rust
- E. R. Priest
- R. C. Canfield
Organizations
- Air Force Cambridge Research Laboratories