A Model for U-Shaped Solar Burst Spectra,
Abstract
A model, for U-shaped solar bursts based on one single group of moderately relativistic electrons radiating in an ambient cold magnetoplasma is presented. Results of computer calculations are discussed. Suggestions for comparison with observation are made. Speculations about the mechanism of proton acceleration are included. (Author)
Document Details
- Document Type
- Technical Report
- Publication Date
- May 01, 1972
- Accession Number
- AD0747033
Entities
People
- Gabor Kalman
- Pradip Bakshi
- Stanford P. Yukon
Organizations
- Boston College