ON THE HARD X-RAY EMISSION OF SOLAR FLARES.
Abstract
A method is proposed for the determination of the effective wavelength lambda sub eff of the X-ray emission of chromospheric flares at the moment of maximum of an SID. The method is based on the utilization of data on the f sub m in reflection frequencies, obtained from World Data Center Ionospheric Stations, and is used for determining the lambda sub eff of seven flares. The derived values are within the limits 2-3 A. (Author)
Document Details
- Document Type
- Technical Report
- Publication Date
- Jan 01, 1966
- Accession Number
- AD0637811
Entities
People
- L. S. Levitsky