ON THE HARD X-RAY EMISSION OF SOLAR FLARES.
SACRAMENTO PEAK OBSERVATORY SUNSPOT N MEX
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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
- Nuclear Physics and Elementary Particle Physics