AN INVESTIGATION OF THE X-RAY EMISSION OF SOLAR FLARES BY THE RADIO ASTRONOMICAL METHOD.
SACRAMENTO PEAK OBSERVATORY SUNSPOT N MEX
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The following conclusions are based on a study of the frequency dependence of the attenuation of cosmic radio noise during sudden ionospheric disturbances 1 The spectral distribution of the X-ray emission intensity of flares varies for each flare 2 some solar flares are characterized by an appreciable intensity increase of X-ray emission in the short-wave region 0.1-1 A. Author
- Nuclear Physics and Elementary Particle Physics