Accession Number : AD0637813
Title : AN INVESTIGATION OF THE X-RAY EMISSION OF SOLAR FLARES BY THE RADIO ASTRONOMICAL METHOD.
Corporate Author : SACRAMENTO PEAK OBSERVATORY SUNSPOT N MEX
Personal Author(s) : Neshpor,Y. I.
Report Date : 1966
Pagination or Media Count : 11
Abstract : 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)
Descriptors : (*SOLAR FLARES, *X RAYS), (*RADIO ASTRONOMY, X RAYS), COSMIC RAYS, EXTRATERRESTRIAL RADIO WAVES, ASTROPHYSICS, USSR
Subject Categories : Astrophysics
Nuclear Physics & Elementary Particle Physics
Distribution Statement : APPROVED FOR PUBLIC RELEASE