Accession Number : AD0637811
Title : ON THE HARD X-RAY EMISSION OF SOLAR FLARES.
Corporate Author : SACRAMENTO PEAK OBSERVATORY SUNSPOT N MEX
Personal Author(s) : Levitsky,L. S.
Report Date : 1966
Pagination or Media Count : 9
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)
Descriptors : (*SOLAR FLARES, *X RAYS), SOLAR DISTURBANCES, IONOSPHERIC DISTURBANCES, ATMOSPHERES, X RAY SPECTROSCOPY, USSR
Subject Categories : Astrophysics
Nuclear Physics & Elementary Particle Physics
Distribution Statement : APPROVED FOR PUBLIC RELEASE