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[en] So far it has not been possible to measure unambiguously the spectrum of impulsive X-rays < approximately 10 keV and hence to deduce a possible low energy cut-off in the energetic electron spectrum. The author reports briefly such an observation made with the ISEE-3 X-ray spectrometer experiment and its implications with regard to the characteristics of energetic electrons in solar flares. (Auth.)
Source
Dryer, M. (National Oceanic and Atmospheric Administration, Boulder, CO (USA). Space Environment Lab.); Tandberg-Hanssen, E. (National Aeronautics and Space Administration, Huntsville, AL (USA). George C. Marshall Space Flight Center) (eds.); International Council of Scientific Unions. Special Committee on Solar-Terrestrial Physics; Committee on Space Research. (COSPAR), 75-Paris (France); 577 p; ISBN 90-277-1163-1; 
; 1980; p. 227-230; D. Reidel; Dordrecht, Netherlands; International Astronomical Union symposium no. 91 on solar and interplanetary dynamics; Cambridge, MA, USA; 27 - 31 Aug 1979
; 1980; p. 227-230; D. Reidel; Dordrecht, Netherlands; International Astronomical Union symposium no. 91 on solar and interplanetary dynamics; Cambridge, MA, USA; 27 - 31 Aug 1979