This paper discusses the necessity for permanent monitoring of ionizing sol
ar radiation in a spectral range from 0.8 to 120 nm, which is most importan
t for geophysics. Such monitoring of the parameters of the solar activity i
s absent so far solely because of the methodological and technical complexi
ty of measurements in this spectral range at spacecraft. A description is g
iven of the entire set of equipment for such a space-based patrol comprisin
g a radiometer with foil, film, and crystal filters and two diffraction-gra
ting spectrometers of the grazing-beam and normal-incidence types. The set
of equipment allows absolute spectral measuring of the total radiation flux
from the solar disk in the x-ray and UV spectral regions from 0.14 to 153
nm. The results of the work on upgrading the set of space-based patrol equi
pment are presented. (C) 1998 The Optical Society of America. [S1070-9762(9
8)02012-0].