It is known, that the short-wave radiation of the Sun in spectral range 0.1 - 200 nm represents one of key elements of solar-terrestrial relationship system, and its flux monitoring at orbit of the Earth allows to decide a whole series of fundamental and applied problems of physics of the Sun, upper atmosphere and ionosphere. In spite of the fact that nowadays the wide experience in satellite measurements of soft X-ray and extreme ultraviolet (EUV) radiation of the Sun has been accumulated, the gaps in realization of full permanent monitoring of this radiation still remain. So, in the operational space experiments: SOHO, TIMED and SORCE, - devices, which determining a spectral distribution and absolute values of fluxes of solar radiation (such as spectrometers and photometers), work in different spectral ranges. Besides this, TIMED and SORCE have not provided the permanent monitoring of the Sun, because the time of measurements are ~ 3 min and 60 min correspondingly from hour and a half orbits of these satellites. Moreover, SORCE instrumentation does not cover the main part of EUV radiation. Existed permanent measurements from full disk of the Sun by ionization chambers of GOES occur only in a narrow spectral interval 0.05 - 0.8 nm. One of the most perspective ways to realize this monitoring is the launch of "Space solar patrol" (SSP) instrumentation, produced by S.I. Vavilov State Optical Institute [1,2]. Thus, both at selection of a satellite for the SSP installation, and at processing of the measured data the cooperation with universities is possible and even desirable (so, for example, as variant for SSP launching is the small satellite "Mozhaets", developed by A.F. Mozhaiskii Military Space Academy) [1,2]. References: 1. Avakyan S.V., Afanas`ev I.M., Voronin N.A., et al. Space Solar Patrol and problems of Space Weather. // Opt. Zh. 73, No. 4, 10-17, 2006. [J. Opt. Technol. 73 (4), 2006]. 2. Afanas`ev I.M., Avakyan S.V., Kuvaldin E.V., et al. Achievements in creation of the Space patrol apparatus of ionizing radiation of the Sun. // Nuclear Inst. and Methods in Phys. Res., Section A, No. 543, 312-316, 2005.