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711.
A. S. Meshchanov 《Russian Aeronautics (Iz VUZ)》2008,51(3):259-268
A system of differential equations for the angular motion of an observation satellite (OS) equipped with an inertial drive electromagnetic device (EMD) without a controlling flywheel engine is presented. Apart from lag, the calculated and uncertain limited external and parametric disturbances constantly acting on the OS control system are taken into account. It is proposed that the sliding conditions be used to obtain the high-precision OS control with the specified direct indices of the transient process quality in the angular motion. A problem of equivalent system transformation is solved to safely provide the invariance of the sliding conditions to all listed disturbances with respect to the Euler angles and their first and second derivatives. 相似文献
712.
The results of experimental and numerical studies of natural frequencies and vibration modes of a centrally secured circular plate of constant thickness are presented. The studies are carried our using the interference holography and finite element methods and the results are considered as guiding lines for determining vibration characteristics of real disks. 相似文献
713.
I. Büsching O.C. de Jager 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
In this study, we investigate how restrictive the γ-ray emission from the Galactic center region, as seen by HESS and other Cherenkov air shower arrays, is against various models for cosmic ray injection. We derive diffusion coefficients which fit the observed spatial scales of diffuse γ-ray emission from the extended emission associated with the molecular clouds SgrA, B and C. Using these diffusion coefficients, we then obtain a limit for time scale of assumed recent proton acceleration near the SMBH, as the spatial size of SgrA∗ in VHE γ-rays has to be consistent with the observed unresolved HESS point source size at this position. The signal from this hadronic component may be mixed with the expected VHE inverse Compton emission from the nearby unresolved pulsar wind nebula. 相似文献
714.
I. Yoshikawa S. Kameda K. Hikosaka G. Murakami D. Rees H. Nozawa S. Okano O. Korablev 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
The Mercury’s Sodium Atmosphere Spectral Imager (MSASI) on BepiColombo (BC) will address a range of fundamental scientific questions pertaining to Mercury’s exosphere. The measurements will provide new information on regolith–exosphere–magnetosphere coupling as well as new understanding of the dynamics governing the exosphere bounded by the planetary surface, the solar wind and interplanetary space. MSASI is a high-dispersion visible spectrometer working in the spectral range around sodium D2 emission (589 nm). A tandem Fabry–Perot etalon is used to achieve a compact design. We presents a design of the spectral analyzer using Fabry–Perot interferometer. We conclude that: (1) The MSASI optical design is practical and can be implemented without new or critical technology developments; (2) The thermally-tuned etalon design is based on concepts, designs and materials that have good space heritage. 相似文献
715.
I. Sh. Sharafeev 《Russian Aeronautics (Iz VUZ)》2008,51(1):105-108
Structures of models for computer-aided calculation of cutting conditions and time standards for the NORMA computer-aided design system of labor standards (CADS LS) are described. 相似文献
716.
The paper presents the study of turbulent properties of the solar wind plasma, namely, the intermittency of fluctuations of the solar wind ion flux in the earlier unexplored region of comparatively high frequencies (0.01–1 Hz). Special attention is given to a comparison of intermittency for solar wind observation intervals containing sharp (shorter than 10 min) and high-amplitude (greater than 20%) changes of the ion flux to intervals without such changes. The solar wind observation intervals containing sharp changes of the flux are found to be essentially more intermittent than the intervals of quiet solar wind. Such a comparison allows one to reveal the fundamental difference in turbulent properties of the solar wind depending on the presence or absence of sharp boundaries in plasma structures. 相似文献
717.
K.S. Cheng D.O. Chernyshov V. Dogiel 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
X-ray observations indicate that the Galactic black hole Sgr A∗ is inactive now, however, we suggest that Sgr A∗ can become active when a captured star is tidally disrupted and matter is accreted into the black hole. Consequently the Galactic black hole could be a powerful source of relativistic protons with a characteristic energy ∼1052 erg per capture. The diffuse GeV and TeV γ-rays emitted in the direction of the Galactic Center (GC) are the direct consequences of p–p collisions of such relativistic protons ejected by very recent capture events occurred ?105 yr ago. On the other hand, the extended electron-positron annihilation line emission observed from GC is a phenomenon related to a large population of thermalized positrons, which are produced, cooled down and accumulated through hundreds of past capture events during a period of ∼107 yr. In addition to explaining GeV, TeV and 511 keV annihilation emissions we also estimate the photon flux of several MeV resulting from in-flight annihilation process. 相似文献
718.
M. M. Ganiev 《Russian Aeronautics (Iz VUZ)》2008,51(2):223-225
The results of experimental studies concerning the physico-mechanical properties of adhesive joints and epoxide compound-based coatings after ultrasonic machining are presented. Also considered is a change of adhesive strength and residual stresses in different “metal — polymer” systems. 相似文献
719.
A. G. Sattarov 《Russian Aeronautics (Iz VUZ)》2008,51(2):166-172
A method and results of calculating the laser radiation power values necessary to place an artificial earth satellite in orbit are presented; the values depend on the initial vehicle mass, velocity of the working fluid efflux from the laser rocket engine nozzle, velocity of vehicle motion, optimal values of thrust-to-weight ratio taking into account irreversible energy losses in the rocket engine jet. The possibility of creating a spacecraft with small initial mass is substantiated. A layout scheme of the propulsive system is proposed that makes it possible to divide total laser radiation power and to use atmospheric air as a working fluid. 相似文献
720.
D. P. Sharma R. K. Sood G. Stringfellow S. D. James K. M. Hill R. K. Manchanda 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1993,13(12):375-378
The galactic X-ray source GX 1+4 has been undergoing remarkable changes since early 1991. The X-ray pulsar has shown fast spin down accompanied by an increase in the hard X-ray intensity. We have obtained 1.6Å resolution spectra of the optical counterpart extending the known spectrum to 8500Å. The Ca II (8498Å) line seen for the first time from this source is indicative of a nova burst scenario. Other lines detected for the first time are detailed and the significance of these features is discussed. 相似文献