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In article the opportunity of use strapdown inertial navigation system (SINS) on the base of fiber-optic gyroscopes and quartz accelerometers corrected from star sensors and satellite navigation equipment (SNE) for perspective interplanetary spacecrafts motion control on phases of interplanetary trajectory insertion, trajectory correction, and braking during transition to Mars orbit is investigated. Results of onboard control complex accuracy characteristics estimation are presented at the given dynamic spacecraft scheme which is taking into account the liquid oscillations in tanks and structure elements elasticity. At modelling the errors of measuring devices installation, errors of SINS initial alignment and instrumental errors of SINS sensitive elements, variation of control engines parameters were taken into account. The structure of the developed complex of imitation modelling of interplanetary spacecraft controlled motion is resulted. Estimations of active flight legs realization accuracy were received by a method of statistical modelling of spacecraft controlled motion  相似文献   
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A number of exact solutions of a problem on heat exchange in channels under unsteady conditions at the low Biot numbers and sufficiently low Brune numbers with and without consideration for a heat carrier stay period in a pipeline are obtained.  相似文献   
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Within the framework of the concept of steady-state flow of a flux of dust particles through the cusp channel of the Earth's magnetosphere, we develop the idea that the magnetic cusp is a generator of dust swarms in the near-Earth space. The analytical dependencies for the density (concentration) of dust particles in the cusp and near-Earth space region are obtained.  相似文献   
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The analytical solution of a nonlinear nonstationary inverse problem of heat conduction for a bodies with low heat conduction coefficients of one-dimensional geometry is presented. The solutions obtained make it possible to restore the boundary conditions rather exactly using the results of heat flux measurements.  相似文献   
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Lobanov  A. B.  Pavlichenko  E. A. 《Cosmic Research》2003,41(6):567-573
The results of numerical modeling of dust plasma dynamics in the geomagnetic tail are presented for the southward and northward orientations of the interplanetary magnetic field in the model with reconnection of magnetic field lines of geomagnetic and interplanetary magnetic fields. It is shown that in reconnection regions the compression shock waves arise, at the fronts of which the dust plasma fluxes with higher-than-background density are generated.  相似文献   
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A possibility of attaining steady flow of detonation products with specific energy much larger than the specific chemical energy of explosive is demonstrated in the case when a cylindrical charge of explosive is fitted with an evacuated cavity. Simple estimates and results of numerical analysis of the process are presented. Steady process may be considered to occur under the following assumptions: (1) effects arising due to jet interaction with cavity walls are negligible; (2) the detonation process is steady. In the case of limited explosive lengths these assumptions have been shown to be correct.When the cavity is filled with gas or liquid, a variety of steady and non-steady flow regimes is possible, depending on the density of the filling medium. One well-known case is that of flow with irregular reflection of shock waves at the cavity axis accompanied with the formation of Mach intersections. Another interesting flow regime is observed to occur in the case of low density filling medium (liquid hydrogen, for example). In this case the filling medium is driven by a “detonation piston” at constant velocity, equal to the velocity of detonation, forming a uniform growing column of hot shock-compressed matter, specific energy of which exceeds by one order of magnitude the specific energy of the explosive. Obviously, the walls of the vessel containing hydrogen must be able to withstand radial loads for a sufficiently long time (20 μ sec).The relative merits of these methods in comparison to others in high speed gas-dynamics is discussed.  相似文献   
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We present the results of the mathematical modeling based on the multiunit computational technologies of the vortex zone structure between periodic flow rectangular cross-section turbulators placed on the surface. We used the factorized finite-volume method for solving the Reynolds equations, being closed with the use of Menter’s shear stress transfer model, and the energy equation on different-scale intersecting structured grids. The detailed analysis of the corresponding streamlines is presented.  相似文献   
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