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V. N. Sidorenko M. B. Denisenko A. I. Igonin V. S. Tikunov 《Geography and Natural Resources》2011,32(3):205-212
We present the results derived from reconstructing, for the first time, the time series of some demographic indices of Russia’s
regions for the last 150 years. The problem posed for analysis was resolved through the use of extensive, officially published
statistical data sets as gathered by these authors at the microlevel (uyezds, and districts) and referred within the contemporary
boundaries of the subjects of the Russian Federation using economic-statistical methods and geoinformation technologies. 相似文献
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The main features of the transformation of organic matter (OM) in the greenschist, amphibolite, and granulite facies of metamorphism are considered based on the example of the Ukrainian crystal shield. The occurrence area and OM content in highly carbonaceous ancient rocks are characterized. The composition of primary sedimentary rocks and the processes of accumulation of biophile elements under the OM transformation are reconstructed. 相似文献
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A. I. Neishtadt D. J. Scheeres V. V. Sidorenko P. J. Stooke A. A. Vasiliev 《Celestial Mechanics and Dynamical Astronomy》2003,86(3):249-275
Reactive torques, due to anisotropic sublimation on a comet nucleus surface, produce slow variations of its rotation. In this paper the secular effects of this sublimation are studied. The general rotational equations of motion are averaged over unperturbed fast rotation around the mass center (Euler-Poinsot motion) and over the orbital comet motion. We discuss the parameters that define typical properties of the rotational evolution and discover different classifications of the rotational evolution. As an example we discuss some possible scenarios of rotational evolution for the nuclei of the comets Halley and Borrelly. 相似文献
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Krivtsov A. P. Rzhiga O. N. Sidorenko A. I. Sinilo V. P. Zakharov A. I. 《Earth, Moon, and Planets》1990,(1):533-537
Radar images of Venus' surface, obtained from the Venera 15 and 16 spacecraft and from the Earth, show many impact craters that are radar bright compared with their surroundings. It is demonstrated in this report that this phenomenon cannot be caused by higher surface roughness of meteorite impact area only. Obviously, enhanced reflectivity is required as well. It is supposed that the necessary enlargement of reflectivity might be caused by raised conductivity of surface material in the impact area, if the meteorite is related by chemical composition to iron or iron-stony types.'Geology and Tectonics of Venus', special issue edited by Alexander T. Basilevsky (USSR Acad. of Sci., Moscow), James W. Head (Brown University, Providence), Gordon H. Pettengill (MIT. Cambridge, Massachusetts) and R. S. Saunders (J.P.L., Pasadena). 相似文献
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Long-term premonitory seismicity patterns in Italy 总被引:1,自引:0,他引:1
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Vladislav V. Sidorenko Alessandra Celletti 《Celestial Mechanics and Dynamical Astronomy》2010,107(1-2):209-231
This paper is devoted to the dynamics in a central gravity field of two point masses connected by a massless tether (the so called “spring–mass” model of tethered satellite systems). Only the motions with straight strained tether are studied, while the case of “slack” tether is not considered. It is assumed that the distance between the point masses is substantially smaller than the distance between the system’s center of mass and the field center. This assumption allows us to treat the motion of the center of mass as an unperturbed Keplerian one, so to focus our study on attitude dynamics. A particular attention is given to the family of planar periodic motions in which the center of mass moves on an elliptic orbit, and the point masses never leave the orbital plane. If the eccentricity tends to zero, the corresponding family admits as a limit case the relative equilibrium in which the tether is elongated along the line joining the center of mass with the field center. We study the bifurcations and the stability of these planar periodic motions with respect to in-plane and out-of-plane perturbations. Our results show that the stable motions take place if the eccentricity of the orbit is sufficiently small. 相似文献
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Characteristics of the ocean state simulated with the Finite-Element Sea-Ice Ocean Model (FESOM) under the normalized year
forcing of Coordinated Ocean-ice Reference Experiments (COREs; Griffies et al., Ocean Model 26:1–46, 2009) are compared with those of other models participating in COREs. In contrast to these models, FESOM is run on an unstructured
mesh (with resolution varying between 20 and 150 km). It is shown that the ocean state simulated by FESOM is in most cases
within the spread of other models, demonstrating that the unstructured mesh technology has reached the stage when it becomes
a reliable tool for studying the large-scale ocean general circulation. 相似文献
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