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11.
Aleksey Marchenko Nicolai Vasiliev Artem Nesterov Yuri Kondrashov Nikolay Belyaev 《寒旱区科学》2017,9(3):192-196
Measurements of the thermal deformations of frozen soil samples were performed in the cold laboratory in temperature range from 0°C to-12°C.Fiber Bragg Gratings strain and temperature sensors were used to measure the deformation and temperature inside the samples.A number of tests with the samples prepared from Kaolin and Cambrian clay saturated with fresh water,and prepared from fine and silt sand saturated with fresh or saline water,are performed.Thermal deformations of the samples are analyzed depending on the cyclic changes of their temperature. 相似文献
12.
Jin Huijun Jin Xiaoying He Ruixia Luo Dongliang Chang Xiaoli Wang Shaoling Marchenko Sergey S Yang Sizhong Yi Chaolu Li Shijie Harris Stuart A 《中国科学:地球科学(英文版)》2019,62(8):1207-1223
The formation and evolution of permafrost in China during the last 20 ka were reconstructed on the basis of large amount of paleo-permafrost remains and paleo-periglacial evidence, as well as paleo-glacial landforms, paleo-flora and paleofauna records. The results indicate that, during the local Last Glacial Maximum(LLGM) or local Last Permafrost Maximum(LLPMax), the extent of permafrost of China reached 5.3×106-5.4×106 km2, or thrice that of today, but permafrost shrank to only0.80×106-0.85×106 km2, or 50% that of present, during the local Holocene Megathermal Period(LHMP), or the local Last Permafrost Minimum(LLPMin). On the basis of the dating of periglacial remains and their distributive features, the extent of permafrost in China was delineated for the two periods of LLGM(LLPMax) and LHMP(LLPMin), and the evolution of permafrost in China was divided into seven periods as follows:(1) LLGM in Late Pleistocene(ca. 20000 to 13000-10800 a BP)with extensive evidence for the presence of intensive ice-wedge expansion for outlining its LLPMax extent;(2) A period of dramatically changing climate during the early Holocene(10800 to 8500-7000 a BP) when permafrost remained relatively stable but with a general trend of shrinking areal extent;(3) The LHMP in the Mid-Holocene(8500-7000 to 4000-3000 a BP)when permafrost degraded intensively and extensively, and shrank to the LLPMin;(4) Neoglaciation during the late Holocene(4000-3000 to 1000 a BP, when permafrost again expanded;(5) Medieval Warming Period(MWP) in the late Holocene(1000-500 a BP) when permafrost was in a relative decline;(6) Little Ice Age(LIA) in the late Holocene(500-100 a BP), when permafrost relatively expanded, and;(7) Recent warming(during the 20 th century), when permafrost continuously degraded and still is degrading. The paleo-climate, geography and paleopermafrost extents and other features were reconstructed for each of these seven periods. 相似文献
13.
E. I. Marchenko N. N. Eremin A. Yu. Bychkov A. E. Grechanovskii 《Moscow University Geology Bulletin》2017,72(5):299-304
Semi-empirical and quantum chemical studies of Al atom energy in CaSiO3 and MgSiO3 with the perovskite-type structure at pressures and temperatures of the Earth’s mantle are reported. The phase diagram for CaSiO3 is reproduced and refined. Probable mechanisms of Al incorporation in the structures studied are considered. According to the results of the calculations, Al is preferably incorporated into MgSiO3, rather than into CaSiO3. Evaluation of the isomorphic capacity of perovskite phases in relation to Al shows that the Al content in MgSiO3 may reach 2.4 mol % at 120 GPa and 2400 K. CaSiO3 cannot be a source of Al atoms in the Earth’s mantle. 相似文献
14.
Aleksey S. Telyakovskiy Gastão A. Braga Satoko Kurita Jeff Mortensen 《Advances in water resources》2010
For certain initial and boundary conditions the Boussinesq equation, a nonlinear partial differential equation describing the flow of water in unconfined aquifers, can be reduced to a boundary value problem for a nonlinear ordinary differential equation. Using Song et al.'s (2007) [7] approach, we show that for zero head initial condition and power-law flux boundary condition at the inlet boundary, the solution in the form of power series can be obtained with Barenblatt's (1990) [2] rescaling procedure applied to the power series solution obtained in Song et al. (2007) [7] for the power-law head boundary condition. Polynomial approximations can then be obtained by taking terms from the power series. Although for a small number of terms the newly obtained approximations may be worse than polynomial approximations obtained by other techniques, any desired accuracy can be achieved by taking more terms from the power series. 相似文献
15.
16.
The results of the field observation of freezing melted puddles on the drift ice in the Arctic Basin carried out in July–September of 2005 during cruise 23 of R/V Akademik Fedorov are analyzed, and a thermodynamical model of the process based on these results is developed. The essential features of the evolution of puddles in the period of autumn cooling were revealed. The unfrozen liquid layer was shown to be a qualitative component of the system that defines its behavior as a whole. We concluded that the sea ice growing from below is absent until the thickness of the frozen water reaches a critical value that is determined by its initial salinity. 相似文献
17.
Moore MJ Mitrofanov IV Valentini SS Volkov VV Kurbskiy AV Zhimbey EN Eglinton LB Stegeman JJ 《Marine pollution bulletin》2003,46(1):107-119
Roach, goby and sturgeon were examined for cytochrome P4501A (CYP1A) expression and histopathology, in relation to contaminant burdens in fish and sediment. Gradients of induction of CYP1A were observed. Roach from the Ural and Ily River Deltas and roach and goby from the two stations nearest the Caspian Sea oil fields displayed higher levels of CYP1A expression in several organs than was observed in fish from further offshore. Great sturgeon and Russian sturgeon showed higher levels of CYP1A expression than was seen in starred sturgeon and gobies in the Ural delta. No fish showed evidence of contaminant-related histopathologies in the organs examined, despite the elevated CYP1A levels. Low levels of polychlorinated biphenyls and elevated levels of inshore and riverine petroleum hydrocarbons from these habitats suggest that this ongoing hydrocarbon exposure, and that from natural sources and long-term oil exploration on the Northeastern Caspian shore, contributed to the CYP1A induction observed. 相似文献
18.
L. A. Akimov S. A. Beletskii I. L. Belkina O. I. Bugaenko Yu. I. Velikodskii I. A. Zhitnik A. P. Ignat’ev V. V. Korokhin S. V. Kuzin G. P. Marchenko A. A. Pertsov 《Astronomy Reports》2005,49(7):579-586
A spectral analysis of a series of integrated MgXII 8.42 Å X-ray intensities recorded by the CORONAS-F SPIRIT spectroheliometer is presented. Statistically significant peaks for periods in the intervals 12–30 min and 40–200 min were found in the power spectra. The power spectrum for these periods changed after the emergence of new photospheric magnetic flux in the active region NOAA 9840. 相似文献
19.
T. Morel S. V. Marchenko P. R. J. Eenens A. F. J. Moffat G. Koenigsberger I. I. Antokhin T. Eversberg G. H. Tovmassian G. M. Hill O. Cardona N. St-Louis 《Astrophysics and Space Science》1998,260(1-2):173-176
Evidence is presented for the existence of a 2.3 day periodicity in the line-profile changes of the apparently singleWolf-Rayet star WR 134. This cyclical variability may be induced either by the presence of an orbiting collapsed companion,
or by the rotational modulation of a largely inhomogeneous outflow.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
20.
Marchenko Moffat Eversberg Hill Tovmassian Morel & Seggewiss 《Monthly notices of the Royal Astronomical Society》1998,294(4):642-656
As a conclusion of our all-sky variability survey of the 'enigmatic' variable WN8 stars, we have carried out coordinated multisite photometric and spectroscopic observations of WN8 stars in 1989 and 1994–1995. We confirm the leading role of the stellar core in restructuring the whole wind. This emerges as a statistical trend: the higher the level of the ∼continuum (i.e. ∼core) light variations, the higher the variability of the P Cygni edges of the optical emission lines. However, the form of the correlation between the light and profile variations is generally different for each individual star. The high level of activity of WN8 stars may be supported/induced by pulsational instability. 相似文献