An application of a Markov-chain model of shore erosion for describing the dynamics of sediment flux     

V. Ostroumov  V. Rachold  A. Vasiliev  V. Sorokovikov 《Geo-Marine Letters》2005,25(2-3):196-203

Acquisition of coastline retreat rate time sequences (RRTS) is an important component of Arctic coastal monitoring. These data can be used not only to estimate sediment input into the sea during a fixed time period, but also to dynamically simulate sediment flux intensity. The RRTS were investigated at the Marre-Sale (Kara Sea) and Malii Chukochii Cape (East Siberian Sea) key sites. Statistical analysis demonstrated that the RRTS possess Markov characteristic. This allowed coastline dynamics to be described using a Markov-chain model. A model is discussed that combines Markov characteristic and information about the composition and structure of the permafrost sediments to describe sediment flux dynamics.  相似文献   

The influence of ultrahigh-energy cosmic rays on star formation in the early Universe     

E. O. Vasiliev  Yu. A. Shchekinov 《Astronomy Reports》2006,50(10):778-784

The presence of ultrahigh-energy (UHE) cosmic rays results in an increase in the degree of ionization in the post-recombination Universe, which stimulates the efficiency of the production of H₂ molecules and the formation of the first stellar objects. As a result, the onset of the formation of the first stars is shifted to higher redshifts, and the masses of the first stellar systems decrease. As a consequence, a sufficient increase in the ionizing radiation providing the reionization of the Universe can occur. We discuss the possible observational manifestations of these effects and their dependence on the parameters of UHE cosmic rays.  相似文献   

Physical properties of cobalt dugganites Pb3TeCo3P2O14 and Pb3TeCo3As2O14     

M. M. Markina  B. V. Mill  Y. A. Ovchenkov  E. A. Zvereva  A. N. Vasiliev 《Physics and Chemistry of Minerals》2016,43(1):51-58

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Evolution of Intergalactic Gas in the Neighborhood of Dwarf Galaxies and Its Manifestations in the HI 21 cm Line     

E. O. Vasiliev  M. V. Ryabova  Yu. A. Shchekinov  S. K. Sethi 《Astrophysical Bulletin》2018,73(4):401-412

Low-mass galaxies are known to have played the crucial role in the hydrogen reionization in the Universe. In this paper we investigate the contribution of soft x-ray radiation (E ~ 0.1–1 keV) from dwarf galaxies to hydrogen ionization during the initial reionization stages. The only possible sources of this radiation in the process of star formation in dwarf galaxies during the epochs preceding the hydrogen reionization epoch are hot intermediate-mass stars (M ~ 5–8 M_⊙) that entered the asymptotic giant branch (AGB) stage and massive x-ray binaries. We analyze the evolution of the intergalactic gas in the neighborhood of a dwarf galaxy with a total mass of 6 × 10⁸M_⊙ formed at the redshift of z ~ 15 and having constant star-formation rate of 0.01–0.1 M_⊙ yr^?1 over a starburst with a duration of up to 100 Myr. We show that the radiation from AGB stars heats intergalactic gas to above 100 K and ensures its ionization x_e ? 0.03 within about 4–10 kpc from the galaxy in the case of a star-formation rate of star formation 0.03–0.1 M_⊙ yr^?1, and that after the end of the starburst this region remains quasi-stationary over the following 200–300 Myr, i.e., until z ~ 7.5. Formation of x-ray binaries form in dwarf galaxies at z ~ 15 results in a 2–3 and 5–6 times greater size of the ionized and heated region compared to the case where ionization is produced by AGB stars exclusively, if computed with the “x-ray luminosity–star-formation rate” dependence (L_X ~ f_XSFR) factor f_X = 0.1 and f_X ~ 1, respectively. For f_X ? 0.03 the effect of x-ray binaries is smaller that that of AGB star population. Lyα emission, heating, and ionization of the intergalactic gas in the neighborhood of dwarf galaxies result in the excitation of the 21 cm HI line. We found that during the period of the starburst end at z ~11.5–12.5 the brightness temperature in the neighborhood of galaxies is 15–25 mK and the region where the brightness temperature remains close to its maximum has a size of about 12–30 kpc. Hence the epoch of the starburst end is most favorable for 21 cm HI line observations of dwarf galaxies, because at that time the size of the region of maximum brightness temperature is the greatest over the entire evolution of the dwarf galaxy. In the case of the sizes corresponding to almost 0.’1 for z ~ 12 regions with maximum emission can be detected with the Square Kilometre Array, which is currently under construction.  相似文献   

The order-disorder transition in gallium analogue of albite,NaGaSi3O8     

E. E. Senderov  N. S. Vasiliev  E. I. Yudin 《Physics and Chemistry of Minerals》1982,8(2):51-54

The order-disorder transformation in NaGaSi₃O₈ was studied at \(P_{H_2 O} \approx 100\) bar using a hydrous sodium gallium silicate gel and synthetic Ga-albites of various degrees of order as initial materials. The structural state of the gallium albites was determined by the angle separation in X-ray powder patterns of 131 and 1 \(\bar 3\) 1, and of \(\bar 2\) 04 and 060 peaks. The direction of order-disorder transformations was found to change sharply at 938 (±3)°C. This indicates a first order phase transition in NaGaSi₃O₈ as in albite, of which it is the structural analogue.  相似文献   

Early diagenetic greigite as a recorder of the palaeomagnetic signal in Miocene–Pliocene sedimentary rocks of the Carpathian foredeep (Romania)     

Iuliana Vasiliev  Mark J. Dekkers  Wout Krijgsman  Christine Franke  Cor G. Langereis  Tom A. T. Mullender 《Geophysical Journal International》2007,171(2):613-629

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Landslide susceptibility deterministic approach using geographic information systems: application to Breaza town, Romania     

Iuliana Armaş  Florin Vartolomei  Florica Stroia  Livioara Braşoveanu 《Natural Hazards》2014,70(2):995-1017

The study is a deterministic-based approach on landslide susceptibility. The purpose of the paper is to create quantitative susceptibility maps by joining the one-dimension infinite slope stability model with a raster-based GIS (ILWIS) and taking into account the spatial distribution of input parameters. A landslide-prone area, with relative homogeneous geology and geomorphology, located in the Subcarpathian sector of the Prahova River, Romania, was selected for the study. There are frequent problems caused by active landslides in the studied area, especially in years with heavy precipitation, often causing destruction of houses and roads situated on the slopes (1992, 1997, and 2005). Detailed surveys covering a 7-year period provided the necessary input data on slope parameters, hydrological components, and the geotechnical background. Two simulations were used: one on dry soil conditions and one on fully saturated soil conditions. A third test was based on the level of the groundwater table mapped in summer 2008. Detailed analyses were particularly focused on landslides to compare predicted results with actual results using field measurements. The model is very suitable for use in raster GIS because it can calculate slope instability on a pixel basis, each raster cell being considered individually. The drawback of the model is the highly detailed data of input parameters. Despite this disadvantage, in conclusion, the usefulness of slope stability models on a large-scale basis was emphasized under infinitely high failure plain conditions and lithological homogeneity.  相似文献   

Thermodynamic characteristics of water in natural water bodies with a high mineralization     

S. I. Prokopiev  T. E. Ovchinnikova  O. F. Vasiliev 《Izvestiya Atmospheric and Oceanic Physics》2010,46(2):256-260

To adequately describe the hydrophysical processes in water bodies with a high mineralization, it is necessary to take into account the dependence that the thermodynamic characteristics of water have on the amount of salts contained in it. This work investigates some widely known formulas for calculating a number of thermodynamic parameters of mineralized water. The density, freezing temperature, specific heat of evaporation, and relative pressure of saturated vapor over the surface are considered. The possibilities of using these formulas when modeling hydrophysical processes in water bodies with salinity in the range of 0–250 pro mille are analyzed. It is shown that the formulas under consideration should be used when the salinity does not exceed 100 pro mille. If the mineralization is higher, it is necessary to elaborate more suitable formulas on the basis of an approximation of in situ data or data from handbooks.  相似文献   

Methane Content and Emission in the Typical Tundra and the Southern Tundra of the Western Russian Arctic     

Vasiliev  A. A.  Melnikov  V. P.  Zadorozhnaia  N. A.  Oblogov  G. E.  Streletskaya  I. D.  Savvichev  A. S. 《Doklady Earth Sciences》2022,505(1):506-511

Doklady Earth Sciences - The results of studying the emission, content, and isotopic composition of methane in soils of the active layer in the zones of typical and southern shrubby tundra of the...  相似文献   

Fractals in fluctuations of Antarctic ice sheet surface elevation     

V. M. Kotlyakov  L. N. Vasiliev  A. B. Kachalin  M. Yu. Moskalevsky  A. S. Tyuflin 《Doklady Earth Sciences》2015,465(1):1177-1181

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