Geodynamic setting of gold ore deposits of the neoproterozoic bodaibo trough     

Academician of the RAS M. I. Kuz’min  V. V. Yarmolyuk  A. I. Spiridonov  V. K. Nemerov  A. I. Ivanov  G. L. Mitrofanov 《Doklady Earth Sciences》2006,407(2):397-400

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Geodynamic setting of gold ore deposits of the neoproterozoic bodaibo trough     

M. I. Kuz&#;min  V. V. Yarmolyuk  A. I. Spiridonov  V. K. Nemerov  A. I. Ivanov  G. L. Mitrofanov 《Doklady Earth Sciences》2006,407(3):397-400

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Specific features of picroilmenite composition in various diamondiferous fields of the Yakutian province     

S. I. Kostrovitsky  N. V. Alymova  D. A. Yakovlev  I. V. Serov  A. S. Ivanov  V. P. Serov 《Doklady Earth Sciences》2006,406(1):19-23

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Basanites of Mt. Khukhch: First mineralogical-geochemical data on the Neogene K-Na alkaline magmatism in western Kamchatka     

A. B. Perepelov  M. Yu. Puzankov  A. V. Ivanov  T. M. Filosofova 《Doklady Earth Sciences》2006,409(5):765-768

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Response of the Arctic benthic community to excessive amounts of nontoxic organic matter     

Serge Chivilev  Mikhail Ivanov 《Marine pollution bulletin》1997,35(7-12):280-286

The paper presents a study of the effect of excessive amounts of organic matter (OM) on Arctic benthos. The source of nontoxic OM is from the mariculture of blue mussels in the White Sea (north-western area of Russia). The use of multivariate analysis procedures made it evident that in the Arctic conditions benthos is incapable of annual utilization of more than 1.5 kg dry OM m⁻² from an external source. Mineralization of OM accumulated in sediments will deteriorate the oxygen regime. The critical concentration of OM in sediments is 9–10%. An excess over this threshold leads to the formation of oxygen-free zones at the bottom, and degradation of benthos community.  相似文献   

Improved spatial resolution for U-series dating of opal at Yucca Mountain, Nevada, USA, using ion-microprobe and microdigestion methods     

James B Paces  Leonid A Neymark  Harold M Persing 《Geochimica et cosmochimica acta》2004,68(7):1591-1606

Two novel methods of in situ isotope analysis, ion microprobe and microdigestion, were used for ²³⁰Th/U and ²³⁴U/²³⁸U dating of finely laminated opal hemispheres formed in unsaturated felsic tuff at Yucca Mountain, Nevada, proposed site for a high-level radioactive waste repository. Both methods allow analysis of layers as many as several orders of magnitude thinner than standard methods using total hemisphere digestion that were reported previously. Average growth rates calculated from data at this improved spatial resolution verified that opal grew at extremely slow rates over the last million years. Growth rates of 0.58 and 0.69 mm/m.y. were obtained for the outer 305 and 740 μm of two opal hemispheres analyzed by ion microprobe, and 0.68 mm/m.y. for the outer 22 μm of one of these same hemispheres analyzed by sequential microdigestion. These Pleistocene growth rates are 2 to 10 times slower than those calculated for older secondary calcite and silica mineral coatings deposited over the last 5 to 10 m.y. dated by the U-Pb method and may reflect differences between Miocene and Pleistocene seepage flux. The microdigestion data also imply that opal growth rates may have varied over the last 40 k.y. These data are the first indication that growth rates and associated seepage in the proposed repository horizon may correlate with changes in late Pleistocene climate, involving faster growth during wetter, cooler climates (glacial maximum), slower growth during transition climates, and no growth during the most arid climate (modern). Data collected at this refined spatial scale may lead to a better understanding of the hydrologic variability expected within the thick unsaturated zone at Yucca Mountain over the time scale of interest for radioactive waste isolation.  相似文献   

Iceberg drifting and distribution in the Vilkitsky Strait studied by detailed satellite radar and optical images     

A. A. Kucheiko  A. Yu. Ivanov  A. A. Davydov  A. Yu. Antonyuk 《Izvestiya Atmospheric and Oceanic Physics》2016,52(9):1031-1040

This paper is devoted to the detection and identification of icebergs in the Russian Arctic Seas from the use of high- and medium-resolution radar and optical images from EROS-B, Radarsat-1, Radarsat-2, SPOT-4 and SPOT-5 Earth observation satellites. In July–September of 2011–2013, the SCANEX Research and Development Center, the Federal State Unitary Enterprise Atomflot, and other partner organizations provided operational satellite monitoring of icebergs in the Kara Sea and the Laptev Sea. More than 130 highly detailed optical and radar images were received and processed. The Vilkitsky Strait—one of the narrowest and most dangerous places within the Northern Sea Route—was chosen as an experimental polygon. As a result, iceberg location in the strait during the 2011–2013 navigation periods was analyzed, as were the iceberg size, area, drift direction, and height.  相似文献   

Modeling of oil spreading in a problem of radar multiangle diagnostics of Sea surface pollutions     

A. Ya. Matveev  A. A. Kubryakov  A. G. Boev  D. M. Bychkov  V. K. Ivanov  S. V. Stanichny  V. N. Tsymbal 《Izvestiya Atmospheric and Oceanic Physics》2016,52(9):940-950

The possibilities of a multiangle method of radar diagnostics to determine thickness of an oil film on a sea surface by comparing the radar data with the quantitative modeling results obtained using the model of oil spreading dynamics are analyzed. The experimental results of the remote sensing of the Caspian Sea water area near the Neftyanye Kamni oil field by the Envisat-1 synthetic aperture radar (SAR) and the new Floating Objects Tracking System (FOTS) model of oil spreading are used for the analysis. The model allows to calculate the dynamics and change in the mass and size of an oil slick basing only on the available data of satellite measurements and atmospheric reanalysis.The model takes into account the main processes that influence the slick formation (gravity spreading, advective transport, dispersion, emulsification, turbulent mixing, and evaporation). This model is used to calculate the thickness evolution and dynamics of the displacement of oil slicks in the period between two consecutive radar images of this region (0.5–4 days) and to estimate the volumes of oil spilled in the field. The good consistence of the height of the oil film calculated using radar measurements and the modeling results confirms the method’s reliability.  相似文献   

The Ozernoye meteorite: New data on mineralogy     

Yu. V. Erokhin  V. A. Koroteev  V. V. Khiller  E. V. Burlakov  K. S. Ivanov  D. A. Kleimenov 《Doklady Earth Sciences》2016,471(2):1273-1276

New data on the mineral composition of the Ozernoye meteorite, found in the Kurgan region in 1983, are presented. It has been found that that the meteorite’s matter is composed of olivine (chrysolite), orthopyroxene (bronzite), clinopyroxene (augite), maskelynite, chromite, ilmenite, metals Fe and Ni (kamasite, taenite), sulfides (troilite, pentlandite), chlorapatite, and merrillite. Augite, taenite, pentlandite, and merrillite were identified in the Ozernoye meteorite for the first time. The chemical compositions are given for all these minerals. The meteorite itself is an ordinary chondrite stone belonging to petrological type L5.  相似文献   

Scientific problems addressed by the Spektr-UV space project (world space Observatory—Ultraviolet)     

A. A. Boyarchuk  B. M. Shustov  I. S. Savanov  M. E. Sachkov  D. V. Bisikalo  L. I. Mashonkina  D. Z. Wiebe  V. I. Shematovich  Yu. A. Shchekinov  T. A. Ryabchikova  N. N. Chugai  P. B. Ivanov  N. V. Voshchinnikov  A. I. Gomez de Castro  S. A. Lamzin  N. Piskunov  T. Ayres  K. G. Strassmeier  S. Jeffrey  S. K. Zwintz  D. Shulyak  J.-C. Gérard  B. Hubert  L. Fossati  H. Lammer  K. Werner  A. G. Zhilkin  P. V. Kaigorodov  S. G. Sichevskii  S. Ustamuich  E. N. Kanev  E. Yu. Kil’pio 《Astronomy Reports》2016,60(1):1-42

The article presents a review of scientific problems and methods of ultraviolet astronomy, focusing on perspective scientific problems (directions) whose solution requires UV space observatories. These include reionization and the history of star formation in the Universe, searches for dark baryonic matter, physical and chemical processes in the interstellar medium and protoplanetary disks, the physics of accretion and outflows in astrophysical objects, from Active Galactic Nuclei to close binary stars, stellar activity (for both low-mass and high-mass stars), and processes occurring in the atmospheres of both planets in the solar system and exoplanets. Technological progress in UV astronomy achieved in recent years is also considered. The well advanced, international, Russian-led Spektr-UV (World Space Observatory—Ultraviolet) project is described in more detail. This project is directed at creating a major space observatory operational in the ultraviolet (115–310 nm). This observatory will provide an effective, and possibly the only, powerful means of observing in this spectral range over the next ten years, and will be an powerful tool for resolving many topical scientific problems.  相似文献