利用密度和核磁共振测井分析Mallik 5L-38井的天然气水合物饱和度     

T．Takayama  陆敬安 《海洋地质》2006,(3):64-70

以前的研究表明密度和核磁共振测井数据可用来精确计算储层的天然气饱和度。传统的气体储层中开发的用于天然气饱和度计算的密度-磁共振法也可用于天然气水合物饱和度分析。在不使用复杂方程或假设的情况下，基于经验方程，密度-磁共振方法可得到精确的地层孔隙度、气体和（或）天然气水合物饱和度。本文通过密度-磁共振响应方法来识别Mallik 5L-38井所穿沉积剖面中的天然气水合物带。结果证明密度-磁共振方法可以计算经气体校正后的孔隙度和精确的天然气水合物饱和度。  相似文献   

1nm锰矿相的金属阳离子交换能力的研究   总被引：6，自引：3，他引：6  

钱江初  T.A.Mellin 《海洋学报》1996,18(4):56-62

人工合成的1nm锰矿相和铜、钴、镍等二价金属阳离子的交换实验表明,1nm锰矿相具有强烈的金属阳离子交换能力.正是这种金属阳离子的交换能力,使得大洋多金属结核大量地富集了铜、钴、镍等有价金属元素.1nm锰矿相对几种金属阳离子的交换的优先顺序为:Cu>Co>Zn≥Ni>Ca>Mg.多金属结核中镍的含量往往高于铜、钴、锌等元素,但在交换顺序中它却低于铜、钴、锌等,这种不一致性说明结核成矿后期的金属离子交换并非是有价金属结合进结核的唯一途径.多金属结核富含铜、钴、镍等有价金属可能是结核初始成矿和成矿后期金属离子交换等多种因素共同作用的结果.  相似文献   

Detection of DNA damage in mussels and sea urchins exposed to crude oil using comet assay     

Taban IC  Bechmann RK  Torgrimsen S  Baussant T  Sanni S 《Marine environmental research》2004,58(2-5):701-705

The single-cell microgel electrophoresis assay or the comet assay was used to evaluate DNA damage of dispersed crude oil on sea urchins (Strongylocentrotus droebachiensis) and mussels (Mytilus edulis L.). Sea urchins were exposed to 0.06 and 0.25 mg/L dispersed crude oil in a continuous flow system, while the mussels were exposed to 0.015, 0.06 and 0.25 mg/L dispersed crude oil. Sea urchin coelomocytes and mussel haemocytes were sampled after 4 and 5 weeks exposure, respectively. In the sea urchin coelomocytes, there was a significant concentration-related increase in the percentage of DNA in comet tail. In mussel haemocytes, there was a significantly higher percentage of DNA in comet tail for all treatments compared to the control. The responses were concentration-related up to 0.06 mg/L oil. The two highest exposure concentrations of mussels were not significantly different from each other. These results indicate that the comet assay can be used for biomonitoring of DNA damage in marine invertebrates following oil contamination.  相似文献   

渤海东部（华北地台）晚第四纪地层学与沉积环境     

Marss.  T 刘光威 《海洋地质前沿》1997,(3):12-14

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Multi-level assessment of chronic toxicity of estuarine sediments with the amphipod Gammarus locusta: II. Organism and population-level endpoints     

Costa FO  Neuparth T  Correia AD  Costa MH 《Marine environmental research》2005,60(1):93-110

This study aimed to test the performance of the amphipod Gammarus locusta (L.) in chronic sediment toxicity tests. It constitutes part of a multi-level assessment of chronic toxicity of estuarine sediments, integrating organism and population-level endpoints with biochemical markers responses. Here we account for organism and population-level effects, while biomarker responses were reported in a companion article. Five moderately contaminated sediments from Sado and Tagus estuaries were tested, comprising 3 muddy and 2 sandy sediments. These sediments either did not show acute toxicity or were diluted with control sediment as much as required to remove acute toxicity. Subsequent chronic tests consisted of 28-day exposures with survival, individual growth and reproductive traits as endpoints. Two of the muddy sediments induced higher growth rates in the amphipods, and improved reproductive traits. This was understood to be a consequence of the amount of organic matter in the sediment, which was nutritionally beneficial to the amphipods, while concurrently decreasing contaminant bioavailability. Biomarker responses did not reveal toxicant-induced stress in amphipods exposed to these sediments. One of the sandy sediments was acutely toxic at 50% dilution, but in contrast stimulated amphipod growth when diluted 75%. This was presumed to be an indication of a hormetic response. Finally the two remaining contaminated sediments showed pronounced chronic toxicity, affecting survival and reproduction. The sex ratio of survivors was highly biased towards females, and offspring production was severely impaired. The particulars of the responses of this amphipod were examined, as well as strengths versus limitations of the sediment test. This study illustrates the utility of this chronic test for toxicity assessment of contaminated estuarine sediments, with potential application all along Atlantic Europe.  相似文献   

Evolutionary status of the pre-protostellar core L1498     

Kuiper TB  Langer WD  Velusamy T 《The Astrophysical journal》1996,468(2):761-773

L1498 is a classic example of a dense cold pre-protostellar core. To study the evolutionary status, the structure, dynamics, and chemical properties of this core we have obtained high spatial and high spectral resolution observations of molecules tracing densities of 10(3)-10(5) cm-3. We observed CCS, NH3, C3H2, and HC7N with NASA's DSN 70 m antennas. We also present large-scale maps of C18O and 13CO observed with the AT&T 7 m antenna. For the high spatial resolution maps of selected regions within the core we used the VLA for CCS at 22 GHz, and the Owens Valley Radio Observatory (OVRO) MMA for CCS at 94 GHz and CS (2-1). The 22 GHz CCS emission marks a high-density [n(H2) > 10(4) cm -3] core, which is elongated with a major axis along the SE-NW direction. NH3 and C3H2 emissions are located inside the boundary of the CCS emission. C18O emission traces a lower density gas extending beyond the CCS boundary. Along the major axis of the dense core, CCS, NH3 and C3H2 emission show evidence of limb brightening. The observations are consistent with a chemically differentiated onion-shell structure for the L1498 core, with NH3 in the inner and CCS in the outer parts of the core. The high angular resolution (9"-12") spectral line maps obtained by combining NASA Goldstone 70 m and VLA data resolve the CCS 22 GHz emission in the southeast and northwest boundaries into arclike enhancements, supporting the picture that CCS emission originates in a shell outside the NH3 emitting region. Interferometric maps of CCS at 94 GHz and CS at 98 GHz show that their emitting regions contain several small-scale dense condensations. We suggest that the differences between the CCS, CS, C3H2, and NH3 emission are caused by a time-dependent effect as the core evolves slowly. We interpret the chemical and physical properties of L1498 in terms of a quasi-static (or slowly contracting) dense core in which the outer envelope is still growing. The growth rate of the core is determined by the density increase in the CCS shell resulting from the accretion of the outer low-density gas traced by C18O. We conclude that L1498 could become unstable to rapid collapse to form a protostar in less than 5 x 10(6) yr.  相似文献   

Detection of a new interstellar molecular ion, H2COH+ (protonated formaldehyde)     

Ohishi M  Ishikawa SI  Amano T  Oka H  Irvine WM  Dickens JE  Ziurys LM  Apponi AJ 《The Astrophysical journal》1996,471(1):L61-L64

A new interstellar molecular ion, H2COH+ (protonated formaldehyde), has been detected toward Sgr B2, Orion KL, W51, and possibly in NGC 7538 and DR21(OH). Six transitions were detected in Sgr B2(M). The 1(1,0)-1(0,1) transition was detected in all sources listed above. Searches were also made toward the cold, dark clouds TMC-1 and L134N, Orion (3N, 1E), and a red giant, IRC + 10216, without success. The excitation temperatures of H2COH+ are calculated to be 60-110 K, and the column densities are on the order of 10(12)-10(14) cm-2 in Sgr B2, Orion KL, and W51. The fractional abundance of H2COH+ is on the order of 10(-11) to 10-(9), and the ratio of H2COH+ to H2CO is in the range 0.001-0.5 in these objects. The values in Orion KL seem to be consistent with the "early time" values of recent model calculations by Lee, Bettens, & Herbst, but they appear to be higher than the model values in Sgr B2 and W51 even if we take the large uncertainties of column densities of H2CO into account. We suggest production routes starting from CH3OH may play an important role in the formation of H2COH+.  相似文献   

Near-infrared spectroscopy of dark asteroids     

Barucci MA  Lazzarin M  Owen T  Barbieri C  Fulchignoni M 《Icarus》1994,110(2):287-291

Near-infrared (J, H and K bands) spectra of nine dark asteroids (chosen among a sample of supposed primitive objects between C and D classes) have been obtained at the Mauna Kea Observatory (Hawaii) with the 2.2-m telescope using KSPEC as spectrograph. The aim of this work was to search for evidence of the presence of organic materials in these objects as found in other planetary bodies as 5145 Pholus, and in some cometary nuclei. A careful analysis of the data has revealed flat or slightly redder spectra than the solar one for all observed asteroids. No evidence of distinct absorption features was found.  相似文献   

Is Russia's demographic situation improving?     

Heleniak T 《Post-Soviet geography》1995,36(10):644-648

"Since the Russian economy recently has shown sings of stabilization, there now is evidence that demographic trends are beginning to improve somewhat. Although the population declined by 164,200, to 148.1 million at the beginning of 1996, the release of new statistical compendia by the Russian statistical agency (Goskomstat Rosii) in 1995 and early 1996 makes it possible to identify several positive trends.... Life expectancy increased for the first time since 1985. The infant mortality rate declined for the second year in a row. The crude death rate declined for the first time in a decade. The birth rate remained at about the same level for the third consecutive year. The rate of natural increase (births minus deaths), although still negative, recorded a moderate increase."  相似文献   

Ethnic results of the 1979 Soviet census     

Shabad T 《Soviet geography》1980,21(7):440-488

This article is based on summary results concerning ethnic composition in the USSR according to the 1979 census. "These results...have been rearranged... to reflect not only the ethnic composition of the USSR and of its republics over time (1959, 1970, 1979), but also shifts in the distribution of particular ethnic groups. Furthermore, ethnic groups are discussed in a regional sequence. In combination with the migration tables based on previous results of the 1979 census...some conclusions can be drawn concerning the ethnic makeup of migrants among republics."  相似文献