Occurrence and distribution of shortnose sturgeon,Acipenser brevirostrum,in the upper tidal Delaware River     

Robert W. Hastings  John C. O’Herron  Kevin Schick  Mark A. Lazzari 《Estuaries and Coasts》1987,10(4):337-341

Sampling in the upper tidal Delaware River between Trenton, New Jersey, and Philadelphia, Pennsylvania, from July 1981 through December 1984 demonstrated the existence of a significant population of shortnose sturgeon. The sturgeon aggregate in the river channel during daylight hours, especially in the area between Trenton and Florence, New Jersey (river km 211.8 to 198.8). Occurrence in the river downstream of Florence appears to be restricted by poor water quality during summer months. Sturgeon were present in the study area throughout the year, but largest numbers were collected from May though November. No spawning was observed during this study, but presence of males with milt suggests that spawning possibly occurs in the Trenton area. Preliminary population estimates (Peterson, Schnabel and Seber-Jolly) indicate an adult population of approximately 6,000–14,000 shortnose sturgeon occupying the upper tidal Delaware River.  相似文献   

An astrometric study of the triple star ADS 48     

O. V. Kiyaeva  A. A. Kiselev  E. V. Polyakov  V. B. Rafal’skii 《Astronomy Letters》2001,27(6):391-397

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Hayashi spectra of the northern hemisphere mid-latitude atmospheric variability in the NCEP–NCAR and ECMWF reanalyses     

Alessandro Dell’Aquila  Valerio Lucarini  Paolo M. Ruti  Sandro Calmanti 《Climate Dynamics》2005,25(6):639-652

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XI International Conference of Radiolarian Paleontologists (InterRad-XI)     

V. S. Vishnevskaya  E. O. Amon  M. S. Afanas’eva  D. A. Zas’ko  T. N. Palechek 《Stratigraphy and Geological Correlation》2007,15(3):333-339

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Long-period oscillations of the line-of-sight velocities in and near sunspots at various levels in the photosphere     

V. I. Efremov  L. D. Parfinenko  A. A. Solov’ev 《Astronomy Reports》2007,51(5):401-410

New observational data on long-period oscillations of the line-of-sight velocities detected via the Doppler shifts of spectral lines observed at various heights in and near sunspots are presented. The sunspots and nearby magnetic elements oscillate with periods ranging from 40 to 80 min. The oscillations in the line-of-sight velocities persist over the entire observation session (up to four hours). These results support theoretical models in which this phenomenon represents natural long-period oscillations (vertical-radial displacements) of entire magnetic elements (sunspots, pores, and magnetic knots) about some stable equilibrium positions.  相似文献   

Hydrocarbons and other volatile components in alkaline rocks from the Ukrainian shield and Kola Peninsula     

S. G. Kryvdik  V. A. Nivin  A. A. Kul’chitskaya  D. K. Voznyak  A. M. Kalinichenko  V. N. Zagnitko  A. V. Dubyna 《Geochemistry International》2007,45(3):270-294

Gas chromatography and other analytical techniques (EMR, PMR, and IR spectroscopy) were used to examine volatile components (CH₄, C₂-C₃, CO₂, CO, H₂, H₂O, and others) in alkaline rocks and minerals from the Ukrainian Shield (eight massifs and dikes of grorudites) and from the Khibina and Lovozero massifs in the Baltic Shield. The alkaline rocks from the Ukrainian Shield are mostly of Proterozoic (1.7–2.1 Ga) age. The alkaline rocks from the Kola Peninsula were confirmed to be rich in methane (21 ± 14 μl/g on average) and other hydrocarbons, whereas the analogous rocks from the Ukrainian Shield are poor in methane (2.1 ± 1.6 μl/g on average at a maximum of 14 μl/g). The latter rocks are richer in CO₂, which is one of the major volatile components of alkaline rocks, including agpaitic nepheline syenites from the Kola Peninsula. The rocks from the Ukrainian Shield often have elevated contents of nitrogen (up to 20 μl/g). The reasons for the differences in the composition of volatile components of rocks from the Kola Peninsula and Ukrainian Shield are as follows: the agpaitic crystallization trends of large massifs in the Kola Peninsula and much less clearly pronounced agpaitic trends in the small massifs in the Ukrainian Shield, the affiliation of these rocks with different complexes, the deeper erosion levels of the Ukrainian alkaline massifs, different ages of these rocks, etc.  相似文献   

Zoning of diamonds from the Mir kimberlite pipe: Results of Fourier-transformed infrared spectroscopy   总被引：1，自引：0，他引：1  

E. A. Vasil’ev  S. V. Sofroneev 《Geology of Ore Deposits》2007,49(8):784-791

Plates prepared of diamonds from the Mir kimberlite pipe were examined with FTIR spectroscopy. It is shown that B1 defects were formed by annealing during crystal growth, whereas B2 centers arose after growth cessation. The development of B2 centers in a natural diamond is the secondary process with respect to the aggregation of the nitrogen admixture. The kinetics of this process is related to the breakdown of an oversaturated solid solution. The results obtained make it possible to estimate the temperature and duration of natural diamond growth.  相似文献   

Principal stages in evolution of Precambrian organic world: Communication 1. Archean and Early Proterozoic     

V. N. Sergeev  M. A. Semikhatov  M. A. Fedonkin  A. F. Veis  N. G. Vorob’eva 《Stratigraphy and Geological Correlation》2007,15(2):141-160

Expounded in this work are the results of critical consideration of published and original data on biologic nature and appearance chronology of different groups of Archean and Lower Proterozoic (3.5–1.65 Ga) paleontological remains known from geological record. Conclusions are substantiated by morphological analysis of structurally preserved microfossils, their facies distribution, and by inferable genesis and principal evolutionary trends of Archean stromatolites. A special attention is paid to variations of organic and carbonate carbon isotope composition in sedimentary successions with paleontological remains and to recent information about discovered, most ancient biomarkers of large groups of organic world. As a result of this approach, a detailed model of Precambrian organic world evolution is suggested.  相似文献   

Lithosphere formation in the central Slave Craton (Canada): plume subcretion or lithosphere accretion?     

Sonja Aulbach  William L. Griffin  Norman J. Pearson  Suzanne Y. O’Reilly  Buddy J. Doyle 《Contributions to Mineralogy and Petrology》2007,154(4):409-427

Major-element compositions of minerals in peridotite xenoliths from the Lac de Gras kimberlites provide constraints on the mode of lithosphere formation beneath the central Slave Craton, Canada. Magnesia contents of reconstructed whole rocks correlate positively with NiO and negatively with CaO contents, consistent with variable partial melt extraction. Alumina and Cr₂O₃ contents are broadly positively correlated, suggestive of melt depletion in the absence of a Cr–Al phase. Garnet modes are high at a given Al₂O₃ content (a proxy for melt depletion), falling about a 7 GPa melt depletion model. These observations, combined with high olivine Mg# and major-element relationships of FeO-poor peridotites (<7.5 wt%) indicative of melt loss at pressures >3 GPa (residual FeO content being a sensitive indicator of melt extraction pressure), and similar high pressures of last equilibration (∼4.2 to 5.8 GPa), provide multiple lines of evidence that the mantle beneath the central Slave Craton has originated as a residue from high-pressure melting, possibly during plume subcretion. Apparent low melt depletion pressures for high-FeO peridotites (>7.5 wt%) could suggest formation in an oceanic setting, followed by subduction to their depth of entrainment. However, these rocks, which are characterised by low SiO₂ contents (<43 wt%), are more likely to be the result of post-melting FeO-addition, leading to spuriously low estimates of melt extraction pressures. They may have reacted with a silica-undersaturated melt that dissolved orthopyroxene, or experienced olivine injection by crystallising melts. A secular FeO-enrichment of parts of the deep mantle lithosphere is supported by lower average Mg# in xenolithic olivine (91.7) compared to olivine inclusions in diamond (92.6).  相似文献   

A RATAN-600 Zenith-Field sky survey. Catalog of radio sources     

N. N. Bursov  Yu. N. Pariĭskiĭ  E. K. Maĭorova  M. G. Mingaliev  A. B. Berlin  N. A. Nizhel’skiĭ  I. A. Glushkova  T. A. Semenova 《Astronomy Reports》2007,51(3):197-214

A catalog of radio sources detected in a deep RATAN-600 survey is presented. The catalog was obtained in the region 0^h ≤ RA_2000.0 ≤ 24^h, Dec_2000.0 = 41°30′42″ ± 2′, at the declination of the bright radio source 3C 84. There were nine sessions of multi-wavelength observations at wavelengths λ = 1–55 cm, and more than 300 daily scans were accumulated at each wavelength. This is the first stage in the reduction of an extensive database accumulated by the Cosmological Gene Project. The RATAN-600 Zenith Field (RZF) catalog was obtained at the central wavelength of 7.6 cm, and contains 437 radio sources, virtually all of which have been identified with NVSS objects. Most of the flux densities for the catalog sources are above the 5σ level. Noise from faint (mainly new) background sources at a level of about 0.8 mJy has been detected. The minimum flux density of the catalog, 2.5 mJy, is comparable to the flux-density linit of the NVSS catalog. The catalog is more than 80% complete for sources with flux densities >3 mJy.  相似文献