Phase equilibria in the system K2O-FeO-MgO-Al2O3-SiO2-H2O-CO2 and the stability limit of stilpnomelane in metamorphosed Precambrian iron-formations     

Takashi Miyano  Cornelis Klein 《Contributions to Mineralogy and Petrology》1989,102(4):478-491

The phase relations of Al- and Fe-bearing silicates in the system K₂O-FeO-MgO-Al₂O₃-SiO₂-H₂O-CO₂, in the presence of quartz and magnetite, are discussed on the basis of mineralogic and petrologic data from Precambrian iron-formations and blueschist facies meta-ironstone from the Franciscan Formation, California. These relations allow an estimation of the physiochemical conditions during low-grade metamorphism of iron-formations. Petrologic data together with available experimental and predicted thermodynamic data on the associated minerals place the upper stability limit of stilpnomelane in iron-formations at about 430–470° C and 5–6 kilobars. Fe-end member stilpnomelane can persist to a maximum temperature of 500° C and pressures up to 6–7 kilobars, although it is unlikely to occur in metamorphosed iron-formations. In iron-formation occurrences the stilpnomelane stability field is bordered by four equilibrium reactions with the assemblages stilpnomelane-zussmanite-chlorite-minnesotaite, stilpnomelane-zussmanite-chlorite-grunerite, stilpnomelane-biotite-chlorite-grunerite, and stilpnomelane-biotite-almandine-grunerite. The stability field is reduced by increasing X(CO₂) and X _Mg ^Stil , and is also a function of a(K ⁺)/ a(H ⁺) in the metamorphic fluid. If the value of a(K ⁺)/ a(H ⁺) is smaller than that defined by the above assemblages, stilpnomelane decomposes to chlorite, but if larger, it is replaced by biotite. At pressures less than 4 kilobars, the zussmanite field is restricted to a very high value of a(K ⁺)/a(H ⁺) (> 5.0 in log units at 1.0 kilobar) where iron-formation assemblages are not stable.  相似文献   

Preferred orientation of plagioclase—neutron diffraction and U-stage data     

H.-R. Wenk  H.J. Bunge  E. Jansen  J. Pannetier 《Tectonophysics》1986,126(2-4)

Pole figures of anorthosite mylonite (An 65) from San Juan Bautista, California, were determined with neutron diffraction using a 23 position sensitive detector. This novel technique enables us to deconvolute the complex diffraction spectrum of this triclinic mineral into fifteen separate peaks hkl which are measured simultaneously. All pole figures display strong preferred orientation with complicated triclinic distributions from which it appears that (001) poles are concentrated normal to the schistosity plane of the specimen. The triclinic mineral is well suited to discuss some fundamental issues of texture representation. If crystals are measured individually (e.g., on the U-stage), positive and negative ends of directions can be unequivocally identified and the whole sphere, rather than a hemisphere, is necessary to represent the distribution of positive axes. This is illustrated for a plagioclase-rich amphibolite from Ornö Huvud, Sweden.  相似文献   

Geotomographic imaging in the study of mining induced seismicity   总被引：1，自引：0，他引：1  

R. P. Young  D. A. Hutchins  J. McGaughey  J. Towers  D. Jansen  M. Bostock 《Pure and Applied Geophysics》1989,129(3-4):571-596

Geotomographic imaging is a technique which allows seismic waves to be used to gain information about the internal structure of rock masses, in a way conceptually similar to medical CAT scanning. Traditional approaches to the study of mining-induced seismic phenomena have concentrated on using passive monitoring methods. This paper gives an overview of the developments in the acquisition, processing and interpretation of geotomographic data and outlines how images can be used in conjunction with passive techniques to study mining-induced seismicity.Presented at the Fred Leighton Memorial Workshop on Mining Induced Seismicity, Montreal 1987.  相似文献   

Derivation ofK-indices using magnetograms constructed from digital data     

E. R. Niblett  E. I. Loomer  R. L. Coles  G. Jansen Van Beek 《Surveys in Geophysics》1984,6(3-4):431-437

The purpose of this study is to investigate the feasibility of deriving the traditionalK index from magnetograms plotted from recorded digital data. Digital magnetic data from Ottawa Observatory are available for theX, Y, andZ components in the form of 1 min averaged values and spot values at selected sampling intervals of 1 sec or greater. It is found that the lowerK values tend to be biased downward by one level when a digitizing interval greater than 30 sec is used for construction of the artificial magnetograms. However, for digitizing intervals of 30 sec or less the reconstructed analogue plots are just as reliable as standard-run Ruska magnetograms for the derivation ofK.Contribution from the Earth Physics Branch No. 1132.  相似文献   

The Queens' flare: Its structure and development; precursors,pre-flare brightenings,and aftermaths     

Cornelis de Jager  Marcos E. Machado  Aert Schadee  Keith T. Strong  Zdeněk Švestka  Bruce E. Woodgate  W. Van Tend 《Solar physics》1983,84(1-2):205-235

We continue previous research on the limb flare of 30 April, 1980, 20:20 UT, observed in X-rays by several instruments aboard the Solar Maximum Mission (SMM). It is shown quantitatively that the flare originated in an emerging magnetically confined kernel (diameter ～ 20″) which existed for about ten to fifteen minutes, and from which energetic electrons streamed, in at least two injections, into a previously existing complicated magnetic loop system thus forming a less bright but extended and long-lived tongue. The tongue had a length of ～ 35 000 km and lasted ～ 90 min in X-rays (～ 10 keV); at lower energies (～ 0.7 keV) it was larger (～ 80 000 km) and lasted longer. The total number of energetic electrons (≈ 10³⁷) initially present in the kernel is of the same order as the number present in the tongue after the kernel's decline. This gives evidence that the energetic electrons in the tongue originated mainly in the kernel. The electron number densities in the kernel and tongue at maximum brightness were ～ 4.5 × 10¹¹ and ～ 1 × 10¹¹ cm^#X2212;3, respectively. During the first eight minutes of its existence the tongue was hotter than the kernel, but it cooled off gradually. Its decline in intensity and temperature was exponential; energy was lost by radiation and by conduction through the footpoints of the loop system. These footpoints have a cross-section of only ～ 3 × 10⁶ km². This small value, as well as photographs in a Civ UV emission line, suggests a highly filamentary structure of the system; this is further supported by the finding that the tongue had a ‘filling factor’ of ～ 10^#X2212;2. Several faint X-ray brightenings (? 0.005 of the flare's maximum intensity) were observed at various locations along the solar limb for several hours before and after the flare. At ～ 30 min before the flare's onset a faint (? 0.02) flare precursor occurred, coinciding in place and shape with the flare. First the kernel precursor was brightest but the tongue precursor increased continuously in brightness and was the brightest part of the precursor some 10–15 min after the first visibility of the kernel precursor, until the start of the main flare. This suggests (weak) continuous electron acceleration in the tongue during a period of at least 30 min. The main flare was caused by strong emergence of magnetic field followed by two consecutive field line reconnections and accelerations in a small loop system, causing footpoint heating. Subsequently plasma streamed (convectively) into a pre-existing system of larger loops, forming the tongue.  相似文献   

Large turbulent elements in supergiant photospheres     

Cornelis De Jager  Jan Vermue 《Astrophysics and Space Science》1979,62(1):245-250

During the cool phase of the super-supergiant HR 8752, which happened around 1973, when the star's spectral type was K2...K5 Ia⁺, the most probable vertical extent of the main turbulent elements in the star's photosphere was about 6 times the density scale height, which is about half the stellar radius. In early-type photospheres (class Ia) it is about 10 times the atmospheric density scale height (about 0.25 of the stellar radius), while in less extreme (luminosity class Ib) medium-type supergiants the most probable vertical extent of the elements is approx. 8 times the density scale height (0.05R). Large turbulent elements are apparently a common feature in supergiant photospheres; the more extreme the supergiant the larger the relative size of the eddies.  相似文献   

Ancient geochemical cycling in the Earth as inferred from Fe isotope studies of banded iron formations from the Transvaal Craton   总被引：8，自引：0，他引：8  

Clark M. Johnson  Brian L. Beard  Nicolas J. Beukes  Cornelis Klein  Julie M. O'Leary 《Contributions to Mineralogy and Petrology》2003,144(5):523-547

Variations in the isotopic composition of Fe in Late Archean to Early Proterozoic Banded Iron Formations (BIFs) from the Transvaal Supergroup, South Africa, span nearly the entire range yet measured on Earth, from –2.5 to +1.0‰ in ⁵⁶Fe/⁵⁴Fe ratios relative to the bulk Earth. With a current state-of-the-art precision of ±0.05‰ for the ⁵⁶Fe/⁵⁴Fe ratio, this range is 70 times analytical error, demonstrating that significant Fe isotope variations can be preserved in ancient rocks. Significant variation in Fe isotope compositions of rocks and minerals appears to be restricted to chemically precipitated sediments, and the range measured for BIFs stands in marked contrast to the isotopic homogeneity of igneous rocks, which have δ⁵⁶Fe=0.00±0.05‰, as well as the majority of modern loess, aerosols, riverine loads, marine sediments, and Proterozoic shales. The Fe isotope compositions of hematite, magnetite, Fe carbonate, and pyrite measured in BIFs appears to reflect a combination of (1) mineral-specific equilibrium isotope fractionation, (2) variations in the isotope compositions of the fluids from which they were precipitated, and (3) the effects of metabolic processing of Fe by bacteria. For minerals that may have been in isotopic equilibrium during initial precipitation or early diagenesis, the relative order of δ⁵⁶Fe values appears to decrease in the order magnetite > siderite > ankerite, similar to that estimated from spectroscopic data, although the measured isotopic differences are much smaller than those predicted at low temperature. In combination with on-going experimental determinations of equilibrium Fe isotope fractionation factors, the data for BIF minerals place additional constraints on the equilibrium Fe isotope fractionation factors for the system Fe(III)–Fe(II)–hematite–magnetite–Fe carbonate. δ⁵⁶Fe values for pyrite are the lowest yet measured for natural minerals, and stand in marked contrast to the high δ⁵⁶Fe values that are predicted from spectroscopic data. Some samples contain hematite and magnetite and have positive δ⁵⁶Fe values; these seem best explained through production of high ⁵⁶Fe/⁵⁴Fe reservoirs by photosynthetic Fe oxidation. It is not yet clear if the low δ⁵⁶Fe values measured for some oxides, as well as Fe carbonates, reflect biologic processes, or inorganic precipitation from low-δ⁵⁶Fe ferrous-Fe-rich fluids. However, the present results demonstrate the great potential for Fe isotopes in tracing the geochemical cycling of Fe, and highlight the need for an extensive experimental program for determining equilibrium Fe isotope fractionation factors for minerals and fluids that are pertinent to sedimentary environments.  相似文献   

Editorial     

Cornelis de Jager  Zdeněk Švestka  Robert F. Howard 《Solar physics》1989,121(1-2):ix-ix

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Abundance and size distribution of transparent exopolymer particles (TEP) in a coccolithophorid bloom in the northern Bay of Biscay     

Jérôme Harlay  Caroline De Bodt  Anja Engel  Sandra Jansen  Quentin d’Hoop  Judith Piontek  Nicolas Van Oostende  Steve Groom  Koen Sabbe  Lei Chou 《Deep Sea Research Part I: Oceanographic Research Papers》2009,56(8):1251-1265

The distribution of transparent exopolymer particles (TEP) was investigated during a coccolithophorid bloom in the northern Bay of Biscay (North Atlantic Ocean) in early June 2006. MODIS chlorophyll-a (Chl-a) and reflectance images before and during the cruise were used to localize areas of important biological activity and high reflectance (HR). TEP profiles along the continental margin, determined using microscopic (TEP_micro) and colorimetric (TEP_color) methods, showed abundant (6.1×10⁶–4.4×10⁷ L^?1) and relatively small (0.5–20 μm) particles, leading to a low total volume fraction (0.05–2.2 ppm) of TEP_micro and similar vertical profiles of TEP_color. Estimates of carbon content in TEP (TEP-C) derived from the microscopic approach yielded surface concentration of 1.50 μmol C L^?1. The contribution of TEP-C to particulate organic carbon (POC) was estimated to be 12% (molar C ratio) during this survey. Our results suggest that TEP formation is a probable first step to rapid and efficient export of C during declining coccolithophorid blooms.  相似文献   

Geographic prospects for large-scale African mammal wildlife conservation     

Cornelis VanderPost 《GeoJournal》2007,69(4):223-237

This work assesses current geographic prospects for large-scale conservation of Africa’s mammals on the basis of statistics on wildlife habitat, elephant numbers, political stability and potential for environmental tourism and concludes that these prospects depend on events in a small number of eastern and southern African (core) countries, geographically grouped into a ‘safari-belt’ between South-Africa and Kenya. Additional countries with good potential are connected to this belt. African countries need more global scientific support for their conservation efforts, particularly with respect to ongoing trans-boundary conservation efforts.  相似文献