Preface     

Ivan Pšenčík 《Studia Geophysica et Geodaetica》2006,50(3):323-324

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Tin–polymetallic sulfide deposits in the eastern part of the Dachang tin field (South China) and the role of black shales in their origin   总被引：3，自引：0，他引：3  

Pašava  Jan  Kříbek  Bohdan  Dobeš  Petr  Vavřín  Ivan  Žák  Karel  Delian  Fan  Tao  Zhang  Boiron  Marie-Christine 《Mineralium Deposita》2003,38(1):39-66

The Dafulou and Huile vein and stratabound cassiterite-sulfide deposits and sheeted ore veins at the Kangma cassiterite-sulfide deposit are located in the eastern part of the Dachang tin field. These deposits are hosted in a sedimentary sequence containing significant concentrations of organic matter in the form of Lower Devonian calcareous black shales and hornfels. These rocks together with the younger intrusion of Longxianggai granite (91DŽ Ma) actively participated in the formation of Sn-polymetallic deposits. The following three major stages have been distinguished in stratiform and vein-type orebodies at Dafulou, Huile and Kangma: stage I (cassiterite, pyrrhotite, arsenopyrite, tourmaline, carbonate), stage II - main sulfide stage (quartz, cassiterite, arsenopyrite, pyrrhotite, sphalerite, stannite, pyrite, carbonates) and stage III (native Bi, galena, electrum, sulfosalts). Stage IV (post-ore), recognized at Huile is represented by barren carbonates and zeolites. Whole rock geochemistry has revealed that at Dafulou, Bi and Cu correlate strongly with S, whereas V and Pb correlate well with C_org (organic carbon). The similar distribution patterns of selected elements in average slightly mineralized low-Ca black shales indicate a fluid composition similar for all deposits studied. Studies of graphitization of the organic matter in black shales adjacent to orebodies indicate that d₍₀₀₂₎ and FWHM (full width in half maximum)/peak height values gradually decrease in the following sequence: Dafulou deposit M Kangma deposit M Huile deposit. The pyrolysate of wall rocks at the Dafulou deposit is relatively enriched in asphaltenes and maltenes (55.6-72.0% of the pyrolysate) comparable with pyrolysate obtained from more distal black shales (19.2-28.5%). Typical GC-MS spectra of pyrolysate from distal black shales are dominated by alkanes in the n-C15 to n-C25 range, aromatic molecules being represented mostly by alkyl-naphthalenes. In contrast, only traces of aliphatic hydrocarbons in the n-C14 to n-C18 range and elemental sulfur were identified in pyrolysates from pyrrhotitized wall rocks. The earliest fluid inclusions of the studied system occur in the quartz-tourmaline-cassiterite assemblage of stage I at Dafulou. These inclusions are H₂O-CO₂-CH₄-rich, with 10 to 20 vol% of aqueous phase. P-T conditions of the trapping of inclusions are estimated to be up to 400 °C and 1.3 to 2.0 kbar (between 5.0 and 7.5 km under lithostatic pressure). In contrast, the presence of a low density gaseous CO₂-CH₄ phase indicates relatively low pressures during the formation of the breccia-type quartz-calcite-cassiterite-sulfide mineralization (stage II), when P-T conditions probably reached approx. 380 to 400 °C and 0.6 kbar (up to 6 km under hydrostatic pressure). Fluid inclusion data and oxygen isotope thermometry indicate that cassiterite-sulfide ores of the main sulfide stage (stage II) formed from aqueous-carbonic fluid (CO₂/CH₄ =ᄺ) at temperatures of up to 390 °C at Dafulou and in a temperature range of 250 to 360 °C at Huile and 260 to 370 °C at Kangma. The '³⁴S values of sulfides from Dafulou range mostly between -1 and -6‰, whereas sulfides from the Kangma and Huile deposits are characterized by more negative '³⁴S values (between -8 and -11‰, and between -9 and -12‰, respectively). These data suggest that bacteriogenic sulfides of black shales were a dominant source of reduced sulfur for epigenetic (vein and replacement) mineralization. Oxygen isotopic compositions of five quartz-cassiterite pairs from Dafulou and Huile show a relatively narrow range of calculated oxygen isotope temperatures (250-320 °C, using the equation of Alderton 1989) and high '¹⁸O_fluid values between +8 and +10‰ (SMOW), which are in agreement with fluid derivation from and/or high temperature equilibration with the Longxianggai granite. The carbon and oxygen isotope composition of carbonates reflects variable carbon sources. Stage I calcite is characterized by narrow ranges of '¹³C (-7.0 to -9.5‰ PDB) and '¹⁸O (+15.0 to +17.5‰ SMOW). This calcite shows ubiquitous deformation, evidenced by intense development of twins. Fluid compositions calculated at 330 °C for the Dafulou and Huile deposits and at 270-300 °C for the Kangma deposit ('¹⁸O_fluid between +10.0 and +11.5‰ SMOW, '¹³C_fluid between -5.5 and -7.5‰ PDB), agree with fluid derivation from and/or equilibration with the peraluminous, high-'¹⁸O Longxianggai granite and suggest a significant influence of contact metasedimentary sequences (carbon derived from decomposition and/or alteration of organic matter of calcareous black shales). The '¹³ C values of organic matter from the Lower to Upper Devonian host rocks at the Dafulou deposit (-24.0 and -28.0‰) fit with a marine origin from algae. However, organic matter adjacent to the host rock-ore contact displays a slight enrichment in ¹³C. The organic carbon from the Huile and Kangma deposits is even more ¹³C enriched (-24.6 to -23.5‰). The most heavy '¹³ C values (-16.5‰) were detected in hornfels sampled at the contact of the Upper Devonian sediments with the Longxianggai granite. The '¹³C data broadly correlate with the degree of structural ordering (degree of graphitization) of organic matter, which indicates that both variables are related to thermal overprint.  相似文献   

Multiwavelength monitoring of GRS 1915+105     

Bandyopadhyay  Martini  Gerard  Charles  Wagner  Shrader  Shahbaz  & Mirabel 《Monthly notices of the Royal Astronomical Society》1998,295(3):623-631

Since its discovery in 1992, the superluminal X-ray transient GRS 1915+105 has been extensively observed in an attempt to understand its behaviour. We present here first results from a multiwavelength campaign undertaken from 1996 July to September. This study includes X-ray data from the RXTE All Sky Monitor and BATSE , two-frequency data from the Nançay radio telescope, and infrared photometry from the 1.8-m Perkins telescope at Lowell Observatory. The first long-term, well-sampled infrared light curve of GRS 1915+105 is presented herein; it is consistent with the interpretation of this source as a long-period binary. We compare the various light curves, searching for correlations in the behaviour of the source at differing wavelengths and for possible periodicities.  相似文献   

Linear Amplification of Horizontal Strong Ground Motion in Zagreb (Croatia) for a Realistic Range of Scaled Point Sources   总被引：2，自引：0，他引：2  

Marijan Herak  Ivan Lokmer  Franco Vaccari  Giuliano F. Panza 《Pure and Applied Geophysics》2004,161(5-6):1021-1040

— The linear amplification of the larger horizontal component of strong ground motion along a selected profile in the city of Zagreb is estimated by examining the synthetic waveforms corresponding to a suite of 16 realistically chosen scaled point sources. The accelerograms, computed for the average bedrock model by modal summation, are propagated through local laterally heterogeneous anelastic models by the finite-difference algorithm. The ratio of peak ground acceleration (PGA) and of the response spectra (RS), obtained by using local and bedrock models, define the PGA and RS amplification AMP(PGA) and AMP(RS), respectively. Even variations of the order of commonly observed uncertainties of only dip and rake angles of the causative fault show that both AMP(PGA) and AMP(RS) vary at some sites by more than a factor of two. It follows that, especially for strongly laterally heterogeneous structures, local effects must be determined for each of the relevant sources considering all associated uncertainties as completely as possible. Such a conclusion certainly holds for the case of the microzonation of Zagreb, where the local geology is quite complex, and the seismicity is not confined to a single seismic source zone.  相似文献   

Discussion on "Gold deposits of the Tapajós and Alta Floresta Domains, Tapajós-Parima orogenic belt, Amazon Craton, Brazil" by Santos JOS, Groves DI, Hartmann LA, Moura MA, McNaughton NJ (Mineralium Deposita 36:278–299, 2001)     

Ana Dreher  Silvio Vlach  Sergio Martini 《Mineralium Deposita》2002,37(8):782-784

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Stromboli and its 1975 eruption     

G. Capaldi  I. Guerra  A. Lo Bascio  G. Luongo  R. Pece  A. Rapolla  R. Scarpa  E. Del Pezzo  M. Martini  M. R. Ghiara  L. Lirer  R. Munno  L. La Volpe 《Bulletin of Volcanology》1978,41(3):259-285

On November 4, 1975 in the evening, an eruption took place at Mt. Stromboli. On the following day lava flowed on the Sciara del Fuoco downward to the sea, accompanied by an intense explosive activity at the crater plane. Direct observations on the volcanic activity were carried out since November 6 while a seismic survey was made from Nov. 7 to 12. The total volume of the lava outpoured during this period of activity that lasted 21 days, was estimated to be about 10⁴ m³. This paper reports the results of direct observations, and of the petrological, radioactive disequilibria and seismic activity studies performed for this eruption. The eruption was preceded by an insignificant change of seismic activity, which was monitored by a seismic station located about 2 km East of the crater. A shallow seismicity was strietly related to crater explosions accompanying the eruptive phenomenon. Radioactive disequilibria showed a lack of disequilibrium between²²⁸Ra and²³²Th explainable in terms of a fast rising of magma in the conduit. Chemical analyses of lava samples and deep seismic sounding data indicate a correspondence between the depth (10–15 km) at which crystallization pressure of phenocrysts occurs and a low velocity laver.  相似文献   

Mønsted and Sevel salt domes,North Jutland,and their influence on the Quaternary morphology     

Ivan Madirazza 《International Journal of Earth Sciences》1968,57(3):1034-1066

This paper deals with two salt domes, Mønsted and Sevel, located in northern Jutland, and is primarily concerned with the problem of Quaternary salt tectonics and its possible relationship to the Quaternary morphology.Geological mapping of the two areas during the summers of 1965 and 1966 included a detailed surveying by means of a theodolite of a stream valley extending over the north-eastern part of Mønsted salt dome and of two valleys in the southern part of Sevel salt dome. In the Mønsted area extensive use of aerial photographs was made.In the light of the results of the geological study, an interpretation of the available geophysical data — in the case of Mønsted both gravimetric and magnetic — is attempted.

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Zusammenfassung Die Salzstöcke Mønsted und Sevel in Nordjütland werden untersucht. Es wird versucht in beiden Gebieten eine Beziehung zwischen Quartär-Morphologie und Salztektonik herzustellen.Eine geologische Kartierung der beiden Gebiete wurde im Sommer 1965 und 1966 durchgeführt. Sie umfaßt eine detaillierte Vermessung des Bachlaufes, der über den Nordostteil des Mønsted-Salzstockes fließt, so wie zweier Täler im Südteil des Sevel-Salzstockes.Die Ergebnisse der geologischen Untersuchung werden in Beziehung zu den geophysikalischen Daten — für Mønsted gravimetrische und magnetische gesetzt.

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Résumé Cet article traite deux dômes de sel, Mønsted et Sevel, situés au Nord du Jutland, et il s'occupe en premier lieu du problème de la tectonique du sel pendant le Quaternaire, et son éventuelle influence sur la morphologie quaternaire.L'étude géologique des deux régions, faite au cours des étés 1965 et 1966, comprenait un mesurage détaillé à l'aide d'un théodolite d'une vallée qui s étend sur la partie Nord-Est du dôme de sel à Mønsted et de deux vallées dans la partie Sud du dôme de sel à Sevel. Dans le cas de Mønsted on a fait ample usage de photographies aériennes.S'appuyant sur les résultats de l'étude géologique, l'auteur propose une interprétation des données géophysiques disponibles, qui dans le cas de Mønsted, comportent des mesurages tant gravimétriques que magnétiques.

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Mø nsted Sevel . . ( Mønsted).

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Hydromagnetic dynamo model with spiral convection     

Ivan Cupal  Reviewer G. Siráň 《Studia Geophysica et Geodaetica》1976,20(3):236-254

Summary The present paper deals with a hydromagnetic dynamo model of the generation mechanism of the Earth's magnetic field. An attempt has been made at selecting a flow-velocity field in the Earth's core which would satisfy the condition 0 for regenerating the field according to [2], and which would yield a velocity field pattern on the core surface as given in the papers by Kahle et al. [9]. These conditions are satisfied by the velocityv=V ₁+U ₂ ^c –V ₂ ^c and, geometrically, this velocity field is represented in space by a spiral convective motion. On the core surface two downflows and two upflows with the corresponding rotating cells may then be found. Only the axisymmetric harmonic component regeneration of the magnetic field has been considered. Adequate regeneration equations have been obtained by means of Braginski's method of quantity estimates in order of magnitude.  相似文献   

Geometrical spreading of seismic body waves in laterally inhomogeneous media with curved interfaces of the second order     

Vlastislav ěrvený  Ivan Pšenčík  Reviewer J. Vaněk 《Studia Geophysica et Geodaetica》1975,19(3):298-299

Summary Seismic rays and geometrical spreading in laterally inhomogeneous media are described by a system of ordinary differential equations of the first order. When the ray crosses an interface of the second order, certain quantities in the system change discontinuously. The initial conditions for the system at the point of intersection of the ray with the interface are presented.  相似文献   

Tracking station positioning from artificial satellite observations     

Ivan I. Mueller 《Surveys in Geophysics》1975,2(3):243-276

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