Clay mineral diagenesis and quartz cementation in mudstones: The effects of smectite to illite reaction on rock properties   总被引：1，自引：0，他引：1  

Christer Peltonen  Øyvind MarcussenKnut Bjørlykke  Jens Jahren 《Marine and Petroleum Geology》2009

The Late Cretaceous to Early Tertiary sequence of the Vøring and Møre Basins from the Norwegian Sea has been examined with respect to mineralogy based on 319 cutting samples from five wells. A clear relationship between mineralogy and well log data is demonstrated. A significant change with respect to velocity, porosity and density occurs within the depth interval corresponding to 80–90 °C. At shallow depths/temperatures (<2.0 km/70 °C), compaction is mainly mechanical and the physical properties are similar to what has been measured by experimental compaction of mudstones. At greater depths, however, the log derived velocities and densities are higher than those produced by experimental compaction indicating significant chemical compaction. XRD analyses show a progressive alteration of smectite to illite (S–I) within this depth/temperature interval which results in the release of significant amounts of silica into solution. Detrital silt and fine-grained quartz showed no secondary quartz overgrowths. These grains are isolated within a clay matrix and surrounded by clay minerals, thus limiting the available surface area and pore space for quartz overgrowths. Chemical analyses (XRF) indicate that silica is conserved within this depth interval, and the amount released from S–I alteration was locally precipitated. Field emission gun-scanning electron microscopy (FEG-SEM) and cathode luminescence (CL) identified authigenic micro-crystalline quartz cement within the clay matrix at temperatures above ∼85 °C. This is accompanied by an increase in velocity and density indicating that the S–I reaction and the precipitation of authigenic quartz caused a significant change in the rock stiffness.  相似文献   

A 22 GHz receiver with high phase stability for radioastron space-VLBI-mission     

Petri Piironen  Juha Mallat  Antti Räisänen  Petri Jukkala 《Experimental Astronomy》1994,5(3-4):389-404

A space-qualified low-noise 22 GHz receiver for the international space-VLBI mission Radioastron has been constructed. The microwave electronics is realized by using thermally matched hybrid circuits. The most important properties of the receiver are phase stability, sensitivity and reliability. The high sensitivity is due to a cooled low noise HEMT amplifier (LNA). The measured receiver noise temperature is less than 100 K. The phase stability is achieved by compact structure and thermal stabilization. Phase stabilities of better than 0.13°/°C and 0.2°/°C for the receiver and the LNA units are measured, respectively. The calculated reliability of the receiver exceeds the requirement of 0.97 for the three year mission.  相似文献   

Spatial feeding patterns of herring (Clupea harengus L.), sprat (Sprattus sprattus L.), and the three-spined stickleback (Gasterosteus aculeatus L.) in the Gulf of Finland, Baltic Sea     

Peltonen  Heikki; Vinni  Mika; Lappalainen  Antti; Ponni  Jukka 《ICES Journal of Marine Science》2004,61(6):966-971

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Magma-country rock interaction and the genesis of Ni-Cu deposits in the Vammala Nickel Belt,SW Finland   总被引：1，自引：0，他引：1  

P. Peltonen 《Mineralogy and Petrology》1995,52(1-2):1-24

Summary Ultramafic cumulate bodies in the Vammala Nickel Belt, some of which host small magmatic Ni-Cu sulphide deposits, are remnants of synorogenic intrusions that were emplaced into the early Proterozoic Svecofennian arc terrane and became progressively boudinaged by continuing tectonic movements.Mineral and sulphide compositions of mineralised Svecofennian intrusions require that sedimentary sulphides (0.5 wt.% Zn; Se/S 100 x 10^–6) played an important role in ore genesis. It is proposed that when ascending magmas encountered sedimentary formations containing abundant sulphidic black schists, they assimilated external sulphur, which led to the formation of an immiscible sulphide phase in the magma. The high Zn contents of interstitial sulphides (280-450 ppm) and liquidus chrome spinels (0.7–1.0 wt.%) indicate that the parental magma contained much more Zn than conventional assimilation processes would allow. Probably, S and Zn were selectively transferred by C-O-H-S fluids from the black schists into the cooling magma. Desulphidisation (involving conversion of pyrite to pyrrhotite) in the country rocks was driven by thermal energy provided by both the intrusions themselves and the concomitant regional metamorphism. Magma-country rock interaction during ore genesis is also indicated by the presence of minor phases such as graphite, ZnS, PbS, MoS₂, an unknown Re-Mo-Cu-Os sulphide and numerous tellurides among the Fe-Ni-Cu sulphides.During the peak of regional metamorphism small felsic dykes intruded the cumulate bodies and remobilised the interstitial Fe-Ni-Cu sulphides into thin massive ore veins. Compared to interstitial ore, vein sulphides are depleted in Cu, Se, and Zn. Some Fe-Ni-Cu sulphides also migrated, probably due to regional strain effects, into the country rocks and mixed with sedimentary sulphides.Those magmas that formed unmineralised intrusions had already intruded sulphidic black schists and assimilated external S and Zn prior to final emplacement, and had thus become depleted in chalcophile elements and Zn by the segregation of sulphides and chrome spinel, respectively.

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Zusammenfassung Die Genese der Ni-Cu Lagerstätte Vammala, SW Finnland Die ultramafischen Kumulatkorper im Vammala Nickel Belt sind Reste einer synorogenen Intrusion, die innerhalb des friihproterozoischen svecofennischen Inselbogens Platz genommen hat and wahrend fortschreitender Tektonik boudiniert worden ist. Einige dieser Körper führen kleine magmatische Ni-Cu-Sulfid-Vererzungen.Die Mineralzusammensetzung dieser mineralisierten svecofennischen Intrusionen zeigen, daß sedimentare Sulfide (0.5 Gew.% Zn; Se/S 100 x 10 - 6) eine wichtige Rolle bei der Erzgenese gespielt haben. Es wird vermutet, daß die Magmen durch sedimentare Formationen, reich an sulfidischen Schwarzschiefern, aufgestiegen sind, und dabei externen Schwefel assimiliert haben. Dies fiihrte zur Entmischung einer SulfidPhase im Magma. Die hohen Zn-Gehalte der disseminierten Sulfide (280-450 ppm) und der Gehalt an liquidus Chromspinell (0.7–1.0 Gew.%) deuten an, daß der Zn-Gehalt im Stammagma weit höher gewesen sein muß, als es konventionelle Prozesse der Assimilation zulassen. Möglichweise wurden S and Zn selektiv durch C-O-H-S Fluide aus den Schwarzschiefern in das abkühlende Magma eingebracht. Die Desulfidisierung (mit Umwandlung von Pyrit zu Pyrrhotin) im Nebengestein wurde durch thermische Energie angetrieben, die sowohl von den Intrusionen selbst wie auch von der gleichzeitigen Regionalmetamorphose stammt. Die Magma-Nebengestein-Interaktion wahrend der Erzgenese ist auch durch untergeordnete Mineralphasen wie Graphit, ZnS, PbS, MoS₂, einem unbekannten Re-Mo-Cu-Os Sulfid and einigen Telluriden, zusammen mit den Fe-Ni-Cu Sulfiden, dokumentiertWährend des Höhepunktes der Regionalmetamorphose intrudierten dünne felsische Gänge die Kumulatkorper, wobei es zu einer Remobilisierung der disseminierten Fe-Ni Sulfide in dunne, massive Erzgänge gekommen ist. Verglichen mit den disseminier ten Erzen sind die Gang-Sulfide an Cu, Se and Zn verarmt. Einige Fe-Ni-Cu Sulfide migrierten, wahrscheinlich aufgrund von regionalen Strain-Effekten, in die Nebengesteine und vermischten rich mit den sedimentären Sulfiden.Jene Magmen, die nicht-mineralisierte Intrusionen gebildet haben, hatten schon vor der eigentlichen Platznahme die Schwarzschiefer intrudiert and externen S and Zn assimiliert; sic verloren durch die Segregation von Sulfiden and Chromspinell chalkophile Elemente and Zn.

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Mitigation of seal-induced damage in salmon and whitefish trapnet fisheries by modification of the fish bag     

Lehtonen  Esa; Suuronen  Petri 《ICES Journal of Marine Science》2004,61(7):1195-1200

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Archean of Greenland and Fennoscandia     

Pentti Hoelttae Victor Balagansky Adam A. Garde Satu Mertanen Petri Peltonen Alexander Slabunov Peter Sorjonen-Ward Martin Whitehouse 《《幕》》2008,31(1):13-19

The North Atlantic craton in southern West Greenland mainly consists of a tectonic collage of Mesoarchean continental crustal terranes, which were amalgamated at c. 2.7 Ga and are currently exposed at mid-crustal amphibolite to granulite facies levels. Tonalitic orthogneisses predominate, intercalated with slightly older tholeiitic to andesitic metavolcanic rocks and associated gabbro-anorthosite intrusive complexes. The North Atlantic craton also contains enclaves of Eoarchean, c. 3.86-3.6 Ga orthogneisses and supracrustal rocks including the Isua greenstone （or supracrustal） belt. This is the oldest known assemblage of rocks deposited at the surface of the Earth, comprising mafic pillow lavas, banded iron formations and metasedimentary schists with local disseminated graphite of possible biogenic origin. Eoarchean rocks have not been found in Kola and Karelia in Fennoscandia where most rocks are 2.9-2.7 Ga tonalitic-trondhjemitic-granodioritic orthogneisses with intercalated coeval greenstone belts and amphibolites. Mesoarchean 3.0-3.2 Ga rocks are found in the eastern and western parts of the Karelian province. Subduction-related rocks like the Iringora supra-subduction type ophiolite and basalt-andesite-dacite-rhyolite series volcanic rocks in many greenstone belts, as well as eclogites are found in the Archean of Fennoscandia. A clear distinction between Greenland and Fennoscandia is the abundance of 2.75-2.65 Ga igneous rocks in Fennoscandia which indicates that these two cratons had a separate evolution during the Neoarchean.  相似文献   

Model development and calibration for the coupled thermal,hydraulic and mechanical phenomena of the bentonite     

Masakazu Chijimatsu  Lenart Börgesson  Tomoo Fujita  Petri Jussila  Son Nguyen  Jonny Rutqvist  Lanru Jing 《Environmental Geology》2009,57(6):1255-1261

In the international DECOVALEX-THMC project, five research teams study the influence of thermal-hydro-mechanical (THM) coupling on the safety of a hypothetical geological repository for spent fuel. In order to improve the analyses, the teams calibrated their bentonite models with results from laboratory experiments, including swelling pressure tests, water uptake tests, thermally gradient tests, and the CEA mock-up THM experiment. This paper describes the mathematical models used by the teams, and compares the results of their calibrations with the experimental data.  相似文献   

Erratum to: “Mantle depth facies of high-pressure pyroxene in the Kola region”     

Zozulya  D. R.  Peltonen  P.  O’Brien  H.  Lehtonen  M. 《Doklady Earth Sciences》2009,425(1):350-56

Doklady Earth Sciences -  相似文献   

Writing the history of water services     

Tapio S. Katko  Petri S. Juuti 《Physics and Chemistry of the Earth》2009,34(3):156-163

This paper analyses the experiences acquired through several research projects on the history of water and sanitation services by two multidisciplinary teams. Challenges have been faced in identifying feasible objectives, realistic resources, time allocations and unexpected external factors. Water history can preserve cultural heritage, promote reputation management, record vanishing knowledge, and discover new facts.  相似文献   

Pyrope and Cr-diopside as indicators of mantle structure and diamond depth facies in the Kola region     

D. R. Zozulya  P. Peltonen  H. O’Brien 《Geology of Ore Deposits》2008,50(7):524-534

PT parameters of crystallization have been determined for pyropes and Cr-diopsides from loose sediments of the Kola region, taking into account the chemical compositions of these minerals. Being either deep-seated xenocrysts or constituents of mantle xenoliths in kimberlites, pyropes and Cr-diopsides bear information on composition of the lithospheric mantle and its diamond resource potential. It was established that pyropes belong to the lherzolitic (45%), harzburgitic (30%), and eclogitic (25%) mineral assemblages. The Ni thermometry of pyropes yielded their formation temperature at 650–1250°C, which corresponds to a depth interval of 75–190 km. The distribution of different pyrope-bearing assemblages and their trace element composition allowed us to suggest a layered structure of the Kola lithospheric mantle. Its shallow unit (75–110 km) is mainly composed of depleted lherzolite; the medium-deep unit (110–170 km) consists of harzburgite, and the deep unit (170–190 km), of both lherzolite and harzburgite. About 16% of lherzolitic-harzburgitic pyropes were derived from the diamond mantle facies, i.e., from a depth of 140–190 km. Cr-diopsides are subdivided into two genetic groups: eclogitic (high Al₂O₃ and Na₂O, low MgO and CaO) and ultramafic (high MgO, CaO, and Cr₂O₃; low Al₂O₃ and Na₂O). The crystallization parameters of Cr-diopside from deep-seated ultramafic group were determined using the Cr-in-Cpx barometer and En-in-Cpx thermometer. Most samples fall into the graphite stability field (20–45 kbar and 700–1150°C). If these minerals were derived from kimberlites, this implies that the latter were constituents of carbonatite-ultramafic intrusions. Cr-diopsides may also be derived from diamond-free ultramafic xenoliths contained in alkaline ultramafic dikes. Nevertheless, 15% of Cr-diopside compositions fall in the field of diamond stability (55–60 kbar and 1000–1100°C). These conditions fit the geotherm characterizing a low heat flow. The results support the high resource potential of the Kola region for diamonds.  相似文献