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41.
A total of 26 polar bears have been killed in Svalbard since January 1987. Fifteen of these cases were self defense, four precautionary measures, six acts of mercy and one unknown. Twelve of the 15 self defense cases occurred in the wilderness; none occurred in populated areas. Most self defence cases involved nonresidents of Svalbard and hence people not familiar with polar bear behaviour and encounters. 相似文献
42.
DANIELA A. VALLINI BIRGER RASMUSSEN BRYAN KRAPE IAN R. FLETCHER NEAL J. MCNAUGHTON 《Sedimentology》2005,52(1):101-122
An ≈ 26 m thick unit of phosphatic sandstone and black shale (the Phosphatic Unit) in the Palaeoproterozoic Mount Barren Group of south-western Australia contains abundant authigenic xenotime crystals showing well-preserved diagenetic textures. Despite extensive regional deformation and thermal metamorphism, the peak of which occurred at ≈ 1205 Ma, the Phosphatic Unit was preserved as a low-strain envelope because of its pre-compaction carbonate and phosphate cementation. In situ U–Pb geochronology of xenotime reveals four discrete age populations at 1693 ± 4, 1645 ± 3, 1578 ± 10 and 1481 ± 21 Ma. When integrated with petrography, the age data place a timeframe on: (i) sediment deposition; (ii) phosphogenesis; (iii) diagenetic cement infilling; (iv) diagenetic pyrite formation; (v) secondary porosity generation; (vi) hydrocarbon migration; (vii) burial compaction; and (viii) hydrothermal alteration, up until peak thermal metamorphism. Xenotime growth at ≈ 1693 Ma occurred prior to compaction, whereas xenotime growth at ≈ 1645 Ma occurred during burial. Xenotime growth at ≈ 1580 Ma and at ≈ 1480 Ma appears to be the far-field record of thermotectonic events associated with intracontinental extension and magmatism recorded elsewhere in Australia. Geochemical analysis, integrated with geochronology, shows a systematic increase in MREE/HREE in xenotime crystals with decreasing age and with increasing stratigraphic depth. Coupled with a decrease in xenotime abundance and age with depth, it suggests that: (i) the main focus of porosity infilling was at the top of the Phosphatic Unit and progressed downwards over the > 200 Myr period of porosity infilling, and (ii) the changes in xenotime REE chemistry may be due to an influx of MREE from increasing amounts of dissolved apatite or changes, with respect to REE solubility, in the physiochemical nature of the fluids with burial depth. 相似文献
43.
ZSOLT R. NAGY IAN D. SOMERVILLE† JAY M. GREGG STEPHEN P. BECKER KEVIN L. SHELTON‡ ANDREW G. SLEEMAN§ 《Sedimentology》2005,52(3):489-512
The Wexford Basin (south-eastern Ireland) is a NE–SW-trending sedimentary basin containing carbonates and evaporites deposited during the Late Tournaisian and Viséan. Two separate depositional areas are defined on the basis of facies and facies associations. Sediments were deposited in inner ramp, lagoonal and peritidal environments near Rosslare, and in a more open-marine, shallow- to moderately deep-water, mid to outer ramp environment in the western area around Duncormick. Thick breccia deposits that occur in the Wexford Basin formed as a result of (i) fault movement that produced syn-sedimentary debris flows in the Late? Chadian (Breccia type I); (ii) dissolution of anhydrite/gypsum and subsequent collapse of sedimentary strata (Breccia type II); and (iii) fracturing and brecciation of porous rock caused by the movement of high temperature, late diagenetic fluids along fault planes (Breccia type III). The NE–SW facies polarity displayed by both sedimentary successions was the result of NW–SE extension and the reactivation of the NE–SW-trending Wexford Boundary Fault during the Chadian. Extension at the SE margin of the basin with downthrow to the NNW gave the basin a half-graben character. Thickening of the debris flow deposits to the SW suggests that while the half-graben was being tilted it also underwent a NE–SW block rotation due to an axial component of that normal fault. 相似文献
44.
On the effect of mid-air collisions on aeolian saltation 总被引:9,自引:0,他引:9
The effect of mid-air collisions on aeolian saltation is investigated using concentration profiles and grain velocities predicted by a numerical saltation model. The probability of a mid-air collision is found to be greater at high wind speeds. It is also found that mid-air collisions tend to reduce the number of grain/bed impacts and thus reduce the number of ejecta near the bed; this, in turn, reduces the intensity of mid-air collisions. It is suggested that this feed-back mechanism significantly influences transport rates at high wind speeds. 相似文献
45.
BARBARA WOHLFARTH GEOFFREY LEMDAHL SIV OLSSON THOMAS PERSSON IAN SNOWBALL JONAS ISING VIV JONES 《Polar research》1995,14(2):253-275
Bjørnøya, a small (178 km2 ) island situated between the mainland of Norway and southern Spitsbergen, provides the opportunity for the reconstruction of early Holocene terrestrial and limnic palaeoenvironments in the southwestern Barents Sea. The AMS 14 C dating technique, geochemical, mineral magnetic, micro and macrofossil analyses were applied to sediments recovered from lake Stevatnet and the results are interpreted in terms of palaeoenvironmental conditions between 9800 and 8300 14 C bp. After the disappearance of local glaciers before ca 980014 C BP, the lake productivity increased rapidly at the same time as pioneer plant communities developed on soils which gradually became more stable. Insect data indicates that strong seasonal contrasts with mean July temperatures around 9°C and mean January temperatures around −12°C prevailed between 9500 and 8300 14 C BP. These high summer temperatures, possibly as much as 4-5°C higher than the present, favoured the development of a flora including Dryas and Angelica cf. archangelica . The enhanced freeze/thaw processes led to an increased erosion of minerogenic and organic material. After 8000 14 C BP the temperatures may have gradually declined. The environmental reconstruction derived from our data set supports the conceptual insolation model which proposes maximum Holocene seasonality for the Northern Hemisphere at ca 9000 14 C BP. 相似文献
46.
The Influence of Viscosity on Fountains in Magma Chambers 总被引:5,自引:4,他引:5
Geological observations suggest that basaltic magmas mix readilybut that rhyolites and basalts can erupt through the same volcanicvent without mixing. The implication is that viscosity may havean important influence on the mixing of magmas. This paper examines the influence of viscosity on magma mixingwhen a magma of low viscosity is injected as a turbulent fountaininto a chamber containing a magma of higher viscosity. Threeseries of experiments were carried out. In the first, the lowviscosity fluid was injected into the tank at a Reynolds number(Re1) of about 1000 to ensure that flow within the fountainwas fully turbulent. Both fluids were maintained at the sametemperature and the viscosity of the host fluid was varied systematically.If the viscosities of the two fluids are similar, turbulencein the fountain leads to extensive mixing and to formation ofa density-stratified layer which collects at the bottom of thetank. However, if the viscosity ratio of the fluids used isgreater than 400, no detectable mixing occurs. Motion withinthe fountain is again fully turbulent but the high momentumof the input fluid is not transmitted to the more viscous hostfluid. Experiments carried out at intermediate viscosity ratiosresulted in intermediate amounts of mixing. Theoretical considerations suggest that the criterion for mixingin turbulent fountains, when a fluid of low viscosity v1 isinjected into a fluid of much higher viscosity v2 is wd>kv2 where w is the flow velocity through an input pipe of diameterd and k is a constant. This relationship is believed to be ageneral one, applying equally to jets and plumes, although thevalues of k may vary with the nature of the flow. The secondseries of experiments was designed to test this relationshipand determine values of k for fountains. The results show that,if wd/v2 > 70, the inflowing fluid mixes with the host fluidas there was no viscosity difference between them. However,if wd/v2 < 7, little or no mixing occurs even if motion withinthe fountain is fully turbulent. In the third series of experiments the temperature of the inputfluid was 70?C above that of the host fluid. This led to heatingofa thin boundary layer of the host fluid, lowering the viscosityof the host fluid adjacent to the fountain and thus allowingadditional mixing between the fluids. This effect was most obviousin the experiment with the highest viscosity ratio (1229) wherea small amount of mixing was detected, compared with no mixingin the equivalent experiment in the first series. The criterion for mixing, wd> kv2 can be applied to naturalmagmas. The results show that if a primitive basaltic magmais injected, as a turbulent fountain or plume, into a chambercontaining fractionated basaltic magma, the two magmas willmix readily. However, if basaltic magma is injected into a chambercontaining granitic melt, little or no mixing occurs. 相似文献
47.
Pyrite replacement of mollusc shells from the Lower Oxford Clay (Jurassic) of England 总被引:1,自引:0,他引:1
IAN ST JOHN FISHER 《Sedimentology》1986,33(4):575-585
Replacement of originally aragonite mollusc shells by pyrite commonly occurs in the Lower Oxford Clay. Petrographic studies show the shells to have constituted complex microenvironments in the sediment. A range of replacement textures is found showing a variable amount of solution of the original aragonite. Three distinct textures were found in crushed pyrite-replaced ammonite shells from heavily pyritized concretions. (1) A texture reflecting the original shell structure due to the replacement of the organic shell-matrix by pyrite. (2) An ovoid texture seen at several stages of replacement reflecting processes occurring at discrete centres of sulphate reduction. (3) Euhedral crystals lining cracks and fractures in the shell. Three types of replacement are found in small gastropods and bivalves from shell bed, some of which may relate to those seen in the ammonites. (1) Replacement of organic shell-matrix by pyrite preserving good shell-microstructure. (2) Replacement showing outwardly good preservation of morphological features but inwardly only the gross structure, such as growth lines, is preserved. (3) Replacement of the shell in a matrix of euhedral pyrite leaving only lines of carbonate inclusions marking the margins of the shell. The replacement textures and types appear to be dependent on the initial structure of the shell and the access of iron and sulphate into the shell. Early stages of replacement appear to proceed by pyrite formation within the organic matrix of the shell, with little or no solution of the carbonate, this produces textures which faithfully mimic the original shell microstructure. It is thought that the lack of carbonate solution is due to a limited availability of iron, brought about by the less intensively reducing nature of the sediment. Later stages of replacement are promoted by the cracking and fracturing of the shell and are, generally, not as faithful to the original shell structure. This is due to the greater availability of iron as the sediment becomes more reducing with burial. 相似文献
48.
The Effect of Postcumulus Reactions on Composition of Chrome-spinels from the Jimberlana Intrusion 总被引:2,自引:2,他引:2
Chromites in olivine adcumulates, mesocumulates and orthocumulatesfrom drill core of the Jimberlana intrusion have been analysedand related to the cumulate type and to the nature of the surroundingsilicate mineral. Chromites in adcumulates and mesocumulatesshow a restricted range of composition and are high in Mg, Aland Cr. The orthocumulate chromites vary in composition fromthat found in adcumulates to chromites which are much higherin Fe and Ti and with a higher Fe3?: Fe2? ratio. The chromitesin orthocumulates vary in composition depending upon the natureof the enclosing silicate mineral. This is believed to reflectthe ability of the enclosing mineral to protect the originalcumulus chromite from reaction with the intercumulus liquid.Thus chromite within early bronzite oikocrysts was protectedfrom reaction whereas that in plagioclase and phlogopite wasprotected at a much later stage and has a higher Fe and Ti contentChromite within olivine appears to have been able to equilibratewith intercumulus liquid until late in the magmatic historyexcept where the olivine enclosing chromite has itself beensurrounded by bronzite. It is suggested that chromite can exchangeelements with intercumulus liquid through the olivine. Thereare two possibilities; either elements such as Cr, Al, Ti andFe3 ? were able to diffuse through the olivine structure orthe apparently enclosed chromite crystals were able to maintaindirect contact with the melt along fine fractures produced bythe differential thermal contraction of olivine and chromite. The average diameters of chromite crystals within orthocumulatebronzite and olivine are 28 and 20 microns respectively whereaschromites in plagioclase and phlogopite have average diametersof 48 and 56 microns. There is no obvious correlation betweenthe size of the chromite and their composition for grains foundwithin a particular silicate. Chromites of every size have beenable to equilibrate with the liquid unless they were protectedfrom reaction. Nucleation of reaction products played an important role indetermining the final composition of any particular chromitecrystal. The significance of reaction and nucleation on a localscale of millimetres is considered with respect to the majorsilicates and to the location of the last liquid. It is suggestedthat the last liquid tended to concentrate in pockets of reactantcrystals, where product crystals failed to nucleate until latein the magmatic history. It is estimated that in rocks withan orthocumulate texture, the intercumulus liquid crystallizedover a temperature range as large as 300 ?C and that it becamesignificantly more oxidizing near the solidus temperature. 相似文献
49.
Mineralogy, Chemistry, and Genesis of the Boninite Series Volcanics, Chichijima, Bonin Islands, Japan 总被引:12,自引:1,他引:11
TAYLOR REX. N.; NESBITT ROBERT W.; VIDAL PHILLIPE; HARMON RUSSELL S.; AUVRAY BERNARD; CROUDACE IAN W. 《Journal of Petrology》1994,35(3):577-617
The Bonin archipelago represents an uplifted fore-arc terrainwhich exposes the products of Eocene supra-subduction zone magmatism.Chichijima, at the centre of the chain, represents the typelocality for the high-Mg andesitic lava termed boninite. Therange of extrusives which constitute the boninite series volcanicsare present on Chichijima, and are disposed in the sequenceboninite-andesite-dacite with increasing height in the volcano-stratigraphy.Progression to evolved compositions within the Chichijima boniniteseries is controlled by crystal fractionation from a boniniteparental magma containing 15% MgO. Olivine and clinoenstatiteare the initial liquidus phases, but extraction of enstatiticorthopyroxene, followed by clinopyroxene and plagioclase, isresponsible for the general evolution from boninite, throughandesite, to dacite. Some andesites within the overlying MikazukiyamaFormation are petrographically distinct from the main boniniteseries in containing magnetite phenocrysts and a high proportionof plagioclase. As such, these andesites have affinities withthe calc-alkaline series. Major and trace element data for 74 boninitic series rocks fromChichijima are presented. Although major element variation isdominantly controlled by high-level crystal fractionation, thelarge variations in incompatiable trace element concentrationsat high MgO compositions cannot be explained by this mechanism.Nd, Pb, and Sr isotopic data indicate the following: (1) a strongoverprint on 87Sr/86Sr by seawater alteration; (2) Pb isotopeslie above the northern hemisphere reference line (NHRL) andare thus similar to the <30-Ma are and basin lavas of theIzuBonin system, and (3) Nd(40 Ma) ranges between 2.8and 6.8 within the boninite series volcanics. Differences inrare-earth elements (REE), Zr, Ti, and 143Nd/144Nd at similardegrees of fractionation can be explained by the addition ofa component of fixed composition from the down-going oceaniccrustal slab to a variably depleted source region within theoverlying wedge. Data presented for Sm/Zr and Ti/Zr indicatethat boninite series volcanics are characterized by low valuesfor both of these ratios. In particular, boninites appear tohave uniquely low Sm/Zr ratios. These characteristics may bethe result of slab melting in the presence of residual amphibole;the resultant melt could combine with typical slab dehydrationfluids and infiltrate the overlying mantle wedge. Such a fluidmeltcomponent could mix either with shallow mantle or directly withprimitive melts from depleted mantle. Trace elements, REE, andisotope data thus point to a model for boninite genesis whichrequires tightly constrained pressuretemperature conditionsin the slab combined with melting of a variably depleted sourcein the overlying wedge. Such constraints are rarely met exceptduring the subduction of juvenile oceanic crust beneath a young,hot overriding plate. 相似文献
50.
High-Temperature Fluid-Rock Interaction and Scapolitization in an Extension-Related Hydrothermal System, Mary Kathleen, Australia 总被引:1,自引:0,他引:1
OLIVER NICHOLAS H. S.; RAWLING TIMOTHY J.; CARTWRIGHT IAN; PEARSON PAUL J. 《Journal of Petrology》1994,35(6):1455-1491
In the polymetamorphic Mary Kathleen Fold Belt, at the centreof the Proterozoic Mount Isa Inlier, Queensland, an early phaseof extension (17601730 Ma) resulted in intrusion of voluminousgranitic and doleritic magmas into the carbonate-evaporite-dominatedCorella Formation at 510 km depths. Widespread high-temperaturemetasomatism ensued, involving scapolitization in dolerite,formation of albite-scapolite shear zones in granite, exo- andendoskarn formation, and a zone of KNaCa alterationin the lowermost Corella Formation. Granites and dolerites werealtered to an unusual NaCa-rich bulk composition, reflectinghigh-temperature infiltration of highly saline, chemically reactiveexternally derived fluid. The alteration products and theirdistribution suggest not only reaction of magmatic/aqueous fluidswith the country rocks but also extensive halite dissolutionand recirculation of saline fluids back into the intrusive bodies.The bulk of fluid flow occurred at high temperatures (500700C), and major element and isotopic fronts were generally notsmoothed out by the effects of temperature gradients, with theexception of one part of the system which shows evidence forup-temperature fluid flow. Analysis of oxygen isotopic dataand the position of isotopic and geochemical fronts revealstime-integrated fluid fluxes of up to 2 104 m3/m2 for themetasomatism. Although very high salinities (up to 50 mol% NaCl)were attained by evaporite dissolution, 18O values of most alterationproducts are in the range 712%, reflecting a predominanceof oxygen derived from an igneous fluid. The position and interrelationshipsof metasomatic and isotopic fronts indicate an earlier stageof infiltration dominated by fluid released from crystallizinggranite (with 18O 1012%), and a later stage (18O 79%)in which fluid had already interacted with halite and a mixedmafic-felsic igneous source or was repeatedly circulated betweenthese rock types during alteration. The data reflect only aminimal contribution from fluids produced by devolatilizationof the abundant carbonate-bearing rocks in the Corella Formation,and there are substantial areas of Corella Formation rocks thathave escaped metasomatism during this phase of intrusion-relatedhydrothermal activity and during the subsequent regional metamorphicoverprint. Along with the requirement that the fluids dissolvedlarge amounts of halite from the same sequence, and the structuralobservations, we favour a model where fluid was preferentiallychannelled along specific permeable conduits, including formerevaporite layers, before interaction with the now exposed alteredrocks. Fluid was probably driven by both convective circulationand dilatancy-related deformation accompanying emplacement ofmagmas into a major crustal extensional dcollement. 相似文献