Relations between left-lateral strike-slip faults and right-lateral monoclinal kink bands in granodiorite,Mt. Abbot quadrangle,Sierra Nevada,California

Small left-lateral strike-slip faults and right-lateral monoclinal kink bands with subvertical fold axes may be related to the formation of a very large right-lateral kink band (Bear Creek kink band), about 8 km wide and at least 15 km long, trending N27W along Bear Creek Valley in the Mt. Abbot quadrangle, Sierra Nevada, California.A foliation within Bear Creek Valley is defined by vertical slabs of granodiorite bounded by joints and faults. Small strike-slip faults and larger fault zones have nucleated along preëxisting joints and accommodated shearing between granodiorite slabs. The orientations of small cracks that occur near the tips of faults or connect adjacent fault segments indicate that the direction of maximum compression was about 20° counterclockwise from traces of joints at the time the faults nucleated. In some places where faults are closely spaced there are small, right-lateral kink bands with widths of 1 to 20 m. The slabs of granodiorite are gently curved through the kink bands, and analysis of the orientations of slabs in the limbs of the small kink bands indicates that the direction of maximum compression during kink-band formation was 15° to 20° counterclockwise from the traces of faults outside the kink bands. The orientation of the maximum compression for the formation of the small cracks at tips of many strike-slip faults and for the formation of the small kink bands, relative to the orientation of the maximum compression inferred from the joints on the limb of Bear Creek kink band, suggests that the foliation within the Bear Creek Valley has reoriented a maximum of 40° to 60° clockwise. Although the various orientations of joints, faults, and kink bands could be explained in terms of different regional compression directions at different places and at different times in the Mt. Abbot quadrangle, a much simpler interpretation, based on analysis of large and small structures in the granodiorite in Bear Creek Valley, is that they all formed in response to one maximum regional compression in the direction N25E.     

Numerical studies of mesoscale motion in a mixed layer over the Northern Alpine foreland

A one-layer mesoscale model based on the shallow water equations has been developed to examine atmospheric flow patterns within a well mixed planetary boundary layer over the Swiss Middleland. The model incorporates frictional and synoptic forcing effects and has a realistic meso- scale representation of the Alpine and surrounding orography. Some model results are shown for one particular Case Study and also for several situations corresponding to different synoptic scale forcing.     

Surface albedo at a tower site in Lake Ontario

Measurements of incoming global, diffuse and reflected radiation at a tower site in Lake Ontario are used to evaluate components of surface albedo. Albedo for diffuse radiation lies between 0.074 and 0.082 and a coefficient for backscatter from sub-surface water layers shows little deviation from a mean of 0.017. Direct beam albedo for a calm surface follows the Fresnel law. Waves increase direct-beam albedo particularly at higher solar zenith angles. A pronounced dependence of albedo upon zenith angle for clear skies decreases with increasing cloud amount and becomes undetectable in overcast conditions. On a daily basis, albedo ranged between 0.07 in early July to 0.11 in mid-November. Day-to-day scatter is within ±1% of the mean seasonal trend.     

Spreading of rock avalanche debris by mechanical fluidization

SummarySpreading of Rock Avalanche Debris by Mechanical Fluidization Two hypotheses for the motion of large rock avalanches (sturzstroms) are examined: (a) that sturzstrom deposits result from the spreading of a mass of debris in a fluidised state under the influence of gravity, and (b) that the debris becomes fluidised because of the existence of a high shear rate in the basal region. The first hypothesis is supported by data describing the length of sturzstrom deposits, and the second is shown to be in agreement with simple laboratory tests, with the grain-flow theory of Bagnold and with the characteristic features of sturzstrom deposits.With 7 Figures     

An evaluation of three-body interatomic forces and formulation of a general model

Several deficiencies are demonstrated in previous formulations of three-body interatomic forces, and revised and extended formulations are presented for the case of the NaCl lattice. A commonly used formulation of non-central forces and a formulation of the effect of ellipsoidal atom deformation are incorrect. Atom deformation should in general introduce two degrees of freedom in the NaCl lattice, but the only previous correct formulation of deformation effects, the commonly used “breathing shell model,” includes only one degree of freedom. The “shell model” of polarizable atoms has been correctly formulated, but applications seem to have been arbitrarily restricted to the case where short-range forces act only on shells, and not on cores. Because of these errors and incompletenesses, it is concluded that no three-body forces have been convincingly established or characterized, although the necessity of their inclusion in models is clear.     

A spatial and temporal analysis of second home ownership in West Wales

A locational analysis is presented of second (or holiday) homes in Cemaes. West Wales Time series tenure data for the period 1960–1977 was collected for every dwelling in the study area By adopting a data collection methodology including systematic local enquiry, it is hoped that this project avoids the main weaknesses of second home studies in Britain. namely definitional problems, data inaccuracy. and lack of an explicit time dimension Moreover, data collection and analysis was planned within an hypothesis testing framework Using elementary statistical techniques, conclusions are drawn as to the factors affecting the spatial distribution of second homes and its evolution over time.     

Deriving the normalised ion-neutral collision frequency from EISCAT observations

Common programme observations by the EISCAT UHF radar revealed an extended interval, post geomagnetic local noon on 03 April 1992, during which the F-region ion velocity orthogonal to the geomagnetic field was significantly enhanced, to values exceeding 2 km s⁻¹ corresponding to a perpendicular electric field of some 100 mV m⁻¹. Observations from this interval are used to illustrate a method by which estimates of the E-region ion-neutral collision frequency may be derived in the presence of enhanced electric field. From both the rotation of the ion velocity vector and the reduction in the ion velocity magnitude relative to that in the F-region, independent estimates of the normalised ion-neutral collision frequency are made at the UHF E-region tristatic altitudes; the derived values are, in general, lower than model predictions. Although initial calculations assume a stationary neutral atmosphere, first-order estimates of the E-region neutral wind are subsequently employed to calculate revised estimates of the normalised ion-neutral collision frequency; these neutral winds are derived by attributing the difference between predicted and observed enhancements in field-parallel ion temperature to thermospheric motion. The inclusion of neutral winds, which are themselves not inconsiderable, appears to have only a limited effect on the normalised collision frequencies derived.     

Interannual variability and regional climate simulations

Summary An assessment is made of a regional climate model's skill in simulating the mean climatology and the interannual variability experienced in a specific region. To this end two ensembles comprising three realizations of month-long January and July simulations are undertaken with a limited are a operational NWP model. The modelling suite is driven at its lateral boundaries by analysed meteorological fields and the computational domain covers Europe and the North-western Atlantic with a horizontal resolution of 56 km.Validation is performed against both operational ECMWF analyses and objectively analysed precipitation fields from a network of ~ 1400 SYNOP rain gauge stations. Analysis of the simulated ensemble-mean climatology indicates that the model successfully reproduces both the winter and summer distributions of the primary dynamical and thermodynamical field, and also provides a reasonable representation of the measured precipitation over most of Europe. Typically the domain averaged model-biases are below 0.5 K for temperature and 0.1 g/kg for specific humidity. Analysis of the interannual variability reveals that the model captures the wintertime changes including that of the precipitation distribution, but in contrast the summertime precipitation totals for the individual years is not simulated satisfactorily and only partially reproduces the observed regional interannual variability.The latter shortcomings are related to the following factors. Firstly the model bias in the dynamical fields is somewhat larger for summer than winter, while at the same time summertime interannual variability is associated with weaker effects in the dynamical fields. Secondly the summertime precipitation distribution is more substantially affected by small-scale moist convection and surface hydrological processes. Together these two factors suggest that summertime precipitation over continental extratropical land masses might be intrinsically less predictable than wintertime synoptic scale precipitation.With 17 Figures     

Constraints on Archaean crustal evolution of the Zimbabwe craton: a U-Pb zircon,Sm-Nd and Pb-Pb whole-rock isotope study

 The U-Pb ages of zircons from seven felsic volcanic and plutonic rocks from northern Zimbabwe combined with field data and Pb-Pb and Sm-Nd whole-rock isotope data, constrain the timespan of development of the Harare-Shamva granite-greenstone terrain and establish the relative involvement of juvenile mantle-derived and reworked crustal material. Basement-cover field relationships and isotope and geochemical data demonstrate that the greenstones were deposited onto 3.2–2.8 Ga basement gneisses, in ensialic, continental basins. Geodynamic models for the generation of the areally extensive bimodal magmatic products and growth of the pre-existing crustal nucleus consistent with our interpretations are rift-related: (1) intracontinental rifting related to mantle plume activity or; (2) rifting in a back-arc environment related to a marginal volcanic arc. The data, in conjunction with field evidence, do not indicate the presence and accretion of an older (ca. 2.70 Ga) and a younger (ca. 2.65 Ga) greenstone sequence in the Harare part of the greenstone belt, as was recently postulated on the basis of SHRIMP zircon ages. Zircon ages for basal felsic volcanics (2715±15 Ma) and a subvolcanic porphyry (2672±12 Ma) constrain the initiation and termination of deposition of the greenstone sequence. The timespan of deposition of the Upper Bulawayan part of the greenstone sequence corresponds well with radiometric ages for Upper Bulawayan greenstones in the central and southern part of the craton and supports the concept of craton-wide lithostratigraphic correlations for the late Archaean in Zimbabwe. Zircon ages for a syn-tectonic gneiss (2667±4 Ma) and a late syn-tectonic intrusive granodiorite (2664±15 Ma) pinpoint the age of deformation of the greenstone sequence and compare well with a Pb-Pb age of shear zone related gold mineralization (2659±13 Ma) associated with the latter intrusive phase. The intimate timing relation of greenstone deformation and granitoid emplacement, but also the metamorphic evidence for a thermal effect of the batholiths on the surrounding greenstone belts, and the structural and strain patterns in the greenstone sequence around and adjacent to the batholiths, imply that the intrusion of the granitoids had a significant influence on the tectono-thermal evolution of the greenstone belt. Prolonged magmatic activity is indicated by the zircon ages of small, post-tectonic plutons intrusive into the greenstone belt, with a mineralized granodiorite dated at 2649±6 Ma and an unmineralized tonalite at 2618± 6 Ma. The 2601±14 Ma crystallization age of an “external” Chilimanzi-type granite agrees well with existing radiometric ages for similar granites within the southern part of the craton, demonstrating a craton-wide event and heralding cratonization. The similarity between U-Pb zircon ages and T_DM model ages (2.65–2.62 Ga) and the positive ɛNd_T values (+3 to +2) for the late syn-tectonic and post-tectonic intrusive plutons within the greenstone belt indicate magmatism was derived directly from the mantle or by anatexis of lower crustal sources, with very short crustal residence times, and minor contamination with older crust. The rather high model μ₁ values (8.2–8.6) are unlikely to indicate the involvement of significant amounts of older crust and may be inherited from a high U/Pb mantle source, as was suggested by previous workers for the Archaean mantle beneath Southern Africa. The older T_DM ages for the felsic volcanics (3.0–2.8 Ga) and the porphyries (2.8–2.7 Ga) suggest that these felsic magmas were derived by partial melting of a source that was extracted from the mantle ca. 200 Ma prior to volcanism or may indicate interaction between depleted mantle-derived melts and older crustal material. Received: 15 August 1995 / Accepted: 12 January 1996     

The importance of different types of magmatism in VHMS mineralisation: evidence from the geochemistry of the host volcanic rocks to the Benambra massive sulphide deposits, Victoria, Australia

Summary The Wilga and Currawong Cu-Zn massive sulphide deposits in southeastern Australia are hosted by a deformed sequence of Upper Silurian basaltic to rhyolitic volcanic and sedimentary rocks. The syn-volcanic mineralisation occurs immediately above a thick package of rhyolitic volcanic rocks and volcaniclastic rocks (Thorkidaan Volcanics), and is overlain by relatively thin intercalated sills, intrusive domes and flows of basalt, andesite and dacite (Gibson's Folly Formation). The Thorkidaan Volcanics haveNd(420Ma) = -2.2 to - 9.8 and are considered to have been derived by partial melting of older crustal rocks, whereas the basalt-andesite-dacite hangingwall sequence has(Nd(415Ma) = -0.5 to + 2.0 suggesting derivation from a relatively undepleted mantle source. Relatively high-Ti andesitic to dacitic rocks from the Bumble Creek area haveNd(415Ma) = +5.2 to +5.9 suggesting affinities with Ordovician volcanic rocks elsewhere in the Lachlan Fold Belt. The Thorkidaan Volcanics display a limited silica range (73 to 79 wt.%), but have distinctive minor and trace element variations indicating a substantial fractionation history involving feldspar and several accessory phases. Major and trace element compositions of the basalt-andesite-dacite suite display regular variations consistent with a cogenetic relationship by fractional crystallisation. The basaltic rocks mostly have low TiO₂ (< 0.8 wt.%) and other chemical characteristics such as high Zr/Nb and La/Nb which suggest formation in a subduction-related setting; probably an embryonic back-arc basin developed on stretched continental lithosphere, or in small pull-apart basins developed adjacent to a transtensional margin. The magmatic history and paleogeography reflect an extensional tectonic and magmatic cycle comprising uplift, rhyolitic magmatism from crustal melting, extension, subsidence, and penetration of a mantle-derived basalt-andesite-dacite suite up extensional faults to the sea floor. Massive sulphide ores are located exactly at the stratigraphic change from rhyolitic to more mafic mantle-derived magma types. Consideration of the types of mineralisation associated with crustal, S-type granitoids, coupled with thermal constraints limiting the capacity of small bodies of silicic magma to initiate and sustain hydrothermal convection cells of reasonable size, suggests that in the absence of coeval mafic magmatism, S-type crustal-derived silicic volcanic packages are likely to be barren of VHMS deposits. Mineralisation occurs in association with mantle-derived basalt-andesite-dacite suites that either provide the necessary heat to facilitate leaching of the footwall volcanic rocks, or contribute metal-rich hydrothermal solutions during fractional crystallisation, or both.

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Die Bedeutung verschiedener Typen von Magmatismus für VHMS Mineralisationen: Die Geochemie der vulkanischen Nebengesteine der massiven Sulfid-Lagerstätte von Benambra, Victoria, Australien

Zusammenfassung Die massiven Cu-Zn-Sulfid-Lagerstätten von Wilga und Currawong in Südostaustralien treten in einer tektonisch beanspruchten Abfolge von obersilurischen, basaltischen bis rhyolitischen Vulkaniten und Sedimenten auf. Die syn-vulkanische Vererzung ist unmittelbar oberhalb einer mächtigen Abfolge von rhyolitischen Vulkaniten und Vulkanoklastiten (Thorkidaan Vulkanite) zu finden, darüber folgen relativ dünne wechsellagernde Ge, Intrusiv-Dome und Ergüsse von Basalt, Andesit und Dacit (Gibson's Folly Formation). Die Thorkidaan Vulkanite habenNd(420Ma) =-2,2 bis - 9,8 und dürften durch partielle Aufschmelzung älterer krustaler Gesteine entstanden sein. Die Basalt-Andesit-Dacit-Abfolge im Hangenden hat jedochNd(415Ma) = -0,5 bis + 2,0, was auf Herkunft aus einer relativ wenig verarmten Mantelquelle hinweist. Relativ Ti-reiche andesitische bis dacitische Gesteine aus dem Gebiet vom Bumble Creek zeigenNd(415) = +5,2 bis + 5,9. Dies weist auf Beziehungen mit Ordovicischen Vulkaniten in anderen Teilen des Lachlan-Gürtels hin. Die Thorkidaan Vulkanite zeigen SiO₂-Gehalte von 73 bis 79 Gew. %, und charakteristische Variationen der Haupt- und Spurenelementgehalte. Diese lassen eine signifikante Fraktionierung erkennen, an der Feldspäte und verschiedene andere Nebengemengteile beteiligt waren. Die Haupt- und Spurenelementzusammensetzungen der Basalt-Andesit-Decit-Abfolge zeigt normale Variationen, die auf co-genetische Beziehungen mit fraktionierter Kristallisation hinweisen. Die basaltischen Gesteine haben niedrige Gehalte an TiO₂ (< 0, 8 gew. %) sowie hohe Zr/Nb und La/Nb Verhältnisse, die auf Bildung in einem Subduktionsbereich, wahrscheinlich in einem embryonischen Back-Arc Becken, das sich auf ausgedünnter kontinentaler Lithosphäre oder in einem kleinen Pull-Apart Becken in der Nähe eines transtensionalen Randes entwickelt hat, hinweisen. Die magmatische Entwicklungsgeschichte und die Palägeographie weisen auf Dehnungs-Tektonik und auf einen magmatischen Zyklus hin, der Hebung,rhyolitischen Vulkanismus infolge von Krustenaufschmelzung, Extension, Absenkung und Durchdringung mit einer vom Mantel bezogenen Basalt-Andesit-Dacit-Suite entlang von Verwerfungen auf den Meeresboden erkennen läßt. Massive Sulfiderze kommen genau an der stratigraphischen Grenze von rhyolitschen zu mafischen Magmatypen mit Mantel-Ursprung vor. Hier ist es erforderlich, die Vererzungstypen, die zusammen mit krustalen S-Typ Granitoiden vorkommen, ebenso zu erwägen, wie die thermalen Aspekte, die die Fähigkeit kleiner saurer Magmenkörper limitieren, hydrothermale Konvektionszellen ausreichender Größe in Gang zu setzen und zu erhalten. Das weist darauf hin, daß bei Fehlen von gleichaltrigem mafischem Magmatismus saure vulkanische Abfolgen mit Krustenherkunft sehr wahrscheinlich keine VHMS-Lagerstätten führen können. Diese Vererzungen sind an Basalt-Andesit-Dacit-Abfolgen mit Mantelherkunft gebunden, die entweder die notwendige Wärmequelle für die Auslaugung vulkanischer Gesteine im Liegenden lieferten und/oder metallreiche hydrothermale Lösungen während fraktionierter Kristallisation verfügbar machten.