Petrological and Chemical Evolution of the Northeastern Troodos Extrusive Series, Cyprus

Four magma series are distinguished in the northeastern TroodosExtrusive Series: (A) a Lower Low-Ti Series (Lo-LTS) of basalticandesites, (B) a High-Ti Series (HTS) of basaltic andesitesto rhyodacites, (C) a Low-Ti Series(DLTS), the last two beingof basaltic andesite. Trace-element characteristics vary systematicallyfrom Series A to D and are interpreted in terms of a variablecontribution of three major source components (SCs). LILE-enrichedwater-rich fluids (SCI) derived from dehydration of a subductedlithosphere slab were continuously added to the overlying mantlewedge. Increasing LILE/HFSE and LILE/REE ratios and decreasingabsolute HFSE and REE concentrations from Series A to Dindicateprogressive depletion of the actual mantle source (SCII). Anegative Ta anomaly in the lavas decreases from Series A toD and is interpreted to have resulted from partial melting ofthe lower crust (SCII) where Ta-Nb-Ti may be fractionated byTi-rich accessory phases. The contribution of SCIII decreaseswhen the eruptive sites successively move away from the centralaxial zone and the temperature of the lower crust decreases,preventing partial melting of the lower crust. Chemical compositionsof fresh glass separates and phenocrysts indicate a change ofmajor petrogenetic processes from series A to D. Lo-LTS andIITS lavas are intrepreted to be directly related by open-systemfractional crystallization in crustal magma chambers. Removalof observed phenocryst phases clinopyroxene, orthopyroxene,plagioclase, and magnetite, and repeated subsequent mixing ofdacitc to rhyodacitic magmas with batches of replenshing basalticandesites are the major processes, possibly induced by vesicleformation in the mafic layer after a period of some crystallization.LTS and DLTS magmas were directly fed to the surface withoutstagnating at crustal levels, with feeder dykes positioned marginalto the central rift zone and thus by-passing the central magmachambers. These magmas apparently experienced only limited fractionalcrystallization of 10–15 wt.% olivine+clinopyroxene+chromite,probably at the mantle-crust boundary.     

INTEGRATED EXPLORATION FOR LOW-TEMPERATURE GEOTHERMAL RESOURCES IN THE HONEY LAKE BASIN,CALIFORNIA1

An integrated exploration study is presented to locate low-temperature geothermal reservoirs in the Honey Lake area of northern California. Regional studies to locate the geothermal resources included gravity, infra-red, water-temperature, and water-quality analyses. Five anomalies were mapped from resistivity surveys. Additional study of three anomalies by temperature-gradient and seismic methods was undertaken to define structure and potential of the geothermal resource. The gravity data show a graben structure in the area. Seismic reflection data indicate faults associated with surface-resistivity and temperature-gradient data. The data support the interpretation that the shallow reservoirs are replenished along the fault zones by deeply circulating heated meteoric waters.     

湖南会同寒武纪早期有机碳同位素地层学研究

寒武纪早期是地球海洋环境与生命演化的关键时期,但目前扬子东南缘深水相区的早寒武纪地层尚缺乏系统、精确 的地层对比工作。该文选取湖南省怀化地区会同钻孔剖面（深水相区） 的留茶坡组硅质岩、小烟溪组黑色页岩为研究对 象,进行了高分辨的有机碳同位素（δ13Corg） 地层对比,结果在会同剖面自下而上识别出四个正漂移（P1、P2、P3和P4） 与两个负漂移（N1和N2）,结合其他剖面的生物化石记录和锆石U-Pb年龄资料,将会同剖面有机碳同位素与湖南其他 剖面,以及和云南和三峡等地浅水相区剖面的有机碳、无机碳同位素曲线进行对比,认为扬子东南缘埃迪卡拉系-寒武 系界线在湖南深水相区可放置于留茶坡组上部较大的有机碳同位素负漂移（Basal Cambrian Carbon isotope Excursion, BACE） 出现的位置,但由于钻孔深度不够,所以该负漂移未在会同剖面获得,而P1、P2和P3分别对应于寒武系的ZHUCE （ZHUjiaqing Carbon isotope Excursion,第二阶）、CARE （Cambrian Arthropod Radiation isotope Excursion,第三阶） 和MICE（MIngxinsi Carbon Isotope Excursion,第四阶） 正漂移,N1 和N2 分别对应于寒武系的SHICE （SHIyantou Carbon isotope Excursion,第二阶） 和AECE（Archaeocyathid Extinction Carbon isotope Excursion,第四阶） 负漂移,因此会同剖面留茶坡组顶部至小烟溪组底部属于寒武系第二阶,小烟溪组下部属于寒武系第三阶,而小烟溪组中-上部属于寒武系第四阶,而顶 部是否达到第四阶顶部尚无法确认。碳同位素的负漂移可能是海侵时期上升流水体将底层富含12C还原水体带至浅水地区所 致,并分别与埃迪卡拉动物群、小壳化石动物群和古杯动物的灭绝密切相关;而在生物繁盛时期,海洋初级生产力升高, 有机质埋藏增加,导致碳同位素的正漂移。     

Origin of migmatites by deformation-enhanced melt infiltration of orthogneiss: a new model based on quantitative microstructural analysis

A detailed field study reveals a gradual transition from high‐grade solid‐state banded orthogneiss via stromatic migmatite and schlieren migmatite to irregular, foliation‐parallel bodies of nebulitic migmatite within the eastern part of the Gföhl Unit (Moldanubian domain, Bohemian Massif). The orthogneiss to nebulitic migmatite sequence is characterized by progressive destruction of well‐equilibrated banded microstructure by crystallization of new interstitial phases (Kfs, Pl and Qtz) along feldspar boundaries and by resorption of relict feldspar and biotite. The grain size of all felsic phases decreases continuously, whereas the population density of new phases increases. The new phases preferentially nucleate along high‐energy like–like boundaries causing the development of a regular distribution of individual phases. This evolutionary trend is accompanied by a decrease in grain shape preferred orientation of all felsic phases. To explain these data, a new petrogenetic model is proposed for the origin of felsic migmatites by melt infiltration from an external source into banded orthogneiss during deformation. In this model, infiltrating melt passes pervasively along grain boundaries through the whole‐rock volume and changes completely its macro‐ and microscopic appearance. It is suggested that the individual migmatite types represent different degrees of equilibration between the host rock and migrating melt during exhumation. The melt topology mimicked by feldspar in banded orthogneiss forms elongate pockets oriented at a high angle to the compositional banding, indicating that the melt distribution was controlled by the deformation of the solid framework. The microstructure exhibits features compatible with a combination of dislocation creep and grain boundary sliding deformation mechanisms. The migmatite microstructures developed by granular flow accompanied by melt‐enhanced diffusion and/or melt flow. However, an AMS study and quartz microfabrics suggest that the amount of melt present did not exceed a critical threshold during the deformation to allow free movements of grains.     

Temporal and spatial sedimentation rate variabilities in the eastern Gotland Basin, the Baltic Sea

The present study examines sedimentation rates in the eastern Gotland Basin using a variety of methods that reveal considerable heterogeneity in the rates, both spatially and temporally. High-resolution seismic recordings and correlation with long sediment cores indicate increased thickness of strata and higher sedimentation rates (0.75 mm a -1 ) in the eastern part of the basin than in the western part (0.23 mm a -1 ) since the Littorina transgression some 8000 14 C years BP. This difference is apparently a consequence of a counterclockwise near-bottom circulation in the basin with periodically high current speeds that cause winnowing on the steep SE slope of the basin and differential settling of sediments in areas of low current speeds. On shorter time scales, recent sediment accumulation rates based on radiometric dating ( 210 Pb) are in general twice as high as those observed 25 years ago using the same method. The higher modern rates, compared to those of the 1970s, may partly be due to increased eutrophication, as more carbon is buried in the sediment, and partly due to increased erosion in shallow water areas. However, strong lateral variations are evident. The average sediment accumulation rates vary between 119 and 340 g m -2 a -1 (corresponding to sedimentation rates of 2.1-2.5 mm a -1 ) in the deepest part of the basin. Very high rates (6100 g m -2 a -1 , corresponding to sedimentation rates of 30 mm a -1 ) are observed on an intraslope basin site (offshore Latvia) at a water depth of only 70 m. The radiometrically determined sediment accumulation rates are up to three times higher than those estimated from average water column concentrations of suspended matter and from sediment trap flux rates. The discrepancy suggests that sedimentation in the deep basin may have a substantial contribution from near-bottom lateral transport.     

Palynological and oxygen isotope investigations on Late-Glacial sediment cores from Swiss lakes

Results from detailed pollen and ¹⁸O/¹⁶O studies on two sediment profiles from small Swiss lakes are reported. ¹⁸O/¹⁶O records in lacustrine carbonate contain paleoclimatic information because they reflect mainly the isotope ratio in rain and snow which is correlated to temperature. Several transitions between different climatic periods determined palyno-logically are also indicated by marked changes in the isotope ratios in both profiles, namely the transitions Oldest Dryas - Bøiling and Allerød - Younger Dryas - Preboreal. ¹⁸o/¹⁶O was 2 to 3 %0 lower during Younger Dryas than during the adjacent periods, corresponding to a temperature drop of a few degrees Centigrade according to a tentative estimate.     

Lithological and biochemical properties in sediments of Lama Lake as indicators for the late Pleistocene and Holocene ecosystem development of the southern Taymyr Peninsula, Central Siberia

In order to evaluate the sensitivity of aquatic and terrestrial ecosystems to climatic changes, lithological (sediment structure and color, grain size, physical properties) and biochemical (TOC, TOC/TN, δ¹³C of TOC and carbonates) investigations were carried out on an 11.12 m-long sediment core from Lama Lake (Central Siberia, Putorana Plateau). According to the pollen data, the sequence represents the termination of the Pleistocene, and the entire Holocene. It is composed of highly terrigenous and stratified clays and silts. Sediment structure, grain-size distribution, carbonate contents and physical properties of the sediment indicate that glaciers were present in the catchment area of Lama Lake during the period Oldest Dryas to AllerØd. For the same time period, δ¹³C values of TOC give indications of a perennial ice cover. Since the AllerØd, organic matter accumulation has increased, caused by an increasing input of land vegetation and aquatic primary production as revealed by relations TOC contents, TOC/TN ratios and δ¹³C values of TOC. During the Holocene climatic optimum, in late Preboreal and Boreal times, biogenic primary production in Lama Lake reached its maximum and the vegetation in the catchment area changed from grassy tundra to a dense forest. From the Atlantic period to the present, small variations in δ¹³C values of TOC and TOC contents are probably related to the location of Lama Lake on the border between grass and wooded steppe, leading to responses of environmental conditions to even small changes in climate.     

Presolar silicon carbide from the Indarch (EH4) meteorite: Comparison with silicon carbide populations from other meteorite classes

Abstract— Presolar SiC from the Indarch (EH4) meteorite was studied by scanning electron microscopy (SEM), by ion probe analysis for C and Si isotopic compositions, and by static source mass spectrometry for noble gas and C isotopic compositions. The data obtained are compared to SiC data from other meteorites, especially from Murchison (CM2), for which there is the most information available. The isotopic compositions of the major elements in SiC from Indarch and Murchison are similar. Stepped combustion data suggest a mean δ¹³C for SiC from both meteorites of ～+1430%o. Silicon isotopes in Indarch and Murchison SiC also compare well. In some other important respects, however, SiC in the two meteorites are different. Morphologically, SiC from Indarch appears finer grained than SiC from Murchison and is entirely composed of submicron grains. The finer-grained nature of Indarch SiC is confirmed by its noble gas characteristics. The mean Ne-E/Xe-S ratio for bulk Indarch SiC is significantly lower than the same ratio in Murchison (625 ± 47 vs. ～3500) but is similar to that of the finest grain-size fractions (<1 μm) in Murchison. A comparison of noble gas data from SiC from several different meteorites suggests that it might be Murchison SiC, rather than Indarch SiC, that is unusual. The grain-size disparities in SiC between meteorites are difficult to explain by residue processing differences or differing parent body processing. Instead, we speculate that a grain-size sorting mechanism for SiC may have operated in the solar nebula.