Solid solutions in the system acanthite (Ag<Subscript>2</Subscript>S)–naumannite (Ag<Subscript>2</Subscript>Se) and the relationships between Ag-sulfoselenides and Se-bearing polybasite from the Kongsberg silver district,Norway, with implications for sulfur–selenium fractionation

Sulfoselenides [Ag₂(S,Se)] and Se-bearing polybasite have been discovered at the Kongsberg silver district. The selenium-bearing minerals occur in two samples from the northern part of the district, forming either single or polyphase inclusions together with chalcopyrite within native silver. The Ag-sulfoselenides show large chemical variations, covering nearly the complete compositional range between acanthite (Ag₂S) and naumannite (Ag₂Se). For the data presented here, there is no local maximum at the composition Ag₄SSe attributed to the distinct phase called aguilarite, suggesting that this composition can be considered as one of many possible along the monoclinic Ag₂S–Ag₂S_0.4Se_0.6 solid solution series rather than a specific mineral phase. We present a model explaining the variations in the Se-content of Ag₂(S,Se) as a result of gradual de-sulfidization of the rock under oxidizing conditions. During this process, sulfur from the Ag₂S-component of Ag₂(S,Se) oxidized and dissolved in the fluid phase as SO₄^2?, resulting in the formation of native silver. The activity ratio \({a_{{{\text{S}}^{2 - }}}}/{a_{{\text{S}}{{\text{e}}^{2 - }}}}\) of the system gradually decreased due to the removal of SO₄^2?, which resulted in the stabilization of a sulfoselenide with higher selenium content. As a result of reaction progress, grains of Ag₂(S,Se) became gradually enclosed in newly formed native silver, and therefore isolated from further reactions with the grain-boundary fluid. Grains isolated early during the process show low content of Se reflecting high \({a_{{{\text{S}}^{2 - }}}}/{a_{{\text{S}}{{\text{e}}^{2 - }}}}\) of the equilibrium fluid, while grains showing high Se reflect the composition of late low \({a_{{{\text{S}}^{2 - }}}}/{a_{{\text{S}}{{\text{e}}^{2 - }}}}\) fluids. Analyses of Se-bearing polybasite show that selenium is preferentially partitioned into Ag₂(S,Se) compared to polybasite. The model presented here demonstrates how oxidation of sulfoselenides leads to fractionation of sulfur and selenium.     

Geochemistry and zircon U–Pb geochronology constrains late cretaceous plagiogranite intrusions in Mersin ophiolite complex (southern Turkey).

In this study, LA-ICP-MS U–Pb zircon dating were used to determine the age of the newly discovered plagiogranite suite intruding gabbro and volcanic units of Mersin ophiolites from the Inner Tauride Belt. Obtained U–Pb zircon ages from the plagiogranite yielded crystallization ages of 93.0?±?1.5 to 94.2?±?2.4 Ma (Turonian–Cenomanian) supporting the idea of Late Cretaceous active subduction factory in the Tauride Suture Zone. The plagiogranites are mainly granodioritic, and tonalitic in composition, and contain mafic microgranular enclaves (MME) ranging from 10 to 45 cm in size. The plagiogranites are geochemically defined by low K₂O (0.02–1.03 wt%) and TiO₂ (0.17–1.88 wt%) and comparatively high Na₂O (2.3–10.2 wt%) and SiO₂ (70–78 wt%) compositions together with depletion in Ti, Ta, and Nb. The tectonomagmatic discrimination diagrams, trace, and REE-normalized multi-element patterns indicate that the plagiogranites are distinctive calc-alkaline, I-type volcanic arc granites. Plagiogranites are furthermore characterized by the diffuse presence of isotropic pseudomorphic growth of secondary calcic-amphibole (edenite and actinolite) over a pristine not preserved Ca-inosilicate. Inverse geothermobarometry models indicate a secondary amphibole genesis at ca. 600 °C and 1.5–1.7 kbar, suggesting HT-metasomatism affecting the already intruded plagiogranites. While it is already accepted that Mersin ophiolite complex is generated in a supra-subduction zone, this study represents a new contribution on the evolution of the Mersin ophiolite during the Late Cretaceous Neotethys subduction and could shed light on the genesis of plagiogranites in arc-environments.     

Energy Release During Slow Long-Duration Flares Observed by RHESSI

Slow long-duration events (SLDEs) are flares characterized by the long duration of their rising phase. In many such cases the impulsive phase is weak without typical short-lasting pulses. Instead, smooth, long-lasting hard X-ray (HXR) emission is observed. We analyzed hard X-ray emission and morphology of six selected SLDEs. In our analysis we utilized data from the RHESSI and GOES satellites. The physical parameters of HXR sources were obtained from imaging spectroscopy and were used for the energy balance analysis. The characteristic decay time of the heating rate, after reaching its maximum value, is very long, which explains the long rising phase of these flares.     

Petrogenesis of the Neogene volcanic units in the NE–SW-trending basins in western Anatolia,Turkey

The western Anatolian volcanic province formed during Eocene to Recent times is one of the major volcanic belts in the Aegean–western Anatolian region. We present new chemical (whole-rock major and trace elements, and Sr, Nd, Pb and O isotopes) and new Ar/Ar age data from the Miocene volcanic rocks in the NE–SW-trending Neogene basins that formed on the northern part of the Menderes Massif during its exhumation as a core complex. The early-middle Miocene volcanic rocks are classified as high-K calc-alkaline (HKVR), shoshonitic (SHVR) and ultrapotassic (UKVR), with the Late Miocene basalts being transitional between the early-middle Miocene volcanics and the Na-alkaline Quaternary Kula volcanics (QKV). The early-middle Miocene volcanic rocks are strongly enriched in large ion lithophile elements (LILE), have high ⁸⁷Sr/⁸⁶Sr_(i) (0.70631–0.71001), low ¹⁴³Nd/¹⁴⁴Nd_(i) (0.512145–0.512488) and high Pb isotope ratios (²⁰⁶Pb/²⁰⁴Pb = 18.838–19.148; ²⁰⁷Pb/²⁰⁴Pb = 15.672–15.725; ²⁰⁸Pb/²⁰⁴Pb = 38.904–39.172). The high field strength element (HFSE) ratios of the most primitive early-middle Miocene volcanic rocks indicate that they were derived from a mantle source with a primitive mantle (PM)-like composition. The HFSE ratios of the late Miocene basalts and QKV, on the other hand, indicate an OIB-like mantle origin—a hypothesis that is supported by their trace element patterns and isotopic compositions. The HFSE ratios of the early-middle Miocene volcanic rocks also indicate that their mantle source was distinct from those of the Eocene volcanic rocks located further north, and of the other volcanic provinces in the region. The mantle source of the SHVR and UKVR was influenced by (1) trace element and isotopic enrichment by subduction-related metasomatic events and (2) trace element enrichment by “multi-stage melting and melt percolation” processes in the lithospheric mantle. The contemporaneous SHVR and UKVR show little effect of upper crustal contamination. Trace element ratios of the HKVR indicate that they were derived mainly from lower continental crustal melts which then mixed with mantle-derived lavas (~20–40%). The HKVR then underwent differentiation from andesites to rhyolites via nearly pure fractional crystallization processes in the upper crust, such that have undergone a two-stage petrogenetic evolution.     

Influence of Neutron Star Parameters on Evolutions of Different Types of Pulsar

Influences of the mass, moment of inertia, rotation, absence of stability in the atmosphere and some other parameters of neutron stars on the evolution of pulsars are examined. It is shown that the locations and evolutions of soft gamma repeaters, anomalous X-ray pulsars and other types of pulsar on the period versus period derivative diagram can be explained adopting values of B < 10¹⁴ G for these objects if they have smaller mass (e.g. about 0.5 Solar mass) compared to the conventionally adopted values of mass. This approach gives the possibility to explain many properties of different types of pulsar.     

Evidence Linking Slow Solar Wind Streams to Long-Decay X-Ray Events

Outflow of slow solar wind from solar active regions has been reported in recent years by many different authors. Therefore, in this paper we have studied synoptic maps of the solar wind density (SWD) based on interplanetary scintillation (IPS) data for available parts of all the years 1991–1994 and 1997–2001 to verify correlations of maxima in SWD with sources in active regions. We have found convincing evidence that eruptive flares in active regions, and thus X-ray long-decay events (LDEs) in general, can produce short-lived enhancements of the SWD. However, we were not able to get statistically convincing evidence that active regions can be permanent sources of slow solar wind, and propose three possible reasons for this negative result.     

Sensitivity Tests with a One-Dimensional Boundary-Layer Mars Model

We present a series of sensitivity studies conducted using a one-dimensional Mars model (hereafter 1D model) of the University of Helsinki (UH). The reference case was the Pathfinder simulation for the second Martian day. Pathfinder temperatures and new wind speed observations from near the surface were available for validation. The Monin–Obukhov similarity parametrization for surface-layer turbulence was tested with various forms for the stability functions, and compared with the Pathfinder observations. The Dyer–Businger (DB) forms proved appropriate in the highly turbulent daytime Martian boundary layer. An iterative surface-layer treatment was introduced; this did not significantly change the results but showed that the Obukhov length L was about –30 m during daytime and +%5 m during nighttime. The importance of including water vapour and dust in the radiative transfer was tested in the Pathfinder simulations. Water vapour seems to have a significant effect, especially on the nighttime surface temperatures, by increasing the downwelling longwave radiation. Dust acts similarly and has an even greater longwave effect. It also extinguishes solar radiation strongly, thereby damping the surface temperature cycle. The sensitivity of the diurnal surface temperature variation on various physical properties of the soil (regolith) was studied. Thermal inertia and thermal conductivity had the largest effects. The Beagle 2 Lander of the European Space Agency (ESA) landed unsuccessfully on Mars at the end of the year 2003. The selected landing site was in the Northern Hemisphere tropics where seasonal variations are small, and the landing time corresponded roughly to early spring (L_s = 330°). The expected weather conditions at the site were simulated for four approximate Martian months consisting of 60 Martian solar days each. The driving conditions for the simulations were taken from the Mars climate database.     

A Geophysical Study of the Carcavai Fault Zone, Portugal

The Algarve province is located a few hundred kilometres north of the crossing of the E–W Eurasia–Africa plate boundary in an area of diffuse seismicity and broad deformation. It is characterised by a moderate seismicity, with some important historical and instrumental earthquakes causing loss of lives and significant material damages. The area is affected not only by plate boundary earthquakes but also by moderate to large events generated by local sources. The assessment of onshore local sources is, therefore, of vital importance for an evaluation of the regional seismic hazard. This paper discusses the application of geophysical data to the study of the Carcavai fault zone, an outcropping structure more than 20?km long which is seen to deform sediments of the Plio-Quaternary age. The location of some sectors of the fault zone, as well as the vertical offsets of the structure, are still to be confirmed. In order to estimate these and to study the geometry of the fault zone at depth, geophysical data were acquired together with new geological data. Where the location of the fault was less certain, EM and seismic reflection profiles with coarse spatial sampling were carried out. After the detailed location of the fault zone, seismic reflection profiles with a more dense spatial resolution were acquired. The integrated interpretation of the geological and geophysical data confirmed the presence of a large fault zone. The total fault length is still unknown as its extension offshore is still being studied. Together with estimated values of the throw obtained, this data set has improved understanding the seismic hazard in the area by providing more refined estimates of co-seismic rupture, maximum expected earthquake and return periods.     

介绍与简评《地层中地震记录(古地震)》一书

地质历史中有无地震？回答是肯定的。现代板块构造机制解决了地震的构造成因,同样地史中的板块运动也必然诱发地震。遗憾的是有关地史中地震（古地震）的报道实在是太少了,究其原因：①不认识地史中的地震记录;②缺乏有效的研究手段和方法;③忽视这一研究领域,或者将地震记录作其他成因解释。因此古地震研究就成了地质调查中的薄弱环节。     

GML&SVG的开放式WebGIS设计与应用

GML作为一种空间信息的编码、存储和交换格式,已逐渐被接受并广泛使用,为实现空间信息的共享和WebGIS的进一步发展提供了一个强有力的工具;SVG作为一种网络时代的图形文件格式标准,综合了矢量图形、位图图像和纯文本的优点,对网络环境有天然的适应性,代表未来网上图形传输发展的方向,因此,基于GML&SVG的WebGIS研究与应用具有广泛的实用价值和应用前景.文中提出了利用GML进行地理信息的存储和集成,并用SVG实现地理信息的Web显示,操作的开放式WebGIS体系结构和解决方案.且在此基础上,建立了GML&SVG的WebGIS应用系统.