当前地震台站财务管理工作之浅见

本文简要介绍了台站财务管理的现状 ,针对目前台站管理中出现的一些问题 ,阐明加强台站财务管理与会计核算改革的必要性 ,并粗略提出地震台站财务管理工作的改革方向与对策。     

The “unrevealed casualties” of the Irish mortgage crisis: Analysing the broader impacts of mortgage market financialisation

Since 2008, extensive research has examined the impacts of mortgage market financialisation, particularly the socio-spatial patterns of mortgage defaults and foreclosures. However, these standard statistical indicators of mortgage difficulty only capture the ‘overt casualties’ of the crisis, overlooking the mass of households who meet their mortgage commitments, but do so at considerable cost to quality of life. The impacts of the crisis on these ‘unrevealed casualties’ has received insufficient attention within the literature. As such, this article develops a framework to assess mortgage stress levels using standard and atypical indicators of mortgage payment difficulty. This framework differentiates between the ‘overt’ and ‘unrevealed’ casualties and is applied through a case study of suburban Dublin mortgagors to examine the characteristics of these groups, determine the key factors driving their mortgage stress and assess how their attitudes towards homeownership are being reshaped. The results suggest the impact of the mortgage crisis is much larger than previously considered, affecting a more diverse range of suburban households, many of whom may be one financial or non-financial trigger event away from developing a more serious payments problem. Banks’ reckless lending practices are among the strongest predictors of mortgage stress, demonstrating how the failure to adequately regulate banking practices has had detrimental financial impacts for households at the suburban scale. Attitudes toward homeownership and its investment function are increasingly negative, demonstrating how the primary rationale for homeownership expansion (i.e. its potential for wealth creation) is being revaluated by mortgaged households in the wake of the crash.     

国际油气井钻头进展概述 (四)——PDC钻头发展进程及当今态势（下）

近年来,非平面PDC切削齿,如浅凹面PDC齿、Stinger毒牙中心锥形齿、Stinger毒牙刀翼锥形齿、AxeBlade斧式脊形PDC齿和StayCool保持冷却PDC齿等制造的钻头,逐步在油气钻井中得到有效的应用。这些钻头能够以较高的钻进效率和工作寿命钻进某些硬岩和研磨性地层。为了满足水平钻井,特别在页岩气水平井中能够强力排除岩屑,并具有优良的钻井导向性能,国际著名公司推出了许多新型钻头,如ONXY Ⅱ矛式PDC钻头、Seeker导向PDC钻头、CounterForce反力PDC钻头、Speed快速PDC钻头等用于当代油气钻井,取得了良好的效果。文章还介绍了Defyer DPA套管钻头与CuttPro PDC防剪切保护帽。提出了以下建议：继续深入研究PDC钻头,以提高其性能,更好地满足油气钻井的要求;组合化钻头是油气钻头发展的重要趋势;比金刚石性能更好的钻头切削材料有可能今后发现或合成,可用于制作更佳钻井钻头;我国钻头企业需重组和发展状大;各种钻头技术创新应该加强。     

Viscous liquid film flow on dune slopes of Mars

It is shown that viscous liquid film flow (VLF-flow) on the surfaces of slopes of martian dunes can be a low-temperature rheological phenomenon active today on high latitudes. A quantitative model indicates that the VLF-flows are consistent with the flow of liquid brines similar to that observed by imaging at the Phoenix landing site. VLF-flows depend on the viscosity, dynamics, and energetics of temporary darkened liquid brines. The darkening of the flowing brine is possibly, at least partially, attributed to non-volatile ingredients of the liquid brines. Evidence of previous VLF-flows can also be seen on the dunes, suggesting that it is an ongoing process that also occurred in the recent past.     

On China’s growing geo-economic influence and the evolution of variegated capitalism

China’s growing geo-economic clout globally has attracted significant research attention over the past few years. Rather than strictly adopt a national-specific and path-dependent perspective, this paper offers a nuanced perspective on the rationale of Chinese economic expansions overseas. I propose we view China’s growing geo-economic influence as a relational development, inextricably connected to broader changes in global capitalism, especially the failure of the US government to maintain confidence in the dollar. The paper probes critically the underlying logics of two recent developments: (1) the role of the China Investment Corporation (a new sovereign wealth fund) and state-owned enterprises (SOEs) in accessing new markets worldwide; and (2) the policies to extend the global reach of the Chinese yuan. I argue that these phenomena are concatenated to China’s broader aim to secure domestic economic security, given its vast holdings of dollar reserves and its macroeconomic constraints through the maintenance of a fixed foreign exchange regime. These developments in turn contour and sustain the evolution of the variegated global system of capitalism.     

Achieving additional emission reductions under a cap-and-trade scheme

Over the last decade, cap-and-trade emissions schemes have emerged as one of the favoured policy instruments for reducing GHG emissions. An inherent design feature of cap-and-trade schemes is that, once the cap on emissions has been set, no additional reductions beyond this level can be provided by the actions of those individuals, organizations and governments within the covered sectors. Thus, the emissions cap constitutes an emissions floor. This feature has been claimed by some to have undesirable implications, in that it discourages ethically motivated mitigation actions and preempts the possibility that local, state and national governments can take additional mitigation action in the context of weak national or regional targets. These criticisms have become prominent in Australia and the US within the public debate regarding the adoption of an emissions trading scheme (ETS). These criticisms and their potential solutions are reviewed. A set-aside reserve is proposed to automatically retire ETS permits, which would correspond to verified and additional emissions reductions. This minimizes the possibility that ethically motivated mitigation actions are discouraged, allows for additional action by other levels of government, while providing transparency to other market participants on the level of permit retirements.     

Incorporation of argon, krypton and xenon into clathrates on Mars

Calculations of the trapping of heavy noble gases within multiple guest clathrates under Mars-like conditions show that a substantial fraction of the martian Xe, perhaps even the vast majority, could be in clathrates. In addition, the Xe/Kr ratio in the clathrates would probably be much higher than in the atmosphere, so the formation or dissociation of a relatively small amount of clathrate could measurably change the atmospheric ratio. Relatively crude (factor of 2) measurements of the seasonal variability in that ratio by in situ spacecraft would be sensitive to ∼10% of the seasonal atmospheric CO₂ variability being a result of clathrates, rather than pure CO₂ frost. In addition, sequestration of Xe in clathrates remains a viable mechanism for explaining the variable Xe/Kr ratios seen in different suites of martian meteorites.     

Climate, weather, and north polar observations from the Mars Reconnaissance Orbiter Mars Color Imager

The Mars Reconnaissance Orbiter observes Mars from a nearly circular, polar orbit. From this vantage point, the Mars Color Imager extends the ∼5 Mars years record of Mars Global Surveyor global, visible-wavelength multi-color observations of meteorological events and adds measurements at three additional visible and two ultraviolet wavelengths. Observations of the global distribution of ozone (which anti-correlates with water vapor) and water ice and dust clouds allow tracking of atmospheric circulation. Regional and local observations emphasize smaller scale atmospheric dynamics, especially those related to dust lifting and subsequent motion. Polar observations detail variations related to the polar heat budget, including changes in polar frosts and ices, and storms generated at high thermal contrast boundaries.     

Hydrogen content of sand dunes within Olympia Undae

Neutron currents measured using the Mars Odyssey Neutron Spectrometer, seasonally varying temperatures measured using the Thermal Emission Spectrometer, and visible images measured using the High Resolution Imaging Science Experiment (HiRISE) are studied to determine the water content and stratigraphy of Olympia Undae. Both the neutron and thermal infrared data are best represented by a two-layered model having a water-ice equivalent hydrogen content of 30±5% in a lower semi-infinite layer, buried beneath a relatively desiccated upper layer that is 9±6 g/cm² thick (about 6 cm depth at a density of 1.5 g/cm³). A model that is consistent with all three data sets is that the dunes contain a top layer that is relatively mobile, which overlays a niveo-aeolian lower layer. The geomorphology shown by the HiRISE images suggests that the bottom layer may be cemented in place and therefore relatively immobile.     

PFS/MEX observations of the condensing CO2 south polar cap of Mars

The condensing CO₂ south polar cap of Mars and the mechanisms of the CO₂ ice accumulation have been studied through the analysis of spectra acquired by the Planetary Fourier Spectrometer (PFS) during the first two years of ESA's Mars Express (MEX) mission. This dataset spans more than half a martian year, from Ls∼330° to Ls∼194°, and includes the southern fall season which is found to be extremely important for the study of the residual south polar cap asymmetry. The cap expands symmetrically and with constant speed during the fall season. The maximum extension occurs sometime in the 80°-90° Ls range, when the cap edges are as low as −40° latitude. Inside Hellas and Argyre basins, frost can be stable at lower latitudes due to the higher pressure values, causing the seasonal cap to be asymmetric. Within the seasonal range considered in this paper, the cap edge recession rate is approximately half the rate at which the cap edge expanded. The longitudinal asymmetries reduce during the cap retreat, and disappear around Ls∼145°. Two different mechanisms are responsible for CO₂ ice accumulation during the fall season, especially in the 50°-70° Ls range. Here, CO₂ condensation in the atmosphere, and thus precipitation, is allowed exclusively in the western hemisphere, and particularly in the longitudinal corridor of the perennial cap. In the eastern hemisphere, the cap consists mainly of CO₂ frost deposits, as a consequence of direct vapor deposition. The differences in the nature of the surface ice deposits are the main cause for the residual south polar cap asymmetry. Results from selected PFS orbits have also been compared with the results provided by the martian general circulation model (GCM) of the Laboratoire de Météorologie dynamique (LMD) in Paris, with the aim of putting the observations in the context of the global circulation. This first attempt of cross-validation between PFS measurements and the LMD GCM on the one hand confirms the interpretation of the observations, and on the other hand shows that the climate modeling during the southern polar night on Mars is extremely sensitive to the dynamical forcing.