Disk wind in young binaries and its impact on the infrared excesses of young stars

We consider the effect of binarity of young stars on the spectral energy distribution of the IR radiation from circumstellar dust. The formation of a common dust envelope in a binary system with a low-mass secondary component is strongly affected by the disk wind from the secondary. The small velocities in peripheral areas of the wind are such that it can be partially or entirely captured by the primary, even when the distance between the components is up to several astronomical units. As a result, an envelope with a rather complex spatial and kinematic structure is formed. Its mass is many orders of magnitude smaller than that of the accretion disk around the binary. However, the thermal radiation emitted by dust particles of the envelope can be comparable to the total radiation of the accretion disk. This result is discussed in the context of the deficit at near-IR wavelengths (2–10µm) in current models for accretion disks around young stars.     

Application of infrared spectroscopy for rapid petroleum source rock evaluation

This paper demonstrates the utility of infrared (IR) spectroscopy for rapid routine analysis of rock extracts for the purpose of evaluating the composition of petroleum generated in any given sedimentary sequence penetrated during exploratory drilling. Specifically, ratios of the areas of the IR absorption bands (obtained by planimetry) have been used to estimate both the quality and thermal maturity of the organic matter in the corresponding rock samples. Based on the cross-plots of some of the ratios of the areas of the IR absorption bands, evolution pathways which group the organic matter into source related groups have been proposed.     

Influence of artificial channels on the source and extent of saline water intrusion in the wind tide dominated wetlands of the southern Albemarle estuarine system (USA)

Saline water intrusion is degrading water quality in the channelized coastal wetlands of the southern Albemarle estuarine system (AES). The source, transport and fate of the saline water in the southern AES was determined by monitoring specific conductivity and water levels in small artificial channels, the Alligator River, the Alligator–Pungo Canal and the groundwater system for ~12 months. Results indicate that water levels are affected by wind tides which trigger the movement of saline water into the interior of the wetlands via the small canals. The wind tides are mostly driven by episodic southerly winds pushing saline water into the canal network and the groundwater regime proximal to the Alligator River. The saline waters persist in the canals as long as the wind tide events last. Specific conductivities from canals and groundwater are shown to be unexpectedly higher closer to the source of the Alligator River than toward the Albemarle Sound, suggesting that the large Alligator–Pungo Canal facilitates the northward migration of saline water from the Pamlico Sound to the Alligator River. Overwash and reversals in the flow directions between groundwater and surface water bodies suggest that saline water that is present during wind tide events may migrate into the groundwater system from surface water bodies. The results of this study reveal that whereas the large Alligator–Pungo Canal channels saline water to the AES, small artificial channels may also play significant roles in degrading water quality in the interior of channelized coastal wetlands.     

Is there a stellar wind in the BM Ori system?

The IUE spectra of BM Ori show SiIV and CIV absorption lines, which are shifted by ?69 km/s relative to the photospheric lines of a star and do not change their position with the orbital phase of the primary. These satellite lines cannot form in a stellar wind, and probably originate in an ionized gas cloud or microjet located in the line of sight. No satellite lines were found for other bright stars of the Orion Trapezium.     

第二类越补非稳定流水文地质参数简化求解

第二类越流补给非稳定流条件下水文地质参数求解为涉及3个未知数的超越方程,常规的解析法无法直接获解。本文采用优化拟合方法,在工程适应参数范围内,用较为简单的函数实现了对由图表给出的第二类越流补给非稳定流井函数数值关系的替代,并利用水位降深比值关系经整理获得了仅含1个未知量的表达式,经简单试算即可完成参数求解,计算过程简捷,不依赖图表,便于实际工程应用。     

An H<Subscript>2</Subscript>O maser in the infrared source IRAS 20126+4104

Results of monitoring of H₂O maser in the infrared source IRAS 20126+4104, which is associated with a cool molecular cloud, are presented. The observations were carried out on the 22-meter radio telescope of the Pushchino Radio Astronomy Observatory (Russia) between June 1991 and January 2006. The spectrum of the H₂O maser emission extends from ? 16.7 to 4.8 km/s and splits into separate groups of emission features. Cyclic variations of the integrated maser flux with a period from 3.4 to 5.5 years were detected, together with strong flares of up to 220 Jy in individual emission features. It is shown that large linewidths in periods of high maser activity are due to small-scale turbulent motions of the material. An expanding envelope around a young star is accepted as a model for the source. The protostar has a small peculiar velocity with respect to the molecular cloud (～2 km/s). Individual emission features form organized structures, including multi-link chains.     

地下水源热泵水井泵砂与堵塞原因分析

地下水源热泵系统常会出现抽水井泵砂、抽水井和回灌井堵塞等问题,影响系统的正常运行或系统效率。以湖北省荆州市某地下水源热泵工程为例,分析了江汉平原广泛分布的卵砾石夹细砂含水层中成孔方法选择、滤料及过滤管设计中存在的问题;指出了目前在过滤管外包不锈钢丝网是防止在细砂层中水井泵砂的有效手段之一,但宜与泥浆密度轻、对地层污染小的反循环成孔工艺配合使用,且仍要根据含水层的颗粒级配曲线选择滤料,发挥滤料的过滤作用,避免过滤压力转移到包网过滤管,以减少抽水井堵塞。     

Local Ranking of Geological Conceptual Models in Non-stationary Settings Using Multi-point Geostatistics

Mathematical Geosciences - In geomodeling, it is commonly accepted that the distribution of physical properties is controlled by the architecture of geological objects. However, insufficient data...     

Three-dimensional hydrodynamical modeling of mass transfer in the close binary system β Lyr with an accretor wind

We present three-dimensional hydrodynamical modeling of mass transfer in the close binary system β Lyr taking into account explicitly radiative cooling and the stellar wind of the accretor. Our computations show that flow forces wind out from the orbital plane, where an accretion disk with a radius of 0.4–0.5 and a height of about 0.15–0.17 (in units of orbital separation) is formed. Gas motions directed upward from the orbital plane are initiated in the region of interaction of the flow from L₁ and the accretor wind (x = 0.91, y = ?0.17); i.e., a jetlike structure forms. This structure has the shape of a gas pillar above the orbital plane, where gas moves with the velocity of stellar wind. The number density of the gas in this structure is about 10¹⁴ cm^?3, and its temperature is 20 000–45 000 K. At heights of about 0.15–0.20 above the orbital plane, in the region between the jetlike structure and the disk, two spiral shocks form. It is possible that the emission lines observed in the spectrum of β Lyr binary originate in this region.     

基于非平稳时间序列分析的滑坡变形预测

滑坡的位移监测资料通常可用来预测滑坡的变形发展趋势,位移的发展反映了滑坡的变形过程.为了预测在现有条件持续情况下的滑坡变形趋势,将滑坡位移监测数据视为非平稳时间序列,应用时间序列分析方法,建立了滑坡变形趋势的预测模型.以三峡库区秭归县白水河滑坡为例,通过对变形预警区监测点位移实测时间序列的分析,取监测点ZG93和XD-04为代表,建立了时间序列预测模型,从第17个月开始向前做6步预测,分析预测曲线与实测曲线之间的关系,并计算预测误差,结果显示除个别数据点之外,预测误差均在±9%以内,曲线吻合较好,说明所建模型效果良好,从而为判断白水河滑坡未来的变形发展趋势提供了可靠的理论依据.     

局部冲刷对风机支撑系统承载性能的影响

海上风力发电作为一种绿色能源越来越受到重视,单桩基础局部冲刷的研究受到广泛关注。建立了不同冲刷深度的海上风机系统模型,对各模型进行静力、动力分析。结果与前人冲刷模型试验吻合,随着桩基冲刷深度的增大,支撑系统的最大水平位移、最大水平应力和最大弯矩值逐渐增加。冲刷深度为两倍桩径时,最大水平位移、应力及弯矩分别比无冲刷条件下增加了3.61%、12.7%、10.3%。风机系统的自振频率随冲刷深度的增加而降低,高阶频率更易受影响。桩基冲刷对风机系统的动力特性有显著影响,塔顶水平位移时程曲线随冲刷深度不断上移。海上风机设计时必须考虑冲刷对支撑系统承载性能的影响。     

济阳坳陷石炭二叠系埋藏条件及煤型气源岩分布特征

山东地区经历了多次构造运动,含煤地层遭受严重破坏,因此各地煤系保存程度差异较大。济阳坳陷是石炭—二叠系的深陷区,但济阳坳陷构造十分复杂,煤系保存于坳陷中的一些次级凹陷中。石炭二叠系的埋深多在30 0 0~5 0 0 0m范围内,次级凹陷局部出现较大的埋深变化,最大埋深可达上万米,最小埋深仅在千米左右。煤型气源岩主要为煤层和暗色泥质岩。泥质岩最厚为5 5 5.5m (惠民凹陷),煤层最厚4 0.5m (车镇凹陷),泥岩、煤层厚度分布与残留厚度的变化趋势大体一致。研究表明,济阳坳陷石炭二叠系煤层属较好的烃源岩,泥岩整体上为差—中等烃源岩,局部发育有好的烃源岩。     

Study on ground source heat pump system zoning and methods in the Northwest of Shandong Province

Based on the basic geology, hydrogeology, engineering geology, geothermal geology and ground source heat pump(GSHP) engineering of the work space, the thesis studies the local shallow geothermal energy. Three conditions of the attribute index for the suitability zoning of the northwest of Shandong are determined, namely, hydrodynamic condition, geological and hydrogeological condition and geological environment condition. The assessment result is that the total area of the suitable zone is 205.88 km~2, that of relative suitable zone, 1 407.76 km~2, and that of unsuitable zone, 286.8 km~2. The result conforms to the real development situation and provides experience for similar regions needed for selecting and assigning a value to suitability zoning of GSHP.     

A multiple scale modeling system for coastal hurricane wind damage mitigation

Hurricane wind damage constitutes the largest percentage of catastrophic insured losses in the US. Yet the complicated wind structures and their changes are not fully understood and, thus, have not been considered in current risk catastrophic models. To obtain realistic landfall hurricane surface winds, a large eddy simulation (LES) framework in a weather forecasting mode has been developed from a multiple nested Weather Research & Forecasting (WRF) model to explicitly simulate a spectrum of scales from large-scale background flow, hurricane vortex, mesoscale organizations, down to fine-scale turbulent eddies in a unified system. The unique WRF-LES enables the high resolution data to be generated in a realistic environment as a hurricane evolves. In this paper, a simulation of the landfalling Hurricane Katrina is presented to demonstrate various features of the WRF-LES. It shows that the localized damaging winds are caused by the large eddy circulations generated in the hurricane boundary layer. With a sufficient computational power, WRF-LES has the potential to be developed into the next generation operational public wind-field model for hurricane wind damage mitigation.     

Velocity field of the stellar wind of the wolf-rayet star in the V 444 Cyg binary system: A parametric model

An analysis of the λ4244 Å continuum light curve of the eclipsing variable V444 Cyg is used to reconstruct the velocity law v(r) of the stellar wind of the WR star in terms of Lamers parametric and powerlaw models. Both models are inconsistent with the observed light curve, and can be rejected at the <2% significance level. Departures of the Lamers parametric relation from the empirical v(r) law reconstructed in previous papers from the same λ 4244 Å light curve on sets of concave and convexo-concave functions are statistically significant. The stellar wind of the WN5 star continues to accelerate at a considerable distance from the star’s center. This corresponds to an acceleration parameter β>1 in terms of a coarse Lamers-law approximation for the empirical v(r) field.     

An overview on source rocks and the petroleum system of the central Upper Rhine Graben

International Journal of Earth Sciences - The petroleum system of the Upper Rhine Graben (URG) comprises multiple reservoir rocks and four major oil families, which are represented by four distinct...