Emerging and Decaying Magnetic Flux and Subsurface Flows

We study the temporal variation of subsurface flows of 788 active regions and 978 quiet regions. The vertical-velocity component used in this study is derived from the divergence of the measured horizontal flows using mass conservation. The horizontal flows cover a range of depths from the surface to about 16 Mm and are determined by analyzing about five years of GONG high-resolution Doppler data with ring-diagram analysis. We determine the change in unsigned magnetic flux during the disk passage of each active region using MDI magnetograms binned to the ring-diagram grid. We then sort the data by their flux change from decaying to emerging flux and divide the data into five subsets of equal size. The average vertical flows of the emerging-flux subset are systematically shifted toward upflows compared to the grand average values of the complete data set, whereas the average flows of the decaying-flux subset show comparably more pronounced downflows especially near 8 Mm. For flux emergence, upflows become stronger with time with increasing flux at depths greater than about 10 Mm. At layers shallower than about 4 Mm, the flows might start to change from downflows to upflows, when flux emerges, and then back to downflows after the active regions are established. The flows in the layers between these two depth ranges show no response to the emerging flux. In the case of decaying flux, the flows change from strong upflows to downflows at depths greater than about 10 Mm, whereas the flows do not change systematically at other depths. A cross-correlation analysis shows that the flows in the near-surface and the deeper layers might change about one day before flux emerges. The flows associated with the quiet regions fluctuate with time but do not show any systematic variation.     

Interpreting Helioseismic Structure Inversion Results of Solar Active Regions

Helioseismic techniques such as ring-diagram analysis have often been used to determine the subsurface structural differences between solar active and quiet regions. Results obtained by inverting the frequency differences between the regions are usually interpreted as the sound-speed differences between them. These in turn are used as a measure of temperature and magnetic-field strength differences between the two regions. In this paper we first show that the “sound-speed” difference obtained from inversions is actually a combination of sound-speed difference and a magnetic component. Hence, the inversion result is not directly related to the thermal structure. Next, using solar models that include magnetic fields, we develop a formulation to use the inversion results to infer the differences in the magnetic and thermal structures between active and quiet regions. We then apply our technique to existing structure inversion results for different pairs of active and quiet regions. We find that the effect of magnetic fields is strongest in a shallow region above 0.985R _⊙ and that the strengths of magnetic-field effects at the surface and in the deeper (r<0.98R _⊙) layers are inversely related (i.e., the stronger the surface magnetic field the smaller the magnetic effects in the deeper layers, and vice versa). We also find that the magnetic effects in the deeper layers are the strongest in the quiet regions, consistent with the fact that these are basically regions with weakest magnetic fields at the surface. Because the quiet regions were selected to precede or follow their companion active regions, the results could have implications about the evolution of magnetic fields under active regions.     

直线形单排管冻土帷幕平均温度计算方法

冻土帷幕平均温度是人工地层冻结工程设计、施工和安全管理的重要参数.为了确定单排管冻土帷幕的平均温度,进而确定冻土的力学参数和冻土帷幕的承载能力,为冻土帷幕的安全状态作出评价.以单排管冻土帷幕温度场的巴霍尔金解析解为基础,建立了直线形单排管冻土帷幕的平均温度的两种计算模型——等效梯形法和等效三角形法模型,该模型以冻土帷幕某一横截面厚度上的等效梯形法或等效三角形法计算的平均温度来等效整体冻土帷幕的平均温度.在实际工程中可能出现的冻结管平面布置参数变化范围中,全面考察了冻土帷幕平均温度等效梯形法和等效三角形法计算结果与依据巴霍尔金解析解数值积分计算结果的误差.结果表明,等效梯形法和等效三角形法计算的冻土帷幕平均温度误差很小,优于流行的计算方法.     

Structure and evolution of a Messinian mixed carbonate‐siliciclastic platform: the role of evaporites (Sorbas Basin,South‐east Spain)

The Sorbas Member is a late Messinian complex sedimentary system that formed immediately following deposition of the Messinian evaporites in the Sorbas Basin (South‐east Spain). This work describes the sequence architecture and facies organization of a continuous kilometre long, alluvial fan to open platform transect near the village of Cariatiz in the north‐east of the basin. The post‐evaporitic Cariatiz platform was a mixed carbonate‐siliciclastic system composed of four intermediate‐frequency, fifth‐order depositional sequences (Depositional Sequences 1 to 4) arranged in an overall prograding trend. The intense fracturing and brecciation of these deposits is attributed to the deformation and dissolution of an evaporite body measuring several tens of metres in thickness. The four sequences display significant spatial–temporal variability in both architecture and facies distribution, with two main phases: (i) Depositional Sequences 1 and 2 are ooid and oobioclastic dominated, and show normal marine faunas; and (ii) Depositional Sequences 3 and 4 show a higher siliciclastic contribution and are microbialite dominated. These important changes are interpreted as modifications of the primary controlling factors. Following an initial 70 m drowning, possibly linked to increased oceanic input, Depositional Sequences 1 to 3 were controlled mainly by eustatic variations and inherited topography; their progradation destabilized the evaporite body near the end of the Depositional Sequence 2 period. During the second phase, Depositional Sequences 3 and 4 recorded a progressive restriction of the Sorbas Basin related to a 30 to 40 m fall in water level that was driven mainly by regional factors. These regional factors were dissolution and gravity‐induced deformation of the evaporites and correlative evaporative fluid circulation associated with the contrasted arid/humid regional climate that, respectively, controlled sequence geometry and fluctuating water salinity which caused a microbialite bloom.     

振动切喷技术在重庆草街航电枢纽工程中的应用

在振动切刀下部安装有定喷的喷嘴,振动切槽之前,超前进行定喷,将振动切槽与定喷两种工艺综合成一种工艺,构成一种新的薄防渗墙的施工工艺——振动切喷技术。介绍了该新技术在重庆草街航电枢纽工程中的应用情况,实践证明,此工艺提高了防渗墙的施工效率与成墙质量。     

浩布高矿区复杂地层钻进护壁堵漏技术

介绍了浩布高矿区复杂地层钻进中所采取的护壁堵漏技术措施。根据岩层及孔深情况采用了套管护壁堵漏、冲洗液护壁堵漏、水泥封孔护壁堵漏等措施,在实际工作中均收到了较好的效果。套管护壁堵漏简洁、护壁安全可靠;冲洗液护壁堵漏所用的人工钠土低固相泥浆对孔内坍塌、掉块具有较高的抑制功能;水泥封孔护壁堵漏效果好。套管护壁堵漏及水泥封孔护壁堵漏为绳索取心使用无固相钻井液钻进创造了条件,能有效地提高钻进效率。施工中根据钻孔实际情况所采取相应的堵漏措施,收到了良好的效果。     

注浆护壁堵漏工艺在深孔岩心钻探中的应用

简述了深孔岩心钻探破碎岩层护壁堵漏的重要性,注浆参数选择,水泥浆配比、速凝剂掺量的掌握,注浆施工中需把握的几个技术环节及注意事项,注浆施工经验总结及注浆效果评价等。     

白水煤矿煤矸石基本性能研究与分析

通过对白水煤矿煤矸石进行外观分类、化学组成、矿物成分分析和X衍射分析将其分为5种不同外型的煤矸石,其中,第Ⅲ类矸石属于高岭石质矸石黏土岩类矸石,其矿物相主要包括石英、高岭石、伊利石和少量的黄铁矿。实验研究不同类别矸石的粒径范围、陈化时间等对原材料塑性的影响表明:降低原料最大粒径,可以提高塑性,当粒径从-1.0 mm降低到-0.1 mm时,Ⅰ类矸石塑性指数IP提高了6.9;Ⅱ类矸石的IP提高了10.8;Ⅲ类矸石的IP提高了5.6;延长陈化时间,可以提高煤矸石的塑性,当陈化时间3 d时,陈化时间对塑性的贡献明显,当陈化时间4 d,陈化时间对塑性的贡献甚小。据此认为除第Ⅲ类煤矸石不适合制砖以外,其他矸石均可作为制备绿色墙体保温砌块的原材料,混合破碎至-0.5 mm,陈化3天,适合制备绿色墙体保温砌块的需要。     

泰安市岩溶地面塌陷的特征及其成因模式分析

岩溶地面塌陷是岩溶地区因岩溶作用而产生的地面变形现象,是岩溶洞隙上方的岩土体在自然及人为作用下发生变形破坏、并导致地面形成塌陷坑（洞）的一种岩溶地质作用。当它发生于人类活动地区时,就可破坏土地及其附属物,并危及人类生命及财产安全,从而形成地质灾害。就岩溶地面塌陷的特征及其成因模式进行了分析研究,对进一步控制塌陷的发生有重大意义。     

PS-InSAR技术在北京采空塌陷区地表形变测量中的应用探析

本文从采空塌陷区地表形变监测手段入手,分析传统形变监测手段(如水准、GPS、常规D-InSAR等)的不足,详细介绍了PS-InSAR技术原理、优缺点及应用现状。最后通过总结北京地区采空塌陷变形特征,并针对PS-InSAR技术的特点和局限性进行可行性分析,最终提出门城镇地区适宜采用PS-InSAR技术进行地表形变监测。