太阳质子辐射和软X射线耀斑与射电爆发间的相关研究

统计分析了太阳质子事件与微波爆发和软Ｘ射线（ＳＸＲ）耀斑间的关系．结果表明：质子事件的峰值流量与微波爆发和ＳＸＲ耀斑的峰值流量、能通量间呈正的对数线性相关,相关系数０．７—０．８．根据这一统计结果和观测的微波爆发、ＳＸＲ耀斑的有关物理量,可以估算伴随的质子事件峰值流量．太阳质子辐射、ＳＸＲ耀斑和微波爆发三者间的共生关系,可以用磁环中耀斑产生的磁流体动力学过程来解释．大约３３％的质子事件没有对应的Ⅱ型爆发,这表明高能质子的加速有随机ＭＨＤ湍流加速（有Ⅱ型暴）和低频快磁声波湍动加速（无Ⅱ型暴,但有γ射线耀斑）２种不同的加速机制     

科尔沁沙地奈曼旗普通风砂土中的粘土矿物

通过对科尔沁沙地奈曼旗普通风砂土中粘土矿物的研究,结果表明这类土壤中的粘土矿物主要是伊利石,其次为高岭石、绿泥石、伊利石-蒙脱石混层矿物;它们主要来源于母质,其次来自成土过程,降尘输入量极有限。随成土过程不断进行,粘土矿物主要遵循铝硅酸盐矿物→绿泥石→绿泥石-蒙脱石→蒙脱石顺序演变。由于母质本身贫乏、成土过程较弱以及比重差异使蒙脱石有独特的搬运与沉降行为,共同造成土壤中缺乏蒙脱石。     

基于X3D的虚拟三维场景漫游系统设计与实现

X3D是新一代的互联网3D图形规范,为构建基于Web的虚拟三维场景及其人机交互提供了一种新的途径。提出了基于X3D的虚拟三维场景的建模方案,采用了地理信息系统的图层化方法将虚拟三维场景数据划分为独立地物、植被、交通、建筑物和数字地形等数据层,介绍了各数据层的三维建模及实现方法,并以一个典型的城市小区为例阐述了虚拟三维场景的优化与整合技术。     

Three‐dimensional texture of natural pseudotachylyte: Pseudotachylyte formation mechanism in hydrous accretionary complex

Melt‐origin pseudotachylyte is the most reliable seismogenic fault rock. It is commonly believed that pseudotachylyte generation is rare in the plate subduction zone where interstitial fluids are abundant and can trigger dynamic fault‐weakening mechanisms such as thermal pressurization. Some recent studies, however, have discovered pseudotachylyte‐bearing faults in exhumed ancient accretionary complexes, indicating that frictional melting also occurrs during earthquakes in subduction zones. To clarify the pseudotachylyte generation mechanism and the variation of slip behavior in the plate subduction zone, a pseudotachylyte found in the exhumed fossil accretionary complex (the Shimanto Belt, Nobeoka, Japan) was re‐focused and microscopic and three‐dimensional observations of the pseudotachylyte‐bearing fault were performed based on optical, electron, and X‐ray microscope images. Based on the patterns contained in the fragment, the pseudotachylyte is divided into four domains, although no clear domain boundaries or layering structures are not found. Three‐dimensional observation also suggests that the pseudotachylyte were fragmented or isolated by cataclasite or carbonate breccia. The pseudotachylyte was rather injected into the surrounding carbonate breccia, which is composed of angular fragments of the host rock and a matrix of tiny crystalline carbonate. The pseudotachylyte volume was extracted from the X‐ray microscope image and the heat abundance consumed by the pseudotachylyte generation was estimated at 2.18 MJ/m², which can be supplied during a slip of approximately 0.5 m. These observations and calculations, together with the results of the previous investigations, suggest hydrofracturing and rapid carbonate precipitation that preceded or accompanied the frictional melting. Dynamic hydrofracturing during a slip can be caused by rapid fluid pressurization, and can induce abrupt decrease in fluid pressure while drastically enhancing the shear strength of the shear zone. Consequently, frictional heating would be reactivated and generate the pseudotachylyte. These deformation processes can explain pseudotachylyte generation in hydrous faults with the impermeable wall rock.     

Characterizing solute transport in undisturbed soil cores using electrical and X‐ray tomographic methods

Solute transport in undisturbed soil is a complex process and detailed information on the transport characteristics is needed to provide fundamental understanding of the processes involved. X‐ray computer tomography (CT) and electrical resistivity tomography (ERT) have been used to gain information on the transport characteristics. Both methods are non‐intrusive and do not disturb the soil, in contrast to other methods. CT provides high resolution information on bulk density and macropores, while ERT provides a three‐dimensional image of the internal resistivity structure. By adding a suitable solute under steady‐state flow, the internal resistivity changes can be interpreted as a change in resident concentrations. In our experiment two cores from different field sites were investigated. The ERT measurements revealed two transport modes (one fast and one slow) in one of the cores and only one mode in the other. This was consistent with the results of transfer function modelling on the independently measured breakthrough curves (BTCs). The fast transport mode is perhaps a result of many connected macropores, detected by CT, but this could not be verified with the ERT measurements because of the coarser resolution. However, with ERT in both cases we were able to explain the observed BTC qualitatively. Copyright © 1999 John Wiley & Sons, Ltd.     

五莲县七宝山多金属矿矿化特征及地球物理地球化学特征

五莲县七宝山多金属矿位于五莲-胶南成矿带,是山东省重点勘查区和有色金属调查评价区,开展了大量工作,系统总结其多金属矿矿化特征,分析其地球物理、地球化学特征,将为开展外围找矿工作提供参考。通过总结五莲七宝山地区的重力异常特征、航磁异常特征、岩(矿)石物性特征以及地球化学特征,以及对杏山峪和红石岗矿段高精度磁测及激电中梯资料的分析对比,提出七宝山地区低阻、低磁异常带,高低阻过渡带、正负磁异常接触带附近,是找矿的重要地球物理特征标志。地球化学资料显示该区为Cu、Au、Ag等元素构成的近圆形高背景区与七宝山火山机构中心的次火山杂岩体分布范围基本一致,其他异常与已发现的多金属矿床在位置上完全吻合,说明化探异常具有效性。     

Narrow‐Line Seyfert 1 Galaxies with high‐energy sharp spectral drops: reflection‐versus absorption models

With the launch of XMM‐Newton in 1999, two Narrow‐Line Seyfert 1 Galaxies (NLS1s) have been detected (IRAS 13224–3809 and 1H 0707–495) showing sharp spectral drops at energies equal or above the neutral Fe K edge at 7.1 keV without any narrow Fe K reemission. In this paper I summarize our present knowledge on the observed properties of sharp high‐energy spectral drops. I list the problems presently arising from the reflection dominated and the optically thick disc models. Finally, I present an alternative solution which consists of a combination of the accretion disc model and the reflection dominated model. This might solve the problems of the standard accretion disc model. (© 2006 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

A scientific case for XMM‐Newton continuation

The presentations made at the workshop “XMM‐Newton: The Next Decade”, held at ESAC from 4th to the 6th of July 2007, contained an overwhelming amount of new results and well justified scientific questions that can be addressed by observations with XMM‐Newton. XMM‐Newton has over the next decade a solid scientific case. Given the high impact of X‐ray observations, XMM‐Newton operations are not only a matter for “X‐ray astrophysics”, but also of fundamental importance for astrophysics in general. (© 2008 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)