金沙江美姑河牛牛坝水电站库区泥石流对工程影响分析

金沙江美姑河牛牛坝水电站库区泥石流沟分布面积广、发生频率高;调查表明库区现有不同类型泥石流沟31条,其中属于高度危险的泥石流沟4条,中度危险的泥石流沟15条;这些泥石流不会造成严重的堵河问题。在施工期泥石流对水电站工程的影响突出,特别是靠近库首的泥石流对工程的安全构成威胁。水库蓄水后,库区泥石流对水电站工程影响有所降低,但位于大坝下游区的泥石流对水电站正常运行仍有较大的影响。     

海南岛博鳌港沉积物的沿岸输送

分析了博港沿岸沉积牧粒度参数的沿岸变化，并应用沉积物粒径趋势分析模型（GSTA模型）对沉积物运动趋势进行了分析。GSTA模型结果表明，博鳌港沿岸的泥沙在横向上表现为：万泉河口以北岸段为由海向岸运动，近期处于淤积状态；万泉河口以南岸段即玉带滩大致以NNE走向到NE走向的转折点为界，北部主要是由岸向海运动，是侵蚀岸段，而南部则主要为由海向岸运动，有少量的淤积，博鳌港沿岸泥沙输送在纵向上表现为：万泉河口以北由南向北运动，万泉河口以南，北部是由北向南运动，南部是由南向北运动，其次还运用了经验公式对GSTA结果进行了验证，得到了通过万泉河口南部（玉带滩）3个断面的沿岸漂沙量，其沿岸漂沙方向主要为南北向，以上两种分析方法得出的结果和当地的许多地貌证据基本符合，而GSTA模型在玉带滩北部泥沙纵向输运方向与经验公式计算结果所表现出的一些差异，主要是由于研究时间尺度和所用的资料特征的差异性造成的。     

Turning depths of internal tides in the South China Sea inferred from profile data

Theoretically, propagating internal tides in the ocean may reflect at turning depths, where buoyancy frequencies equal tidal frequencies, before colliding with the air-sea interface or rugged bottom topography. Globally, the internal tide lower turning depths（ITLTDs） in the open ocean have been mapped; however, knowledge of the presence of ITLTDs in the South China Sea（SCS） is lacking. In this study, 2 125 high-quality temperature-salinity profiles（including 58 deep-sea hydrographic measurements...     

海底观测网发展现状及趋势研究

文中详细研究了当前世界上最典型的海底观测网的建设发展规模、形式、设备类型以及我国海底观测网的发展现状,并对国内外海底观测网的发展趋势进行总结。对日本、加拿大、美国及欧洲的海底观测网进行了设备级研究,对我国台湾地区、东海、南海的海底观测网现状进行了研究,并讨论了国外先进观测网对我国的海底观测网建设的借鉴意义。文中总结出海底观测网发展的整体趋势为:单节点网络加速验证新型设备及传感器的水下能力;区域尺度网络用于加速多学科发展并提升灾害预警能力;而浮标平台网络作为补充,铺设在远海区域以降低阶段建设成本。     

库车坳陷下侏罗统岩石古应力场与砂岩储层性质

对库车坳陷下侏罗统野外定向岩石样品的岩石力学性质的测试结果表明,下侏罗统以压扁变形明显、拉伸变形较弱为特点。自侏罗纪以来,该区经历了至少4期古构造变形作用,其变形方式主要为近EW向的以脆性变形为主的褶皱变形作用。在平面上,该区明显地表现为东弱西强的构造挤压变形特征,并对砂岩的储层性质产生重要影响。东区平均古构造应力值为19．8～28．3MPa,对应的平均砂岩孔隙度为17．1％;西区平均古构造应力值为62．6～80．1MPa,对应的平均砂岩孔隙度为6．4％～4．6％。     

Changes in Venice Lagoon dynamics due to construction of mobile barriers

The MoSE project (construction of mobile barrier to safeguard the Lagoon of Venice) entails changes to the structure of the lagoon's inlets. This could have consequences for the areas near the inlets and for the dynamics of the lagoon ecosystem as a whole. In order to predict the effects of the proposed alterations on the hydrodynamics of the lagoon, a well-tested hydrodynamic-dispersion model was applied. Simulations were carried out considering both idealised and realistic tide and wind scenarios.     

The particle background of the <Emphasis Type="Italic">X-IFU</Emphasis> instrument

In this paper we are going to review the latest estimates for the particle background expected on the X-IFU instrument onboard of the ATHENA mission. The particle background is induced by two different particle populations: the so called “soft protons” and the Cosmic rays. The first component is composed of low energy particles (< 100s keV) that get funnelled by the mirrors towards the focal plane, losing part of their energy inside the filters and inducing background counts inside the instrument sensitivity band. The latter component is induced by high energy particles (> 100 MeV) that possess enough energy to cross the spacecraft and reach the detector from any direction, depositing a small fraction of their energy inside the instrument. Both these components are estimated using Monte Carlo simulations and the latest results are presented here.     

Preliminary assessment of the ATHENA/WFI non-X-ray background

We present a preliminary assessment of the non-X-ray background for the WFI on board ATHENA conducted at IAAT in the context of the collaborative background and radiation damage working group activities. Our main result is that in the baseline configuration originally assumed for the camera the requirement on the level of non-X-ray background could not be met. In light of the results of Geant4 simulations we propose and discuss a possible optimization of the camera design and pinpoint some open issues to be addressed in the next phase of investigation. One of these concerns the possible contribution to the non-X-ray background from soft protons and ions funneled to the focal plane through the optics. This is not quantified at this stage, here we just briefly report on our ongoing activities aimed at validating the mechanisms of proton scattering at grazing incidence.     

The Cryogenic AntiCoincidence detector for ATHENA X-IFU: a scientific assessment of the observational capabilities in the hard X-ray band

ATHENA is a large X-ray observatory, planned to be launched by ESA in 2028 towards an L2 orbit. One of the two instruments of the payload is the X-IFU: a cryogenic spectrometer based on a large array of TES microcalorimeters, able to perform integral field spectrography in the 0.2–12 keV band (2.5 eV FWHM at 6 keV). The X-IFU sensitivity is highly degraded by the particle background expected in the L2 orbit, which is induced by primary protons of both galactic and solar origin, and mostly by secondary electrons. To reduce the particle background level and enable the mission science goals, the instrument incorporates a Cryogenic AntiCoincidence detector (CryoAC). It is a 4 pixel TES based detector, placed < 1 mm below the main array. In this paper we report a scientific assessment of the CryoAC observational capabilities in the hard X-ray band (E > 10 keV). The aim of the study has been to understand if the present detector design can be improved in order to enlarge the X-IFU scientific capability on an energy band wider than the TES array. This is beyond the CryoAC baseline, being this instrument aimed to operate as anticoincidence particle detector and not conceived to perform X-ray observations.     

基于RS和GIS的松花江流域植被覆盖动态变化研究

利用遥感和地理信息系统技术对1989,1995年的Landsat TM数据和2002年Landsat ETM＋三期遥感数据进行处理,反演和计算松花江流域的归一化植被指数（NDVI）,在此基础上,获取研究区域植被覆盖度。在ArcGIS9.2软件空间分析模块的支持下,对研究区域三期植被覆盖影像进行叠加分析,以流域尺度和栅格尺度分析植被覆盖变化的时间和空间特性,获取研究区域植被覆盖度空间格局分布特征,为该区域植被覆盖度的自动化监测提供很好的技术支持。