新建蒲虹公路过湿路基的换填施工技术研究

基于浦虹公路区域地质、构造、降雨和工程特征的分析,针对不同特点的过湿路段施用不同的换填方案.并相应地制定施工工艺、工艺流程和操作要点.实际工程表明.该换填施工技术符合相应的设计和规范要求,效果良好.     

华北地区砂性土的卸荷回弹试验研究

超采深层地下水引起的地面沉降、地裂缝等灾害已经成为华北地区大中城市的主要地质灾害。本文以华北地区地下水开采漏斗边缘的砂性土为研究对象,通过反复加荷卸荷试验,分析了砂性土的卸荷回弹特征,阐述了砂土并不是完全弹性的,它同样存在一定的塑性特征,并且说明了砂土的回弹量的大小是个变量,其回弹能力随着反复回弹次数、回弹应力大小及哪一应力进行回弹而变化。该研究结果对治理开采深层地下水引起的地面沉降等灾害有重要意义。     

Algorithms for automatic,real-time tsunami detection in wind–wave measurements Part I: Implementation strategies and basic tests

Several, although not all, wind–wave gages are equipped with sensors capable of detecting sea-level oscillations within the tsunami frequency band. The present paper looks at the algorithms to be implemented in the software of these gages in order to automatically perform the real-time detection of a possible tsunami within recorded signals. In particular, a new algorithm is proposed and tested. The first part of the paper concentrates on the algorithms' characteristics, implementation strategies and basic testing. First of all, the situations in which wind–wave measurements are either essential, or useful for real-time tsunami detection are discussed. In the second place, already existing algorithms are recalled, specifying their characteristics and fields of application. Then, the characteristics of the new proposed algorithm – mainly based on an infinite impulse response, time domain filter – are illustrated and analyzed. Performance and efficiency of the considered algorithms are compared using synthetic time series. The second part of the paper discusses the algorithms' use in the framework of Tsunami Early Warning Systems (TEWS), testing them in actual cases.     

X-ray binary unified analysis: pulse/RV application to Vela X1: GP Velorum

A procedure for simultaneous analysis of multiple kinds of observations is developed for binaries that contain X-ray pulsars. A wide variety of observation types might be included, although we consider only velocity: pulse and light: velocity: pulse cases at present. The model operates with equipotentials and can accommodate non-synchronous rotation and eccentric orbits. The duration condition imposed by observed X-ray eclipses is incorporated as an embedded constraint, so that only solutions consistent with the eclipse duration are found. Relations needed for the method of differential corrections in least-squares solutions are specified, and we apply the Marquardt scheme for improvement of solution convergence. Parameters of Vela X1: GP Velorum are obtained from seven combinations of pulse and radial velocity data. The estimated masses are thereby put into some perspective, especially for the neutron star. The mass of the supergiant ( m  sin³  i ) now ranges only ±5 per cent from the mean of seven results, although the uncertainty in i makes the actual mass range larger. We discuss the determinacy of certain parameters and their historical consistency. For example, the systemic radial velocity differs among spectroscopic data sets by more than 20 km s⁻¹. We show that, contrary to published assertions, the orbital inclinations of high-mass X-ray binaries are essentially indeterminable by the usual methods, although lower limits to inclination may be meaningful for some examples.     

Spectral analysis of the 91bg-like Type Ia SN 2005bl: low luminosity, low velocities, incomplete burning

The properties of underluminous Type Ia supernovae (SNe Ia) of the 91bg subclass have yet to be theoretically understood. Here, we take a closer look at the structure of the dim SN Ia 2005bl. We infer the abundance and density profiles needed to reproduce the observed spectral evolution between −6 d and  +12.9 d  with respect to B maximum. Initially, we assume the density structure of the standard explosion model W7; then we test whether better fits to the observed spectra can be obtained using modified density profiles with different total masses and kinetic energies. Compared to normal SNe Ia, we find a lack of burning products especially in the rapidly expanding outer layers  ( v ≳ 15 000 km s⁻¹)  . The zone between ∼8500 and 15 000 km s⁻¹ is dominated by oxygen and includes some amount of intermediate-mass elements. At lower velocities, intermediate-mass elements dominate. This holds down to the lowest zones investigated in this work. This fact, together with negligible-to-moderate abundances of Fe-group elements, indicates large-scale incomplete Si burning or explosive O burning, possibly in a detonation at low densities. Consistently with the reduced nucleosynthesis, we find hints of a kinetic energy lower than that of a canonical SN Ia: the spectra strongly favour reduced densities at  ≳13 000 km s⁻¹  compared to W7, and are very well fitted using a rescaled W7 model with original mass  (1.38 M_⊙)  , but a kinetic energy reduced by ∼30 per cent (i.e. from  1.33 × 10⁵¹  to  0.93 × 10⁵¹ erg  ).     

地电化学提取有效性及提取条件试验--以半干旱草原风成砂浅覆盖景观区为例

地电化学方法作为覆盖区矿产资源勘查的一种有效手段,其原理是在人工外加电场作用下,将近地表介质中呈电活动态的物质选择性地提取,通过研究电提取元素组合、含量分布及异常特征,进而提供找矿信息的一种勘查方法。笔者通过在内蒙古洛恪顿矿区开展地电化学勘查研究,验证了地电化学法在内蒙古东乌旗风成砂覆盖区勘查的有效性,并通过对不同提取时间、不同密度的载体物质等提取条件的对比研究,确定在该区进行地电化学勘查的提取时间为24 h,载体物质选用高密度泡塑。     

地震波的计算机自动提取——智能跟踪与细化

本文通过对地震图特征的分析,提出了一个地震波的计算机自动提取方法.该方法由地震图扫描输入、灰度规一化、水平线消除、时标和起震点提取及智能跟踪与细化等步骤组成.在地震波的跟踪与细化过程中,充分利用了地震波的先验知识,以提高地震波自动提取的智能化水平.实验证明,该方法可取得较满意的结果.