地段地理学及其实践意义

地段地理学是以微观尺度的地段研究为对象的现代应用地理学的工程化方向为其基本内涵,通过运用案例对其进一步分析说明,充分表明了地段地理学的实践意义。     

面积率α幂修正Neugebauer方程

网目调地图彩色印刷颜色再现 ,由于光在油墨和纸张第一表面上的反射和光在油墨和纸张内部的多重反射 ,将产生网点在转移过程中面积率的扩张和亏损。这一效应将破坏原始 Neugebauer方程关于色块三剌激值和网点面积率之间的线性关系。本文作者提出面积率 α幂修正的 Neugebauer方程 ,对于三色和四色印刷过程给出计算结果。     

一个韧性转换挤压带的变形分解作用：以阿尔金断裂带东段为例

变形构造研究显示阿尔金划分成具有近水平拉伸线理的韧性左行走滑变形域和具有陡角度倾伏拉伸线理的收缩变形域。在ＳＳ与ＰＳ之间的过渡区域还发现中等角度倾伏的拉伸线理。     

滇东南芦柴冲大型银多金属矿床的海底喷流成矿作用沉积旋回划分

芦柴冲矿床位于滇东南砚山县境内,属南岭地区西南端－－滇东南早泥盆世的层控矿带。经野外调研和室内系统研究,发现矿床为典型非火山成因的、严格受沉积相（台盆相区）控制的海底喷流沉积成因矿床。矿床中发育的南北向同生扩张断裂是重要的控盆和控矿构造,是海底喷流成矿的含矿流体运移的通道,它具周期性的振荡运动的特点,导致海底喷流成矿具周期性的沉积旋回。     

静海台地磁短周期变化异常与其附近地震的关系

近年来的一些研究表明,由于地城前孕震区地下介质的电磁结构的变化,将导致地磁短周期转换函数发生异常变化。本文通过对１９９１年唐山５．２、５．６级地城前后静海台地磁短周期转换函数参数的计算及其结果的分析和研究,提取出了可靠的地震短临前兆信息,确立了将其应用于唐山地区５级以上的震预报的短临异常特征及其指标。     

山东中部一条明显的北西向中强地震带

长清－临沂地震带是山东中部一条明显的北西向中强地震带,由９次中强地震组成。这些地震沿北西向展布,主要分布在四个震源区,大致呈５０￣５５ｋｍ等间距分布。除１６６８年郯城地震与北北东向的郯庐断裂带有关外,其它地震受北西向蒙山断裂控制,是该断裂各为层段新活动的结果。另外,该地城带内地震的发生还有一定深部构造背景。未来应注意研究该带内再次发生中强地震的可能。     

淮南煤矿塌陷区煤矸石填充复垦及其对环境的影响

在分析淮南矿区煤矸石和地面塌陷现状的基础上,探讨用煤矸石填充塌陷区的意义及其对环境的影响。     

柞水原划泥盆系中发现早前寒武纪变质岩系

本文阐述了作者在1：5万区调填图中,从柞水地区商丹断裂带南侧原划泥盆系刘岭群桐峪寺组中解体出前寒武纪中深变质岩系,取得了同位素全岩Sm－Nd年龄平均值2499．83Ma的数据,这对研究秦岭造山带的演化具有重要的地质意义。     

Target selection and accessibility for rendezvous with a Near-Earth asteroid mission

Mission to asteroids and comets has been the hot spot of deep space exploration in the new century. The choice of a suitable target, which involves both scientific value and technical feasibility, becomes a difficult task to accomplish due to limited energy and technology. The aim of this paper is to provide an approach to selecting a target and evaluating accessibility for rendezvous with a Near-Earth Asteroid mission, taking into account scientific value and engineering feasibility. Firstly, according to the orbital characteristics and physical properties of Near-Earth asteroids, we make a summary of some of the most frequent factors influencing the target selection of scientific significance. When selecting the target for a space mission, these factors can be regarded as the scientific motivations. Then in order to avoid the possibility that some high priority targets for science would be discarded due to requiring too high an energy budget by using a classical direct transfer strategy, we calculate the transfer trajectory for rendezvous with candidates by using the planetary swingby technique and the global optimal two-impulse method. Finally, through a comparison between the scientific relevance of each possible target and the corresponding estimate of energy needed for rendezvous missions, the ranking of some candidates is identified.     

Seven-frequency VLBI Observations of the GHz-Peaked-Spectrum Source OQ 208

We present quasi-simultaneous VLBI images of the GHz-Peaked-Spectrum radio source OQ 208 obtained with the Very Long Baseline Array at 1.4,1.7,2.3,5.0,8.4,15.4GHz and the European VLBI Network at 6.7 GHz.The low frequency(1.4,1.7 and 2.3GHz)ob- servations reveal a weak and extended steep-spectrum component at about 30mas away at position angle-110°,which may be a remnant emission.The radio structure of OQ 208 con- sists of two mini-lobes at 5.0,6.7,8.4 and 15.4 GHz.Our spectral analysis further confirms that the southwest lobe undergoes free-free absorption and finds that the free-free absorption is stronger in the inner region.By fitting the 8.4 GHz images from 1994 to 2005,we obtain a separation speed of 0.031±0.006 mas yr~(-1)between the two mini-lobes.This indicates a jet proper motion of 0.105±0.020 c and a kinematic age of 219±42 yr for the radio source.