腾冲火山活动监测,预测与对策研究中的若干重要问题

《膳冲火山活动监测、预测与对策研究》项目是一项集火山活动监测研究、防灾及资源综合开发与利用为一体的系统工程。需要火山地质、地震、地球化学、地球物理、地壳形变及地热等诸多相关学科的合理配置和联合攻关。在过去的３０年,众多学和研究实体对腾冲火山进行 大量的观察和研究获得一批与火山活动的相关的基础研究成果。其中也不乏说明腾冲火山存在在喷发危险性的证据。为了保证本重大项目能在有限时间内及有限的人力、财务     

High resolution spectroscopy of two young active late type stars within 20 parsecs of the Sun

We present high-resolution optical echell spectroscopy of HIP 544 and HIP 46843, two nearby solar like stars. The discovery of these young stars at such a close distance to the Sun is really a surprising phenomenon. It will help us to have a better understanding of the structure and evolutionary history of the Milky Way. The radial ve-locities (RV) of HIP 544 and HIP 46843 are measured to be -6.88±0.13km s-1 and 8.30±0.16km s-1, respectively, which are more accurate than before. The equivalent widths (EW) of the Li I 6707.8 A absorption line of HIP 544 and HIP 46843 are mea-sured to be 110±5mA and 195±5mA respectively. Based on these properties, HIP 544 is estimated to be 100-800Myr old and HIP 46843 30-100Myr old using three relatively creditable methods.     

西秦岭北缘断裂带西端晚第四纪活动特征及其西延问题

西秦岭北缘断裂是青藏高原东北缘的一条以左旋走滑运动为主的大型活动断裂。 通过卫片解译和野外地质调查, 认为断裂西端活动性仍很强烈, 并发现切龙沟一带全新世活动特征明显。 结果表明, 全新世以来西秦岭北缘断裂西端至少有2次古地震事件, 说明断裂经过土房村以后活动并没有停止, 而是继续向西延伸, 最后终止于甘加盆地。     

Arctic oscillation and the antarcic oscillation modes in the atmospheric stratosphere

1IntroductionThompson and Wallace(1998)first found the AOin1998and according to their definition,the spatialpattern of AO from the first EOF mode for the sea lev-el air-pressure(SLP)was that around the North Poleregion there was an oscillation out-of-phase with thatat the mid-latitudes zone.This oscillation had verywide frequency range from interannual to interdecadaltime scales.The AO is similar to the North Atlantic oscilla-tion(NAO)over the Atlantic.As Wallace said,theNAO could be…     

塔克拉玛干沙漠石油公路沿线风沙活动的气候环境

塔克拉玛干沙漠石油公路沿线风沙活动是由塔木盆地内热能释放与冷空气入侵相互作用的结果。冷期,盆地内冷高压逆温作用较强,地面热能不足,使得风力和风沙活动强度弱;暖期,盆地内热源剧增,每当热能源饱和遇到冷空气入侵诱导,导致了强风及强风沙活动天气。可见,区内风沙活动及风成景观的塑造过程,主要是在暖干期进行的。     

Solar wind variation with the cycle

The cyclic evolution of the heliospheric plasma parameters is related to the time-dependent boundary conditions in the solar corona. “Minimal” coronal configurations correspond to the regular appearance of the tenuous, but hot and fast plasma streams from the large polar coronal holes. The denser, but cooler and slower solar wind is adjacent to coronal streamers. Irregular dynamic manifestations are present in the corona and the solar wind everywhere and always. They follow the solar activity cycle rather well. Because of this, the direct and indirect solar wind measurements demonstrate clear variations in space and time according to the minimal, intermediate and maximal conditions of the cycles. The average solar wind density, velocity and temperature measured at the Earth’s orbit show specific decadal variations and trends, which are of the order of the first tens per cent during the last three solar cycles. Statistical, spectral and correlation characteristics of the solar wind are reviewed with the emphasis on the cycles.     

Rapid deglaciation as an initiator of volcanic activity: An hypothesis

Volcanic activity on sub-Antarctic Marion Island is found to have occurred only during the interglacials. The present volcano distribution is associated with a radial and peripheral fault system, the location of which appears to be related to the former glacier distribution. An hypothesis is presented suggesting that the faulting is a result of deglaciation and that the specific location of the faults is due to the differential stresses occurring between ice-covered and ice-free areas during isostatic uplift. The faulting initiates volcanism due to the location of the island within a volcanic region.     

利用远震接收函数反演陕西地震台站下方的地壳厚度

文中利用陕西数字地震遥测台网14个遥测子台记录的远震波形资料,用频率域反褶积方法提取接收函数,由H-Kappa叠加方法反演得到各台站下方的地壳厚度和泊松比。在此基础上结合相关地震构造文献,对陕西地区的地壳特征进行了分析,并讨论了陕西地震活动与地壳结构、地质构造之间的关系。研究结果表明:1)陕西地区的地壳总体趋势是东薄西厚,陕西南部和北部地区地壳较厚(≥40km),位于陕西中部的渭河盆地地壳较薄(34～40km);14个台站中,渭河盆地东部与山西交界的华阴台下方地壳厚度最薄(34km),而盆地西北端的陇县台位于六盘山余脉上,地壳厚度最厚(48km)。2)陕西地区泊松比值总体变化不大(0.24～0.29),可能表明这一地区的岩石组成以中度组分为主;以渭河盆地为界,向北靠近地台一侧泊松比值相对较高,向南靠近秦岭山脉一侧则比值相对较低。3)地震活动与地质构造之间存在内在的联系。渭河盆地处于几个构造体系的复合部位,属于强地震的多发区;陕西南部地区的地震活动相对较弱,主要发生在汉中盆地和安康盆地,受陕南几条主要断裂控制;陕西北部地区地质构造相对稳定,地震活动最弱。泊松比反映了地球内部的物质构成,分析认为其与地震活动存在一     

基于应变积累释放模型研究鄂尔多斯块体地震活动特征

利用1970年以来积累的仪器记录地震目录资料,基于G-R关系的应变积累释放模型,研究了鄂尔多斯块体周缘的应变积累释放分期特征及其所处的应变状态。结果表明,块体周缘的应变积累释放具有明显的两阶段分期特征,其周缘整体的应变释放和积累的分界线大致在公元2000年左右。块体周缘以及块体北缘、东缘、西缘目前均处于应变积累状态,应变积累时间均超过10年,未来将进入应变释放阶段,应变释放强度最大的为块体北缘、其次是块体的东缘和西缘;释放的应变量分别相当于6.5级和6.0级左右地震强度。南缘仍处于应变积累释放的起伏阶段。     

城市建成环境对居民体力活动的影响 ——以福州市的经验研究为例

利用福州中心城区的社会调查、POI、道路网、用地性质等数据,在社区尺度探究城市建成环境对居民休闲型中高强度体力活动的影响。研究发现：① 低密度土地利用与体力活动时长呈正向关联,功能单一和邻近主干道则对体力活动起到抑制作用。② 体力活动目的地对不同人群具有差异化影响,体育用地和付费运动场所仅能促进中高阶层和中高收入者的体力活动,而周边公共运动设施的丰富程度更具普适性意义。③ 通过纳入运动偏好和单独分析保障房、单位大院及房改房住户达到规避居住自选择的目的,证明上述建成环境特征对体力活动的影响是独立且稳健的。