麻黄山西区延长组长4+5至长6储层成岩作用及成岩演化史研究

麻黄山西区长4＋5至长6储层为一套三角洲前缘亚相的细砂岩,研究证明砂岩目前处于中成岩A期。机械压实与胶结作用是孔隙减少的主要作用,也是本区原生孔隙少、储集物性差的直接原因;而大气淡水的淋滤作用及有机酸溶蚀作用,尤其是有机酸溶蚀作用,是产生次生孔隙的主要作用,使局部储层物性有所改善,因此次生孔隙是本区油气的主要储集空间,下一步油气勘探开发应注重对有利次生孔隙空间的预测。     

鄂尔多斯盆地东南部富黄探区延长组长6段物源分析

上三叠统延长组长6段是鄂尔多斯盆地富黄探区主力油层组之一,南部与东北部物源交汇区主控物源不清,通过碎屑组分分析、轻矿物分析、砂岩粒度分析和微量元素地球化学分析等方法对其物源进行了综合研究.研究结果表明,东北部物源区是富黄探区延长组长6段沉积的主物源区;其母岩主要为来自盆地东北缘太古宙及古元古代变质岩,而不存在南部或东部物源体系,并且砂体展布与物源具有很好的对应性.     

庆康灵6号药物对中国对虾免疫力的作用

养殖的中国对虾用尖加０．３％主康灵６号的０实验饲料进行了１８天投喂,在停止投喂实验饲料后的第２、８、１３天分别测定了对虾血淋巴淋巴、血浆的抗菌活力和血细胞溶解物的酚氧化酶活力。     

CAS FGOALS-g3 Model Datasets for the CMIP6 Scenario Model Intercomparison Project(ScenarioMIP)

This paper describes the datasets from the Scenario Model Intercomparison Project(ScenarioMIP) simulation experiments run with the Chinese Academy of Sciences Flexible Global Ocean–Atmosphere–Land System Model,GridPoint version 3(CAS FGOALS-g3). FGOALS-g3 is driven by eight shared socioeconomic pathways(SSPs) with different sets of future emission, concentration, and land-use scenarios. All Tier 1 and 2 experiments were carried out and were initialized using historical runs. A branch run method ...     

利用IRS-P6卫星数据制作遥感影像地图

本文介绍了以IRS-P6卫星数据作为信息源完成大兴安岭林区的遥感影像地图制作的方法, 通过试验初步认识到:利用IRS-P6卫星数据制作遥感影像地图,可以满足1:50000、 1:25000比例尺的平面制图精度要求,在一些专业和专题应用中可以放大到1:15000比例尺使用。     

温度、浓度对流体中氟钛络合物水解的影响:对深部地质过程中钛元素活动的制约

Ti是自然界中丰度最高的高场强元素(HFSE),其主要赋存矿物——金红石的溶解度决定了俯冲带HFSE的活动与循环。而富氟流体被认为是影响Ti等HFSE能否活化、迁移的重要因素。本文对不同浓度的氟钛络合物(K2Ti F6)在100MPa压力和200~500℃温度下的稳定性进行了研究,结果显示其在热液条件下发生显著水解,水解程度与温度和初始浓度密切相关,即温度越高、初始浓度越低,则水解程度越剧烈。对实验数据进行拟合,首次获得了K2Ti F6的表观水解常数与温度的关系式:-ln K=(8972±788)/T-(4.16428±1.40362),其中获得的热力学参数为:ΔrHΘ=74.59±6.55k J/mol,ΔrSΘ=34.62±11.67J/(mol·K)。同时,运用上述获得的关系式将温度推广到俯冲带条件,计算了金红石溶解度和流体中Ti的最大迁移量之间的关系。结果显示,当金红石的溶解度大于1000μg/m L时,富F流体能有效迁移的Ti大于1μg/m L;随着金红石溶解度的增加,Ti的有效迁移百分比也逐渐增大,但俯冲流体中Ti的最大迁移量可能不超过6700μg/m L,比之前的预计要低得多。本文的研究证实了富F流体能最大程度活化并迁移Ti等HFSE。其中,对于岩浆-热液体系而言,F主要通过在岩浆中预富集,然后再大量分配进入晚期流体中而形成富F流体;对于俯冲带而言,多硅白云母的脱水或热解是形成富F流体/超临界流体的有效途径。     

Silicate‐oxide mineral chemistry of mafic–ultramafic rocks as an indicator of the roots of an island arc: The Chilas Complex,Kohistan (Pakistan)

The Chilas Complex is a major lower crustal component of the Cretaceous Kohistan island arc and one of the largest exposed slices of arc magma chamber in the world. Covering more than 8000 km², it reaches a current tectonic width of around 40 km. It was emplaced at 85 Ma during rifting of the arc soon after the collision of the arc with the Karakoram plate. Over 85% of the Complex comprises homogeneous, olivine‐free gabbronorite and subordinate orthopyroxene–quartz diorite association (MGNA), which contains bodies of up to 30 km² of ultramafic–mafic–anorthositic association (UMAA) rocks. Primary cumulate textures, igneous layering, and sedimentary structures are well preserved in layered parts of the UMAA in spite of pervasive granulite facies metamorphism. Mineral analyses show that the UMAA is characterized by more magnesian and more aluminous pyroxene and more calcic plagioclase than those in the MGNA. High modal abundances of orthopyroxene, magnetite and ilmenite (in MGNA), general Mg–Fe–Al spatial variations, and an MFA plot of whole‐rock analyses suggest a calc‐alkaline origin for the Complex. Projection of the pyroxene compositions on the Wo–En–Fs face is akin to those of pyroxenes from island arcs gabbros. The presence of highly calcic plagioclase and hornblende in UMAA is indicative of hydrous parental arc magma. The complex may be a product of two‐stage partial melting of a rising mantle diaper. The MGNA rocks represent the earlier phase melting, whereas the UMAA magma resulted from the melting of the same source depleted by the extraction of the earlier melt phase. Some of the massive peridotites in the UMAA may either be cumulates or represent metasomatized and remobilized upper mantle. The Chilas Complex shows similarities with many other (supra)subduction‐related mafic–ultramafic complexes worldwide.     

Interferometric observations of HCN and CN towards carbon stars

Using the IRAM interferometer we have observed four carbon stars (U Cam, CIT6, Y CVn, IRC+40540) in the HCN(J=1 66l2m2321747n/xxlarge8594.gif" alt="rarr" align="BASELINE" BORDER="0"> 0) and CN(N=1 66l2m2321747n/xxlarge8594.gif" alt="rarr" align="BASELINE" BORDER="0"> 0) lines. Here we present some results for CIT6 and U Cam.     

大地水准面高的计算及其在海底地形反演中的应用

为充分挖掘海洋重力数据在反演海底地形中的应用潜力,尝试探索利用大地水准面高反演海底地形的技术途径,并以夏威夷—皇帝海山链拐点所在海区作为反演试验区进行验证。首先采用Belikov列推法计算伴随(缔和)勒让德函数,利用EIGEN-6C4地球重力场模型解算获取了分辨率为1'的大地水准面高格网数值模型;然后通过综合分析反演比例函数和转换函数特点、研究海区大地水准面高与海底地形的相干特性以及大地水准面高本身尺度特征,获得了利用大地水准面高反演海底地形的频段范围;最终以试验海区大地水准面高为数据输入,构建了相应的海底地形模型(BNT模型),并与ETOPO1等海深模型进行比对分析。试验结果表明:BNT模型检核差值在一倍均方差范围检核点数量占比70.60%,相比正态分布更加集中;BNT模型检核精度低于ETOPO1等海深模型;海深模型检核精度随着水深增加不断提升,水深小于1 000 m时,海深模型相对误差出现较大发散现象;计算海域ETOPO1模型精度最高,GEBCO模型和DTU10模型检核精度相当。     

地震动参数速报技术研究

本论文内容涵盖传感器组网,数据获取、存储、管理、迁移与服务,以及地震动参数计算与发布等检测系统各个环节,在研究过程中,以地震动参数速报技术研究为主题,并注意把相关的技术应用在实际的工作中。“基于IPV6对地震烈度传感器网络”部分直接使用了ShakeMap开发过程中有关数据流的接收、服务,操作系统的重编译,事件检测,图片产出,