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21.
The Cimmerian terrane forms an almost unbroken chain stretching >13,500 km, from central southern Europe to western Indonesia, via SE Europe, the Middle East, Afghanistan, Tibet, SW China and Myanmar. Ar-guably, it is Earth’s most spectacular example of a “sliver” terrane, dwarfing in size more recently devel-oped examples, for instance the Palawan Block in the western Philippines, and the Lord Howe Rise in the Tasman Sea. The presentation will first outline the in-triguing geological features associated with this unique tectonic entity. Following that, recently obtained results following paleomagnetic investigations of two lower Permian rift-related basalt suites will be summarized (Abor Volcanics in northeastern India and Woniusi Ba-salts in Yunnan, China). The two studies are part of a larger programme of ongoing research aimed at deducing (I) the geodynamic configuration that generated the un-usual rifting system, and (II) exactly how Cimmeria fit-ted against Gondwana prior to its dispersal in the Early Permian. The critical unit is Baoshan, which we fit against Gondwana within a narrow longitudinal belt close to where northern India and northwestern Australia were once in close proximity (Fig. 1). Furthermore, we suggest that Sibumasu lay to directly the east, offshore of Australia; Qiangtang and Lhasa almost certainly sat to the west (off northern Greater India-SE Arabia), but we are uncertain as to their exact configuration. Our findings will be compared with several rather different models that have been published in recent years. The new pa-leomagnetic constraint highlights the flexibility authors currently have in reconstructing the region, principally because of the overall lack of similar high-quality data from the various blocks. We explain how new data could resolve these ambiguities, thereby offering more robust explanations for eastern Gondwana’s late Paleozoic de-velopment.  相似文献   
22.
The Moshirabad pluton is located southwest of the Sanandaj–Sirjan Metamorphic Belt, Qorveh, western Iran. The pluton is composed of diorite, monzodiorite, quartz diorite, quartz monzodiorite, tonalite, granodiorite, granite, aplite, and pegmatite. In this study 31 samples from various rocks were chosen for whole‐rock analyses and 15 samples from different lithologies were chosen for mineral chemical studies. The compositions of minerals are used to describe the nature of magma and estimate the pressure and temperature at which the Moshirabad pluton was emplaced. Feldspar compositions are near the binary systems in which plagioclase compositions range from An5 to An53 and alkali‐feldspar compositions range from Or91 to Or97. Mafic minerals in the plutonic rocks are biotite and hornblende. Based on the composition of biotites and whole‐rock chemistry, the Moshirabad pluton formed from a calc‐alkaline magma. Amphiboles are calcic amphiboles (magnesio‐hornblende or edenite). Temperatures of crystallization, calculated with the hornblende–plagioclase thermometer, range 550–750°C. These temperatures indicate that plutonic rocks have undergone some retrogressive changes in their mineral compositions. Aluminum‐in‐hornblende geobarometry indicates that the Moshirabad pluton was emplaced at pressures of 2.3–6.0 kbar, equal to depths of 7–20 km, but with consideration of regional geology, lower pressures than the above pressure range are more probable. Alteration of amphiboles can be the reason for some overestimation of pressures.  相似文献   
23.
新疆春季沙尘天气与前期月环流特征量的关系   总被引:11,自引:2,他引:9  
用新疆春季(3~5月)的沙尘日数和北半球500hPa月环流特征量等资料,使应用相关和逐步回归分析方法,研究了新疆春季沙尘天气与前一年的月环流特征量的关系,相关分析和统计结果表明:(1)新疆春季的沙尘天气不仅与同在中纬度地区的西风带上的经向环流、东亚槽等有关,还更多地与中低纬地区的副热带高压以及高纬地区的极涡等系统的月环流特征量有关。(2)新疆春季沙尘天气与前一年夏、秋季的大气环流之间存在明显的隔季相关现象。(3)利用前一年月环流特征量建立了新疆春季沙尘天气日数之间的9个回归模型,9个分析模型都通过了0.001信度检验。其中,南疆的3个模型沙尘暴、扬沙、浮尘和全疆的扬沙、浮尘模型试报效果最好。  相似文献   
24.
The Bosphorus Strait accommodates two‐way flow between the Aegean and Black Seas. The Aegean (Mediterranean) inflow has speeds of 5 to 15 cm sec?1 in the strait and a salinity contrast of ~12‰ to 16‰ with the Black Sea surface waters on the shelf. An anastomosed channel network crosses the shelf and in water deeper than 70 m is characterized by first‐order channels 5 to 10 m deep, local lateral accretion bedding, muddy in‐channel barforms, and a variety of sediment waves both on channel floors and bar crests, crevasse channels entering the overbank area and levée/overbank deposits which are radiocarbon‐dated in cores to be younger than ~7·5 to 8·0 ka. This channel network accommodates the saline density current formed by the Mediterranean inflow. The density contrast between the density underflow and the ambient water mass is ~0·01 g cm?3, similar to the density contrast ascribed to low‐concentration turbidity currents in the deep sea. Channel‐floor deposits are sandy to gravelly with local shell concentrations. Low‐relief bedforms on the channel floor have relatively straight crests, upflow‐dipping cross‐stratification, heights 1 to 1·5 m and wavelengths 85 to 155 m. Bankfull flows are subcritical, so these probably are not antidunes. Bar tops are ornamented locally with mudwaves having heights 1 to 2 m and wavelengths ~20 to 100 m; these are potentially antidunes formed under shallow overbank flows. Towards the shelf edge, the degree of channel bifurcation increases dramatically and bar tops are dissected locally by secondary channels, some of which terminate in hanging valleys. Conical mounds on the shelf (possibly mud volcanoes or sites of fluid seepage) interact with the channel network by promoting accretion of muddy streamlined macroforms in their lee. This channel network may be one of the largest and most accessible natural laboratories on Earth for the study of continuously flowing density currents. Although the driver is salinity contrast, the underflow transports sufficient sediment to form levée wedges and large streamlined barforms, and presumably transports sediment into deep water.  相似文献   
25.
利用乌鲁木齐市5座100 m气象塔10层气温观测资料,通过统计方法详细分析了乌鲁木齐市城区和郊区近地层不同高度气温季节变化和日变化特征。研究表明:乌鲁木齐市四季均存在逆温,北郊逆温最明显。近地层100 m内主城区气温日较差较小,约为3.5~5.5 ℃;郊区气温日较差较大,约为4.2~7.0 ℃。夏季郊区气温高于城区,冬季北郊气温最低、南郊最高;白天大气基本上为超绝热不稳定状态,夜间城区气温高于郊区。春、秋季,白天城区和郊区温差小、夜间大,且愈近地面温差愈大;春季城区与南郊温差可达2.4 ℃、秋季可达3 ℃。城区和郊区各季节各层最高气温与最低气温出现时间几乎不同步达到。夏季、秋季、冬季和春季最高气温分别约在17:00~18:10、16:00~17:20、14:30~15:50(北郊滞后1.5 h)、17:00~18:00(南郊提前1.5 h)出现,最低气温分别约在7:10~8:20、8:00~9:00、冬季为多个时段(这与出现逆温有关)、7:30~8:40出现。  相似文献   
26.
沙漠气象若干问题研究进展   总被引:2,自引:1,他引:1       下载免费PDF全文
沙漠占据地球陆地面积的1/4,沙漠天气和气候对全球生态、环境及气候等的影响一直都受到社会各界极大关注。本文参考国内外有关沙漠气象学研究的代表性著作,简要回顾了沙漠气象学的国内外发展历史,并从沙漠表层物理特性研究、沙漠天气与边界层研究、沙漠气候研究、沙漠影响区域及全球环境研究等多个方面阐述了沙漠气象学的研究进展。最后对沙漠气象学研究提出了展望。  相似文献   
27.
28.
本文介绍了乌鲁木齐市建成区内5座100 m气象塔地理位置,根据逻辑极值检查、僵值检查、时间一致性检查、空间一致性检查和人工干预检查等组成的一套针对气象塔观测资料的质量控制方法和四点滑动平均插值、要素垂直分布拟合和线性回归方法组成的数据插值方法,对乌鲁木齐市从南至北5座100 m气象塔2012年4月1日至2014年4月30日的资料进行质量控制和数据插值。结果表明:该套方案能很好地找出缺测、错误和可疑的数据,结合人工干预,使得检验结果更为可靠。5座气象塔资料的质量是比较好的,正常数据占总数据的97.17%,其中红光山数据质量最好(正常数据占总数据的99.01%)。非正常数据只是少数情况(占总数据的2.83%),包括缺测和错误数据,其中缺测数据占非正常数据的6.23%(出现在米东和燕南立交),错误数据占非正常数据的93.77%。虚假数据占错误数据的89.99%(大部分为风速、风向),僵值数据占错误数据的5.47%(大部分为气温和湿度).超出逻辑极值数据占错误数据的0.41%(只出现在水塔山气温),不符合一致性数据占错误数据的4.13%(主要为湿度,主要在燕南立交)。利用四点中央插值法、每座气象塔要素垂直分布拟合和不同气象塔之间线性回归方法插值气温和相对湿度的效果较好。  相似文献   
29.
The Tortonian–Calabrian strata of Offshore Makran(Pakistan) is investigated for the purpose of reservoir assessment. The stratigraphy and petrophysics indicate that the Neogene sediments have tight reservoir potential with porosities in the range of 3%–9% and 40%–50% water saturation. The mineralogical cross plots indicate a mixed lithology with an abundance of dolomite and calcite, together with minor quartz content and shale. The seismic interpretation demonstrates medium–high amplitude reflec...  相似文献   
30.
脉冲星发射的辐射信号经过星际介质到达观测天线的过程中,存在色散效应。该效应导致有一定带宽脉冲信号的不同频率成份到达天线时间有延迟,影响对脉冲星的观测。消色散技术是脉冲星观测的关键技术,它对脉冲星观测系统的灵敏度和观测精度至关重要。脉冲星相干消色散过程是:通过对观测信号进行Nyquist采样,对采样数据做傅立叶变换,变换后的频域信号与星际介质Chirp函数乘积,然后再做逆傅立叶变换回时域,得到消色散后的时域信号。乌鲁木齐天文站依托现有的南山25m射电望远镜和VLBI记录终端MK5A系统,自行开发的相干消色散处理软件(Linux操作系统下C语言调用MPI库)和4节点机群系统,建立了脉冲星相干消色散观测系统。  相似文献   
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