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931.
Supercooled water with temperatures below freezing point,was identified from hydrographic data obtained by Chinese and Australian expeditions to Prydz Bay,Antarctica,during the austral summer.The study shows that most supercooled waters occurred at depths of 63-271 m in the region north of the Amery Ice Shelf(AIS) front.The maximum supercooling was 0.16°C below the in-situ freezing point.In temperature and salinity ranges of-2.14--1.96°C and 34.39-34.46,respectively,the water was colder and fresher than peripheral shelf water.The supercooled water had less variability in the vertical profiles compared to shelf water.Based on analysis of their thermohaline features and spatial distribution,as well as the circulation pattern in Prydz Bay,we conclude that these supercooled waters originated from a cavity beneath the AIS and resulted from upwelling just outside of the AIS front.Water emerging from the ice shelf cools to an extremely low temperature(about-2.0°C) by additional cooling from the ice shelf,and becomes buoyant with the addition of melt water from the ice shelf base.When this water flows out of the ice shelf front,its upper boundary is removed,and thus it rises abruptly.Once the temperature of this water reaches below the freezing point,supercooling takes place.In summer,the seasonal pycnocline at-100 m water depth acts as a barrier to upwelling and supercooling.The upwelling of ice shelf outflow water illuminates a unique mid-depth convection of the polar ocean. 相似文献
932.
1 INTRODUCTION Measuring the velocity of ocean currents is one of the most important tasks in physical oceanography research. Many centuries ago, mariners had begun to obtain the sea surface cur- rents from vessel drift records. As early as in 1870s instr… 相似文献
933.
给出并解释了星际介质中轻元素D,3He,4He和Li的最新观测数据.星际介质中轻元素的丰度观测结果可以用来检验标准大爆炸核合成理论,因此对这些元素的丰度研究具有重要的天体物理意义.到目前为止,轻元素丰度的观测结果基本上支持开放宇宙的观点.根据最新的观测结果,在本地星际介质中D丰度可能存在小尺度不均匀性,而对类星体吸收云的观测表明不同观测者所获得的原初D丰度结果最大差别可达一个量级.如果观测是可靠的,那么在目前的标准大爆炸核合成理论和星系化学演化模型框架下还不能解释这种结果.另外种种迹象表明太阳系丰度可能不代表45亿年前本地星际介质的丰度. 相似文献
934.
935.
Kuang Wenhui Zhang Shuwen Du Guoming Yan Changzhen Wu Shixin Li Rendong Lu Dengsheng Pan Tao Ning Jing Guo Changqing Dong Jinwei Bao Yuhai Chi Wenfeng Dou Yinyin Hou Yali Yin Zherui Chang Liping Yang Jiuchun Xie Jiali Qiu Juan Zhang Hansong Zhang Yubo Yang Shiqi Sa Rigai Liu Jiyuan 《地理学报(英文版)》2022,32(9):1705-1723
Journal of Geographical Sciences - High-resolution mapping and monitoring of national land use/cover changes contribute significantly to the knowledge of the interaction between human activities... 相似文献
936.
937.
André M van der Schaar M Zaugg S Houégnigan L Sánchez AM Castell JV 《Marine pollution bulletin》2011,63(1-4):18-26
The development and broad use of passive acoustic monitoring techniques have the potential to help assessing the large-scale influence of artificial noise on marine organisms and ecosystems. Deep-sea observatories have the potential to play a key role in understanding these recent acoustic changes. LIDO (Listening to the Deep Ocean Environment) is an international project that is allowing the real-time long-term monitoring of marine ambient noise as well as marine mammal sounds at cabled and standalone observatories. Here, we present the overall development of the project and the use of passive acoustic monitoring (PAM) techniques to provide the scientific community with real-time data at large spatial and temporal scales. Special attention is given to the extraction and identification of high frequency cetacean echolocation signals given the relevance of detecting target species, e.g. beaked whales, in mitigation processes, e.g. during military exercises. 相似文献
938.
Ke-Sheng Cheng Ju-Chen Hou Jun-Jih Liou Yii-Chen Wu Jie-Lun Chiang 《Stochastic Environmental Research and Risk Assessment (SERRA)》2011,25(2):107-122
A frequency-factor based approach for stochastic simulation of bivariate gamma distribution is proposed. The approach involves
generation of bivariate normal samples with a correlation coefficient consistent with the correlation coefficient of the corresponding
bivariate gamma samples. Then the bivariate normal samples are transformed to bivariate gamma samples using the well-known
general equation of hydrological frequency analysis. We demonstrate that the proposed bivariate gamma simulation approach
is capable of generating random sample pairs which not only have the desired marginal densities of component random variables
but also their correlation coefficient. Scatter plots of simulated bivariate sample pairs also exhibit appropriate linear
patterns (dependence structure) that are commonly observed in environmental and hydrological applications. Caution should
also be exercised when specifying combinations of coefficients of skewness and the correlation coefficient for bivariate gamma
simulation. 相似文献
939.
940.
The Gushan deposit is one of the typical magnetite–apatite deposits associated with dioritic porphyries in the Lower Yangtze River Valley belt of the eastern Yangtze craton. The origin of this deposit is still uncertain and remains a controversial issue. Divergent opinions are centered on whether the iron deposits are magmatic or hydrothermal in origin. However, our field observations and mineralogical studies, combined with previous published petrological and geochemical features strongly suggest that the main ore bodies in the Gushan magnetite–apatite deposit are magmatic. Specific evidence includes the existence of gas bubbles, tubes, and miarolitic and amygdaloidal structures, melt flow banding structure and the presence of “ore breccia”. New electron microprobe analyses of the pyroxene phenocrysts of the dioritic porphyry genetically associated with the Gushan magnetite–apatite deposit show that the Fe contents in the evolving magma dramatically decrease, and then gradually increase. Because there is no evidence of mafic magma recharge, this scenario (decreasing Fe) could be plausibly interpreted by Fe-rich melts separated from Fe-poor silicate melts, i.e., liquid immiscibility was triggered by minor addition of phosphorus by crustal contamination. The occurrence of massive iron ore bodies can be satisfactorily explained by the immiscible Fe-rich melt with enormous volatile contents was driven to the top of the magma chamber due to the low density. The hot and volatile-rich iron ore magma was injected along fractures and spaces between the dioritic intrusions and wall-rocks, and led to an explosion near the surface, resulting in the immediate fragmentation of the roof of the intrusion and wall-rocks, forming brecciated ores. Moreover, other types of ores can be considered as a result of post-magmatic hydrothermal activities. Our proposed metallogenic model involving the Kiruna-type mineralization is consistent with the observed phenomenon in the Gushan deposit. 相似文献