柴达木盆地侏罗系油气成藏模式与油气聚集规律

针对柴达木盆地侏罗系油气勘探目标选择的难点,从烃源岩与圈闭时空配置的角度,建立侏罗系油气早期聚集早期成藏、早期聚集晚期成藏、晚期聚集晚期成藏3种模式。盆地油气来源、充注时期、油藏调整及破坏等方面存在规律性,这决定了油气分布的有序性,呈现出“断褶区聚气,山前、潜伏区聚油,凸起顶、凸起斜坡区油气并存”的基本格局和油气富集程度依次变好的序列。据此预测油气富集范围,从中优选冷湖4号东斜坡、乌南—巴依凸起斜坡、怀头他拉—德北斜坡、潜伏Ⅰ号等新靶区。     

NBFTP: a dedicated data transfer system for remote astronomical observation at Dome A

Dome A,Antarctica,has been thought to be one of the best astronomical sites on the Earth for decades.Since it was first visited by astronomers in 2008,dozens of facilities for astronomical observation and site testing were deployed.Due to its special geographical location,the data and message exchange between Dome A and the domestic control center could only depend on Iridium.Because the link bandwidth of Iridium is extremely limited,the network traffic cost is quite expensive and the network is rather unstable,the commonly used data transfer tools,such as rsync and scp,are not suitable in this case.In this paper,we design and implement a data transfer tool called NBFTP(narrow bandwidth file transfer protocol)for the astronomical observation of Dome A.NBFTP uses a uniform interface to arrange all types of data and matches specific transmission schemes for different data types according to rules.Break-point resuming and extensibility functions are also implemented.Our experimental results show that NBFTP consumes 60%less network traffic than rsync when detecting the data pending to be transferred.When transferring small files of 1 KB,the network traffic consumption of NBFTP is 40%less than rsync.However,as the file size increases,the network traffic consumption of NBFTP tends to approach rsync,but it is still smaller than rsync.     

鄂尔多斯盆地东胜铀矿成矿作用研究

对东胜铀矿提出了物源、地层、古气候等3种成矿因素。岩相学与成矿矿物学研究表明,铀矿石中含有大量的方解石,并且长石与高岭石含量呈正相关,铀矿化与有机质也有一定的联系。结合铀矿地质特征初步分析认为,东胜铀矿是在氧化带铀元素以碳酸铀酰络合物搬运,在酸性介质条件下,还原带长石碎屑蚀变为高岭石,并有钙离子析出。当碳酸铀酰络合物从氧化带迁移到还原带,遇有大量钙离子时发生分解,出现铀矿石与方解石同时沉淀现象,有机质的还原作用也是铀矿沉淀的主要因素,经漫长的地质作用富集成工业矿体。