辽西金羊盆地南部髫髻山组陆相火山岩及旋回层序划分

辽西金羊盆地（金岭寺－羊山盆地）南部髫髻山组陆相火山岩发育,为一套以中性为主的基性、中基性、中性火山岩组合。火山岩碱度主要为钙碱性。火山岩形成环境为活动大陆边缘区,这与本区所处大地构造位置相吻合。根据当前火山岩的研究现状,尝试性地对该盆地髫髻山组火山岩进行了火山喷发旋回层序的划分,共划分了四级火山喷发旋回层序。其中 A-A′剖面Ⅰ级 1个,Ⅱ级 5个,Ⅲ级 17个,Ⅳ级 21个; B-B′剖面Ⅰ级 1个,Ⅱ级 5个,Ⅲ级 18个,Ⅳ级 24个。     

A preliminary research on the climatic records of lacustrine deposits of Qingtu Lake in the last 6000 years

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Tetraploid induction by inhibiting mitosis I in scallopChlamys farreri

Tetraploid induction was carried out by inhibiting mitosis I in fertilized eggs ofChlamys farreri. Mitosis I was blocked with cold shock (5–7°C), Cytochalasin B (0.75 mg/L) and 6-dimethylaminopurine (6-DMAP) (60–75 mg/L) when 60% fertilized eggs released polar body II at 20°C. At 4-cells embryo stage, the ploidy was determined by counting chromosome number. In control groups, most embryos were diploids (72.22%) and aneuploids (24.78%). In Cytochalasin B, cold shock and 6-DMAP treated groups, tetraploids were respectively 10.51%, 4.08%, and 13.34%; aneuploids were 43.10%, 35.93% and 29.16%, and triploids were 7.84%, 8.52% and 18.33%. At D-larva stage, ploidy was determined by flow cytometry (FCM). The ploidy analysis of day 2 larvae showed diploids in control group and also in three treated groups. Juvenile scallops (0.2–0.3cm) which were harvested in two control groups and two CB treated groups were all diploids through checking ploidy individually by FCM. Contribution No. 3648 from the Institute of Oceanology, Chinese Academy of Sciences. Contribution No. 238 from the Experimental Marine Biology Laboratory, Chinese Academy of Sciences. Project funded by grant (No. 819-01-07) from the Chinese Science and Technology Ministry and also by “Hundred Talents Plan” grant from the Chinese Academy of Sciences.     

我国台风高发期东海和南海海区GIIRS/FY-4A温度反演廓线精度研究

基于欧洲中期天气预报中心再分析资料ERA5,对GIIRS/FY-4A温度反演廓线在我国台风高发期东海和南海海区的反演精度进行研究,结果表明:(1)东海海区,无云时GIIRS质量控制0的数据总体RMSE为1.71 K,150～450 hPa高度范围内RMSE小于1 K,450 hPa至近海面RMSE在2 K以内.质量控制...     

中国沿海HY-2A校正微波辐射计水汽含量数据精度检验方法

为评价“海洋二号”卫星（HaiYang-2A, HY-2A）校正微波辐射计（Calibration Microwave Radiometer, CMR）近海水汽产品精度,以中国沿海全球导航卫星系统（Global Navigation Satellite System, GNSS）业务观测站数据和欧洲中期天气预报中心（European Centre for Medium-Range Weather Forecasts, ECMWF)发布的第五代大气再分析资料（ECMWF Reanalysis 5, ERA5）作为验证数据。首先对选取的GNSS业务观测站数据和CMR水汽含量数据进行时空匹配,两者的观测时间一致、空间范围取为100 km;然后利用精密单点定位方法反演GNSS业务观测站上空的大气可降水量（Precipitable Water Vapor, PWV）,同时对1 h分辨率的ERA5再分析资料内插计算,得到CMR水汽数据点处的ERA5 PWV;最后以GNSS PWV和ERA5 PWV为参考,分析2015年CMR水汽产品精度和偏差时空分布。结果表明,CMR水汽含量和GNSS PWV、E...     

Sensitive response of desert vegetation to moisture change based on a near-annual resolution pollen record from Gahai Lake in the Qaidam Basin, northwest China

We present a 50-year pollen record at near-annual resolution from Gahai Lake in the Qaidam Basin on the northeastern Tibetan Plateau. Chronology of a 22-cm short core was established by ²¹⁰Pb and ¹³⁷Cs analysis. The pollen results at 0.5 cm intervals show large changes in Artemisia/Chenopodiaceae (A/C) ratios from < 0.2 to 0.95 in the last 50 years. High (low) A/C ratios represent increase (decrease) in steppe pollen production, which correspond to high (low) relative humidity observed at nearby Delingha weather station. On the basis of good correspondence with instrumental records and carbonate content from Gahai Lake, we conclude that A/C ratio is sensitive to moisture change and can be a very useful index in reconstructing paleoclimate of arid regions. Comparison with pollen and snow accumulation data from Dunde ice core suggests that effective moisture at low and high elevations shows the opposite relationship when mountain precipitation was extremely high, possibly due to topography-induced uplifting and subsiding air dynamics.     

Blazar天体3C 66A光学波段准周期光变分析

研究了Blazar天体3C 66A光学波段的准周期光变行为.收集了3C 66A光学V波段将近18 yr (2003—2021年)的测光数据,观测数据主要来源是:上海天文台(ShAO)、 AAVSO (The American Association of Variable Star Observers)数据库、Steward天文台.使用了Jurkevich和Lomb-Scargle两种方法分析了光变数据.Jurkevich方法得到了(850±90) d (～2.3 yr)和(1150±140) d (～3.2 yr)的光变周期,而Lomb-Scargle方法在充分考虑了“红噪声”效应之后同样得到了(869±70) d和(1111±90) d的光变周期,它们的置信水平分别为>99%和> 95%.通过与之前的研究结果比较,发现～2.3 yr的光变周期在3C 66A的历史光变数据中是一个稳定的周期,而～3.2 yr的周期则是不稳定的.     

射电类星体B3 1637+436A双峰轮廓宽发射线的光变研究

通过对比间隔17yr (静止系12.5yr)的Sloan Digital Sky Survey (SDSS)、Keck LRIS (Low-Resolution Imaging Spectrograph)和Baryon Oscillation Spectroscopic Survey (BOSS)的光学光谱, 对宽线双峰射电类星体B3 1637+436A的吸积盘性质做了初步研究.该类星体的SDSS (2001年5月21日)和Keck LRIS (2003年6月28\lk 日)的连续谱没有明显差异, 而BOSS (2018月6月17日)连续谱在V波段比SDSS暗了约1.2星等.这3条光谱的Hα宽发射线均表现出明显的双峰轮廓. 和连续谱一样, 宽线双峰的发射线轮廓也被认为是来自于吸积盘.通过上述3条光谱的Hα宽线双峰的盘模型拟合发现: BOSS光谱的Hα宽线双峰可以用单个盘模型很好地拟合,谱线发射区距离中心黑洞约900--3000引力半径. 而SDSS和Keck LRIS的Hα双峰轮廓需要用两个盘模型拟合, 对应的吸积盘发射区有两个区域,其中一个发射区(``外盘'')与BOSS类似, 另一个发射区(``内盘'')位于约400--900引力半径范围内, 到中心黑洞的距离显著小于外盘. 结合连续谱的光变特征,推测内盘消失是造成SDSS/Keck LRIS光谱和BOSS光谱在连续谱和发射线轮廓上同时发生光变的主要原因.     

断裂密集带在油运聚成藏中的作用——以三肇凹陷和尚2井区块扶杨油层为例

为研究三肇凹陷和尚2井区块扶杨油层油气成藏规律,采用断裂密集带与油气分布叠合的方法,分析断裂密集带在油气成藏分布中的作用.结果表明:三肇凹陷扶杨油层发育35条断裂密集带,尚2井区块扶杨油层发育9条断裂密集带;油主要分布在断裂密集带两侧,少量分布在断裂密集带内部.断裂密集带对油运移的控制作用表现在2方面:(1)断裂密集带边界断裂为油输导断裂;(2)断裂密集带不利于油横穿其侧向运移,但可沿其侧向运移.断裂密集带对油聚集的控制作用表现在2方面:(1)断裂密集带两侧的地垒和断阶构造是油聚集的有利部位;(2)断裂密集带内部的背形构造也是油聚集的有利部位.