两个古铜辉石样品的G.P区研究

在两个斜方辉石样品中观察到G.P.区亚稳相。内蒙古暗色辉长岩古铜辉石成分是En_(77)Fs_(18·6)Wo_(4·4),其高分辨象显示了密集的单层G.P.区;玄武岩中变辉长岩包体古铜辉石成分是En_(72·2)Fs_(25·7)Wo_(2·1),具双层G.P.区。该包体与具多层G.P.区的月岩橄长岩相似,后期冷却极快。在地体火成岩体结晶和冷却过程中易出现单层G.P.区,而岩体的大小,冷却的快慢可能影响G.P.区的密度。对N-14样品不同放大倍数的高分辨象G.P.区线密度和面密度的统计值同样具代表性。文中设想了G.P.区出溶的假二元系相图。     

活动星系的非相对论性外流

活动星系核有两类常见外流，相对论性的射电喷流和非相对论性的物质外流，前者主要在射电强的适动星系核中，以非热辐射为特征，非相对论性外流主要通过紫外吸收线观测到，总结了类星体非对论性外流的一些性质及其X射线观测给出了的问题，指出现有的观测表明非相对论性外流引起的质量损失很重要。     

冰后回弹对全球及中国参考框架的影响分析

文章利用ICE-5G模型发布的最新预报值,计算分析了冰后回弹对全球和中国区域的影响,发现冰后回弹不仅会引起垂直方向的地壳运动,而且还会引起水平方向的地壳运动,但是水平方向的量级要明显小于垂直方向.全球范围内最大回弹区域位于加拿大,大约为16mm/a,而由冰后回弹所引起的地壳水平方向运动达3mm/a.这个回弹量级对于维持毫米级ITRF的稳定所造成的影响是不容忽视的.中国范围内回弹值大概在0～0.7mm/a,这个量级对于参考框架的影响基本可以忽略.     

High-resolution H i and radio continuum observations of the SNR G290.1−0.8

We have observed the supernova remnant (SNR) G290.1−0.8 in the 21-cm H  i line and the 20-cm radio continuum using the Australia Telescope Compact Array (ATCA). The H  i data were combined with data from the Southern Galactic Plane Survey to recover the shortest spatial frequencies. In contrast, H  i absorption was analysed by filtering extended H  i emission, with spatial frequencies shorter than 1.1 kλ. The low-resolution ATCA radio continuum image of the remnant shows considerable internal structure, resembling a network of filaments across its 13-arcmin diameter. A high-resolution ATCA radio continuum image was also constructed to study the small-scale structure in the SNR. It shows that there are no structures smaller than ∼17 arcsec, except perhaps for a bright knot to the south, which is probably an unrelated object. The H  i absorption study shows that the gas distribution and kinematics in front of SNR G290.1−0.8 are complex. We estimate that the SNR probably lies in the Carina arm, at a distance 7 (±1) kpc. In addition, we have studied nearby sources in the observed field using archival multiwavelength data to determine their characteristics.     

西藏改则县物玛乡北部晚侏罗世吐卡日组珊瑚动物群的发现及其地质意义

西藏改则物玛地区发现了约33属47种及未定种的晚侏罗世珊瑚化石。珊瑚化石指示其所在的地层并非是原来认为的早二叠世下拉组,而是晚侏罗世牛津期—基末里期的吐卡日组。基于对改则物玛北剖面的研究,在吐卡日组之下新建了晚侏罗世萨波直不勒组。进而将班公湖-怒江地层区西段的上侏罗统自下而上划分为萨波直不勒组、吐卡日组和沙木罗组。改则县物玛乡北部吐卡日组的发现证明吐卡日组在班公湖-怒江地层区西部有着更广泛的分布。将“下拉组”修订为吐卡日组也表明班公湖-怒江地层区改则地区物玛段并不存在二叠系灰岩与侏罗系木嘎岗日岩群碎屑岩的构造混杂现象。吐卡日组以浅海碳酸盐台地相的生物礁亚相、鲕粒滩亚相为特征,厚度也十分可观,指示其具有良好的生油和储油潜力,班公湖-怒江地层区西段及南北两侧的碳酸盐岩相上侏罗统的油气前景评价工作应予以重视。