尼泊尔及南侧邻区元古宙以来的构造-沉积演化

迄今,尼泊尔及其南侧邻区元古宙以来的构造-沉积演化尚缺乏系统性研究.为了促进区域地质认识,结合前人研究成果及新的研究发现,对尼泊尔低喜马拉雅带及以南的构造-沉积演化首次进行系统性总结与讨论.结果表明:尼泊尔低喜马拉雅带及以南与印度地盾北缘在地质历史中的构造-沉积演化息息相关,且自元古宙以来,发育了被动大陆边缘→陆内裂谷→被动大陆边缘→前陆盆地等不同构造演化阶段的沉积响应;尼泊尔西部的Dailekh群属于~1.8 Ga以前或前哥伦比亚超大陆之前的被动大陆边缘沉积;Vindhyan超群为下断上坳的陆内裂谷沉积,尼泊尔境内的Lakharpata群相当于下Vindhyan群;Gondwana超大陆裂解导致由北往南形成一系列初始发育时间越来越晚的裂谷盆地;Surkhet群至Siwalik群为被动大陆边缘至前陆盆地沉积,其中,Surkhet群Swat/Subathu组是喜马拉雅南侧地质历史上最后一套海相沉积地层,也是被动大陆边缘向前陆盆地转换期的沉积响应;Siwalik群大规模的磨拉石建造标志着喜马拉雅快速和大幅度隆升,该群沉积成岩后,印度-欧亚板块进一步的挤压作用导致了地质历史上迄今为止最后一次强烈的构造运动,形成MFT与Siwalik褶皱带,并奠定了喜马拉雅带现今构造格局.      

Modeling the X-Ray Timing Properties of Cygnus X-1 Caused by Waves Propagating in a Transition Disk

We found a subsystem of globular clusters in M31 that appears to have a formation history separate from the rest. The member clusters of this subsystem, identified from their distinct distribution in the metallicity-distance diagram, (1) have a common medium metallicity range of -0.9<&sqbl0;Fe&solm0;H&sqbr0;<-0.4, (2) have a line-of-sight velocity distribution with no significant projected rotational motion, and (3) are populated outside the inner subsystem of globular clusters of similar metallicity that shows a significant net rotational motion as a whole. We suggest that this subsystem of globular clusters was formed during a merging event of a dwarf galaxy that took place well after the initial collapse event when most of the globular clusters in M31 were formed.     

Efficient gusA Transient Expression in Porphyra yezoensis Protoplasts Mediated by Endogenous Beta-tubulin Flanking Sequences

1 Introduction Porphyra yezoensis is one of the most widely con-sumed and cultivated seaweeds in the world. Over the past decades, much effort has been made in improving the cultured stocks and developing breeding techniques of alga. At present, nuclear transformation systems of eu-karyotic algae such as green unicellular alga Chlamydo-monas reinhardii (Rochaix and Dillewijn, 1982), diatom Phseodactylum tricornutum (Lioudmila et al., 2000) and simple multicellular green alga Volvox carteri (…     

Gold Deposits of the Yenisei Ridge (Russia) and Age of Its Formation

Please refer to the attachment(s) for more details     

蓝柱石的高温X射线衍射、差热-热重分析、偏振红外光谱和高压拉曼光谱研究

通过高温X射线衍射(XRD)、差热-热重分析、偏振红外光谱和高压拉曼光谱研究了江西大余的蓝柱石的热膨胀行为、稳定性、羟基峰在(010)面上的强度变化及其常温高压拉曼光谱特征。结果表明,蓝柱石在1273K完全非晶化,其热膨胀系数αV为1.2(1)×10-5+0.16(1)T×10-9/K。蓝柱石在750K开始发生分解反应,最大的反应速率发生在1266K。在蓝柱石的(010)面上,羟基吸收峰在光的偏振方向与c轴夹角为70°和250°时最强,在光的偏振方向与c轴夹角为160°和340°时最弱。在常压至12.3GPa的压力范围内,蓝柱石没有发生相变。通过高压拉曼光谱计算得到了蓝柱石的mode Grüneisen参数的算术平均值为0.52(2)、thermal Grüneisen参数为0.64(2)。另外,根据Grüneisen关系式可以求得thermal Grüneisen参数,其值为0.70(6)。     

稻田土壤中甲烷产生率的实验研究

本实验旨在研究稻田土壤中甲烷产生率对稻田CH_4排放的影响.观测结果表明:土壤各深度的甲烷产生率有很大的变化范围(1—4639ng·h~(-1)·g~(-1)d.w.).主要的甲烷产生区域是7—17cm深的土壤层,其中以13cm深的土壤层上的生成速率最大.土壤中甲烷产生率与稻田CH_4排放率在水稻生长的某些阶段有较好的相关性,但它的季节变化却不能与排放的季节变化完全耦合.在水稻生长期,土壤中甲烷产生率随时间而增大,并在8月份水稻收割前达到最大,其日平均值在38—767 ng·h~(-1)·g~(-1)d.w.间变动.稻田土壤中甲烷产生率也存在日变化,一般在下午达到最大值,但却没有发现它与土壤温度有明显的相关关系.在不同施肥及水稻品种的稻田土壤中也观测到不同的甲烷产生率.在土壤中产生的甲烷最多只有28.8％被排放到大气中,而其余多于71.2％的则被氧化在土壤中.     

Photometric observations of three high mass X-ray binaries and a search for variations induced by orbital motion

We searched for long period variation in V-band,IC-band and RXTE X-ray light curves of the High Mass X-ray Binaries(HMXBs) LS 1698 /RX J1037.5-5647,HD 110432 /1H 1249-637 and HD 161103 /RX J1744.7-2713 in an attempt to discover orbitally induced variation. Data were obtained primarily from the ASAS database and were supplemented by shorter term observations made with the 24-and 40-inch ANU telescopes and one of the robotic PROMPT telescopes. Fourier periodograms suggested the existence of long period variat...