Preface: Stars and interstellar medium

This issue presents proceedings of the "Stars and Interstellar Medium" section of the AllRussian Astronomical Conference VAK-2017. Sixteen papers(selected from about 70 talks) cover different problems related to stars, pulsars, interstellar gas and dust, and star formation. The preface briefly reviews these papers.     

台湾地形对台风Meranti(1010)经过海峡地区时迅速增强的影响研究

台风在趋近大陆过程中强度一般衰减, 但Meranti(1010)北上进入台湾海峡过程中却迅速加强, 且在登陆福建时达到最强。采用中国气象局台风资料、NCEP GFS 0.5°×0.5°再分析资料及台湾雷达资料, 结合中尺度数值模式WRF(The Weather Research and Forecasting Model)开展台湾地形敏感性试验, 研究Meranti进入台湾海峡过程中的结构变化及迅速加强机理。结果表明:台湾地形是Meranti迅速加强的一个重要影响因子。Meranti北上过程中, 一方面通过台湾岛地形分流作用及其背风坡效应在台湾海峡内诱生中尺度涡旋, 形成正负相间的涡度分布, 激发出与台风相关的扰动波列。地形强迫抬升及扰动波列可加强垂直运动和积云对流, 有利于台风对流发展。另一方面, 台湾地形还通过改变环境气流使台风高空辐散场加强, 环境风垂直切变减小, 形成有利于台风发展的环流背景。比较不同高度台湾地形试验中台风动能收支发现, 台湾地形激发的扰动波列和积云对流增强了次网格尺度系统与台风间能量的交换, 成为Meranti登陆前迅速加强的主要动能源。     

Models of wave duration and event fre-quency of explosion aftershocks

IntroductionSeismologistsbeganaftershocksequenceinvestigationasearlyasendofthe19thcentury.Theaftershockoccurrencefrequencyhasdifferentmodels,whichincludepowerfunctiondecaymodel(Omori,1894),hyperboladecaymodel(Utsu,1961).Mogi(1962)presentedthattheafter-shockoccurrencefrequencydecayedwithdifferentprinciplesduringdifferenttimephasesaftermainshocks.Henceforthseismologistshavestudiedalargenumberofaftershocksequencesbasedonthesemodels.Chineseseismologistsstudiedthetemporal-spatialcharacteristicsof…     

松辽盆地北部上二叠统林西组地球化学特征及地质意义

为探讨松辽盆地北部林西组地球化学特征、沉积环境及构造背景,对该区黑富地1井所钻遇的上二叠统林西组暗色泥质板岩进行主量元素、微量元素和稀土元素测试分析,结果表明：样品主量元素平均质量分数SiO₂为65.05%、Al₂O₃为17.23%、CaO为2.58%、Na₂O为2.84%、K₂O为3.29%,K₂O/Na₂O值为0.20~3.48,A1₂O₃/（CaO+Na₂O）值为0.41~8.01;稀土元素w（∑REE）值介于80.68×10^-6~215.59×10^-6之间,平均值为173.41×10^-6,δEu值介于0.61~0.88之间,平均值为0.70,表现为Eu的负异常,δCe值介于0.91×10^-6~1.01×10^-6之间,为微弱的Ce负异常,LREE富集,HREE亏损;微量元素以亏损Nb、Ta、Sr,相对富集Rb、Ba、La、Ce、Pb、Nd、Sm为特征。样品元素分析和物源w（TiO₂）-w（Ni）、La/Th-w（Hf）等判别图解表明,林西组沉积物源具有多样性,主要来源于上地壳长英质物源,还有少量来自中、基性岩火成岩物源区。样品微量元素标准化蛛网图,稀土元素球粒陨石标准化配分模式图,K₂O/Na₂O-w（SiO₂）、Th-Co-Zr/10、F₂-F₁构造背景判别图及地球化学参数对比结果表明,松辽盆地北部林西组物源构造背景主要为活动大陆边缘和大陆岛弧,可能形成于靠近大陆岛弧的活动大陆边缘构造背景。林西组应形成于海陆过渡相到陆相环境,水体由半咸水逐渐转变为淡水。     

塔中地区奥陶系喜马拉雅山期S干气充注的证据

塔中地区奥陶系天然气成因多样;Ⅰ号坡折带中东部奥陶系天然气以高干燥系数、 甲烷同位素值重为特征;与塔深1井寒武系原油裂解气接近;应主要来自寒武系原油裂解气成因。寒武系贫H2S、 高成熟原油裂解气在喜马拉雅山期时;气侵奥陶系油气藏;得到了以下主要证据的支持: 1）天然气甲烷δ13C值大多比Chung et al.（1988）天然气模式甲烷δ13C值计算值高3‰以上;2）干燥系数与甲烷δ13C值大体上具有正相关关系;3）天然气干燥系数与H2S含量大体上具有负相关关系。这些特征表明;存在贫H2S、 相对富13C甲烷为主的干气与富H2S、 相对贫13C甲烷的湿气混合作用。奥陶系中H2S-δ34S 值为14‰～20‰;远低于中深1井寒武系原地热化学硫酸盐还原作用（TSR）成因的H2S（33‰）;支持了奥陶系中H2S并不是来源于寒武系古油气藏。于是提出;来自寒武系贫H2S的干气在喜马拉雅山期对良里塔格组和鹰山组油气藏发生了气洗;油气藏的气/油比值增大、 导致了原油蜡含量增高、 甲烷δ13C值发生正偏移。     

黄河口潮滩泥沙絮凝研究

本文基于现场观测的絮团粒径、悬沙浓度及水动力数据,研究了黄河口南部潮滩泥沙絮凝特征。研究发现,黄河口潮滩絮团粒径在25.42～264.44 μm之间,平均为95.20 μm。水体紊动对黄河口潮滩絮凝的影响存在差异,紊动对絮凝促进作用的上限约为G_l=3.76 s⁻¹。紊动强度低于G_l时,紊动促进泥沙絮凝,絮团粒径随紊动加强而增大;反之水体紊动对絮凝主要起抑制作用,絮团粒径随紊动强度增大而减小。悬沙浓度对黄河口潮滩泥沙絮凝起抑制作用,同等紊动条件下高悬沙浓度对应的絮团粒径更小。黄河口潮滩絮团有效密度与粒径呈现负相关关系,沉速主要受粒径影响。本研究补充了对弱潮河口潮滩泥沙絮凝特性的认识。     

CRM─PCIPS物化探数据图像处理系统的开发与实现

本文对ＣＲＭ－ＰＣＩＰＳ物化探数据图像处理系统的需要分析、开发环境、系统结构、文件系统、设计编码、程序调试与测试方法做了概括的介绍，并从“软件工程学”的角度对该项开发工作的进程，成功经验与不足之处进行了全面的评述。     

莫桑比克罗非鱼孵卵期间口腔粘膜变化的研究

用组织学、组织化学和酶技术,对雌性莫桑比克罗非鱼在孵卵前后口腔粘膜的组织结构、抗菌酶的比活力变化进行初步研究。结果表明:在口腔粘膜的上皮中,杯状细胞是一个重要的结构,它随着雌鱼的生理状态的改变而变化。雄鱼、雌鱼和孵卵期的雌鱼口腔粘膜上皮中的杯状细胞数量上的差别显著。孵卵期的雌鱼口腔粘膜类似于哺乳动物的子宫粘膜也是受性激素影响的靶器官。该种鱼的口腔粘膜中存在着两种抗菌酶;蛋白质水解酶和壳多糖酶。孵卵前后,这两种酶的比活力分别提高1.4—2.03倍。说明孵卵时,口腔粘膜为使卵及仔鱼健康的发育,增强了抗菌能力。研究结果证明:抗菌力的增加与口腔粘膜中的杯状细胞的大量增生有着密切的关系。     

Petrogenesis of the Northwest Africa 4898 high‐Al mare basalt

Northwest Africa (NWA) 4898 is the only low‐Ti, high‐Al basaltic lunar meteorite yet recognized. It predominantly consists of pyroxene (53.8 vol%) and plagioclase (38.6 vol%). Pyroxene has a wide range of compositions (En_12–62Fs_25–62Wo_11–36), which display a continuous trend from Mg‐rich cores toward Ca‐rich mantles and then to Fe‐rich rims. Plagioclase has relatively restricted compositions (An_87–96Or_0–1Ab_4–13), and was transformed to maskelynite. The REE zoning of all silicate minerals was not significantly modified by shock metamorphism and weathering. Relatively large (up to 1 mm) olivine phenocrysts have homogenous inner parts with Fo ~74 and sharply decrease to 64 within the thin out rims (~30 μm in width). Four types of inclusions with a variety of textures and modal mineralogy were identified in olivine phenocrysts. The contrasting morphologies of these inclusions and the chemical zoning of olivine phenocrysts suggest NWA 4898 underwent at least two stages of crystallization. The aluminous chromite in NWA 4898 reveals that its high alumina character was inherited from the parental magma, rather than by fractional crystallization. The mineral chemistry and major element compositions of NWA 4898 are different from those of 12038 and Luna 16 basalts, but resemble those of Apollo 14 high‐Al basalts. However, the trace element compositions demonstrate that NWA 4898 and Apollo 14 high‐Al basalts could not have been derived from the same mantle source. REE compositions of its parental magma indicate that NWA 4898 probably originated from a unique depleted mantle source that has not been sampled yet. Unlike Apollo 14 high‐Al basalts, which assimilated KREEPy materials during their formation, NWA 4898 could have formed by closed‐system fractional crystallization.     

倾斜涡度的发展与云南冬季强降水

应用倾斜涡度发展理论,对云南的一次冬季强降水天气进行诊断分析。结果表明：强降水发生在θｅ 陡立密集区内;倾斜涡度发展和条件性对称不稳定是形成强降水的重要因子;大气的弱位势稳定和强斜压性有利于云南冬季强降水的发生。