中国的异珊瑚

从６０年代开始，我国学者陆续发表了异珊瑚的研究成果，建立１３个属，描述１６０余种，所发现属种数量已大大超过国外学者所描述范围，并且在异珊瑚分类，骨骼微细构造及隔壁演变规律研究等方面都取得长足的进展，特别是发现具３个隔壁的异珊瑚，对异珊瑚的隔壁发育方式及各属间隔壁变异关系有了清楚地揭示，在分类方面可将异珊瑚分为具内沟和不具内沟的两个系列，异珊瑚在我国产出时代为泥盆纪早期至石炭纪晚期，我国的异珊瑚绝大     

中国的异珊瑚

从６０年代开始，我国学者陆续发表了异珊瑚的研究成果，建立１３个属，描述１６０余种。所发现属种数量已大大超过国外学者所描述范围，并且在异珊瑚分类、骨骼微细构造及隔壁演变规律研究等方面都取得长足的进展。特别是发现具３个隔壁的异珊瑚，对异珊瑚的隔壁发育方式及各属间隔壁变异关系有了较清楚地揭示。在分类方面可将异珊瑚划分为具内沟和不具内沟的两个系列。异珊瑚在我国产出时代为泥盆纪早期至石炭纪晚期。我国的异珊瑚绝大多数产于早石炭世大塘期的海相地层内，常与Ｙｕａｎｏｐｈｙｌｕｍ带的皱纹珊瑚共生，是划分早石炭世地层的重要化石     

伸展域构造变换带内部构造类型研究

分别从传递带和调节带两个方面论述了构造变换带内的构造类型，将传递带内的构造类型分为传递断层等四种类型，将调节带内的构造类型划分为背斜等四种类型。分析了传递带与调节带内各构造类型的发育条件、几何形态特征以及它们之间的相互关系。研究认为，传递带和调节带内的构造类型主要取决于其发育位置处的构造背景及边界控制条件。     

栖霞东北地区成矿地质条件及找矿预测

胶东栖霞东北部地区处于挤压与拉伸并存的地球动力学环境，发育韧－脆性剪切带，NE－NNE向新型，层间滑动断层3种构造类型，控制着韧性剪切带型，微细浸浸型，层间滑动角砾岩型金矿化的产出，根据成矿地质条件，划分出藏家庄盆地周边和金山－庙后地区两个成矿预测区，有望取得找矿突破。     

四射珊瑚AuloPhyllum fungites骨骼微细构造的电镜研究

本文对Aulophyllum fungires （Fleming）,1828的骨骼微细构造进行了扫描电镜研究.结果表明,其骨骼纵列构造和横列构造全由纤状骨骼方解石晶针构成.晶针大小可分两级:大者在隔壁和横板中,大小近相等,其平均长度为32μm,平均直径为4μm;小者在鳞板,内斜板和柱隔壁中,其平均长度为10μm,平均直径2μm.晶针只在隔壁中沿轴部组成一排晶（?）,其平均直径为30—60μm,晶（?）两侧晶针组成晶束几近垂直,并间歇生长.在纵切面上,横板与隔壁相接处,间歇生长线是连续的,说明两者同步增长和形成过程相同.     

四射珊瑚属Lophocarinophyllum的骨骼构造兼论Lophophyllidiidae科

Lophocarinophyllum属以中轴粗大,隔壁两侧发育平列脊板,横列构造发育微弱为主要特征。骨骼微细构造属纤状及层纤状类型。隔壁和脊板可由单晶榍组成,也可由轴带不规则细小晶榍与两侧带近平行的晶针和晶束组成。由于Lophocarinophyllum acanthiseptum发育微弱横板,将Lophotabularia列为Lophocarinophyllum的同义名。Lophocarinophyllum共包含8个种,其中1个新种(L. stereoseptum sp.nov.). Lophophyllidiidae科有8个属: Lophophyllidium、Sugiyamaella、Lophocarinophyllum、Stereostylus、Neostereostylus、Timorphyllum、Lophamplexus、Paralophophyllidium.     

应用等性块段指数法划分新场井田的构造类型

介绍了等性块段指数法定量划分井田构造类型的基本原理。利用该法对筠连矿区新场井田的构造类型进行定量评价,得出该井田构造指数为1．98,属中等构造,证明原勘探所定构造类型基本正确。     

长刺泡沫状珊瑚(Gyalophylloides Cao 1975)属骨骼微细构造的电镜研究

Gyalophylloides Cao 1975属的电镜研究表明,其骨骼构造以方解石晶片组成的层状骨骼为主,它形成壁部构造和横列构造,在隔壁之间充填联结,在隔壁内包绕隔壁刺,在隔壁刺内联结和包绕杆状体。本属纤状骨骼的组成单元是晶粒和短轴晶柱,它们只见于杆状体轴部。文中还描述了本属的两个新种。     

论韩城矿区煤层气的构造控制

论述了韩城矿区总体构造控气框架及构造类型,分析了矿区的挤压与伸展构造边界,研究并揭示了不同构造类型对煤体结构类型、煤层渗透性能及煤层甲烷含量大小的控制特点与机理,为矿区煤层气勘探开发及评价预测提供了依据。      

异珊瑚隔壁的变异及其分类

自发现具有３个隔壁的异珊瑚新类型之后，对异珊瑚各属之间的隔壁变异关系有了清楚的揭示。按照后生隔壁发育的方式，可分为具内沟的异珊瑚，即由３个隔壁的Ｔｒｉｐｈｙｌｌｉａ，５个隔壁的Ｐｅｎｔａｐｈｙｌｌｉａ，直至多隔壁的Ｆｏｓｓａｐｈｙｌｌｉａ系列和不具内沟的异珊瑚系列，即由４个隔壁的Ｑｕａｄｒａｔｉｐｈｙｌｌｉａ，６个隔壁的Ｈｅｘａｐｈｙｌｌｉａ，直至多隔壁的Ｈ。此外，还可出现具有轴管结构的Ｃｒｅｐｉ     

Homalophyllum属的个体演化及其骨骼微细构造的电镜研究

本文通过对采自内蒙古下泥盆统珠斯楞组的Homalophyllum属的系列切片及电镜研究表明:（1）其个体发育早期,主隔壁细长,无中轴,至晚期,上隔壁变短,一级隔壁在轴部膨大形成明显的中轴。（2）骨胳构造以纤状骨骼为主,呈扇状排列,规则完整的晶榍构成隔壁构造。其基本组成单元为向上逐渐展宽的桨状晶条。本属的层状骨骼为方解石晶片,只见于外壁部分。笔者对Homalophyllum colmniferum（新种）也作了描述。     

Kepingophyllidae壁部微细构造及其演化

笔者用高倍光学显微镜和扫描电子显微镜，对Ｋｅｐｉｎｇｏｐｈｙｌｌｉｄａｅ壁部构造进行了详细的研究，从成因上将其划分为两类：泡沫板集聚型和隔壁始端集聚型，并对壁构造化进行了讨论。     

Classification of optical identifications of radio sources from complete samples

Classifications of the optical counterparts and radio spectra of nine radio sources are presented. The observations were carried out using the 2.1-m optical telescope in Cananea (Mexico) at 4200–9000 Å and the RATAN-600 radio telescope at 0.97–21.7 GHz. Five objects have been classified as quasars (three have redshifts z>2), two as BL Lac objects, one as an elliptical galaxy, and one as an absorption-line galaxy.     

Objects from a cross-identification of the IRAS and low-frequency Texas radio catalogs

A cross-identification of objects in the low-frequency (365 MHz) Texas radio catalog and in IRAS catalogs at four infrared wavelengths has yielded a list of 715 objects for further studies. Objects with steep spectra for which the difference in the centers of gravity of the radio and infrared sources was less than 3″ were selected from this list. Seventeen of the objects have been observed at six wavelengths using the RATAN-600 radio telescope. Spectra of nine objects from the initial list for which there were candidate optical counterparts were obtained using the 2.1-m telescope of the INAOE. The results of these observations are discussed. The presence of steep spectral indices for the radio sources is confirmed. The possible optical counterparts include interacting galaxies, an infrared galaxy, two emission-line galaxies, and a candidate BL Lac object. Optical images of the optical counterparts are presented together with radio and optical spectra.     

Analysis of errors in the tracking mechanisms of the 1.25-m telescope of the Crimean Laboratory of the SAI and the 1.5-m telescope of the Maidanak Observatory

Low-frequency (0–0.5 Hz) errors in the positions of stars in the focal plane of the ZTE 1.25-m telescope of the Crimean Laboratory of the Sternberg Astronomical Institute and the AZT-22 1.5-m telescope of the Maidanak Observatory in Uzbekistan are analyzed using data obtained during the operation of two optical compensators designed to correct the tilt of incoming wave fronts. A spectral analysis is used to identify possible origins of these errors. The amplitudes of periodic errors in the main worm-and-worm gears of the tracking mechanisms have been measured to be 1.5″ (a period of 240 s) for the 1.25-m telescope and 0.15″ (167 s) for the 1.5-m telescope. The rates of constant drifts have also been determined.     

First Telescope of the Russian–Cuban Observatory

Astronomy Reports - Beginning of operation of the first Russian–Cuban Observatory telescope, a wide-field 20-cm robotic telescope installed at the observational site optical station in...     

异珊瑚隔壁的变异及其分类

自发现具有３个隔壁的异珊瑚新类型之后，对异珊瑚各属之间的隔壁变异关系有了清楚的揭示。按照后生隔壁发育的方式，可分为具内沟的异珊瑚，即由３个隔壁的Ｔｒｉｐｈｙｌｌｉａ，５个隔壁的Ｐｅｎｔａｐｈｙｌｌｉａ，直至多隔壁的Ｆｏｓｓａｐｈｙｌｌｉａ系列和不具内沟的异珊瑚系列，即由４个隔壁的Ｑｕａｄｒａｔｉｐｈｙｌｌｉａ，６个隔壁的Ｈｅｘａｐｈｙｌｌｉｕ，直至多隔壁的Ｈｅｔｅｒｏｐｈｙｌｌｉａ。此外，还可出现具有轴管结构的Ｃｒｅｐｉｄｏｐｈｙｌｌｉｄａｅ及具有特殊外壁结构的Ｌｏｎｇｌｉｎｏｐｈｙｌｌｉｉｄａｅ。对已发现的异珊瑚１９个属作了系统的分类，并将异珊瑚置于珊瑚纲内的一个亚纲，同皱纹珊瑚亚纲相并列的分类单位。     

Analysis of the optics of the 2.5-m telescope of the Sternberg Astronomical Institute

The results of alignment and acceptance tests of the optics system of the 2.5-m telescope installed at the Caucausus Mountain Observatory of the Sternberg Astronomical Institute in 2013–2015 are reported. The optical elements of the Ritchey–Chrétien system of the telescope were manufactured by REOSC (France). Measurements of aberrations were carried out using a specially manufactured Shack–Hartmann wavefront sensor. Adjustment of the load-distribution mechanisms of the primary mirror and automatic correction for bending of the structure have made it possible to achieve the target image quality at all operational positions of the telescope, corresponding to 80% of the energy being concentrated in a circle 0.3″ in diameter. Factory interferograms of the mirrors and methods for measuring their abberation using stellar images are presented.