360阶地球重力场模型DQM94A及其精度分析

介绍了适用于中国地区的３６０阶地球重力场模型ＤＱＭ９４Ａ．精度分析结果表明，应用局部积分改进的谱权综合法计算的３６０阶地球重力场模型ＤＱＭ９４Ａ，在表示中国境外地球重力场时，与用改进的基本模型ＯＳＵ９１Ａ精度相当；表示中国及其周边地区地球重力场的精度如下，用模型计算的３０＇×３０＇和１°×１°平均重力异常与相应实测结果较差的均方根基分别为±９．３０×１０^－５ｍ／ｓ２和±７．６５×１０^－５ｍ／ｓ２，在中国３７个ＧＰＳ点上，由ＤＱＭ９４Ａ计算的大地水准面高的精度为±０．８８ｍ．     

抗震设计与加固效果的实震检验

本文以１９９４年１月１７日美国加州北岭地震对各类结构选成的破坏，分析了公路桥梁、建筑物，工业设施，水坝以及基底隔震结构等的不同抗震设计和加固措施的有效性及存在的问题，为今后改进抗震设防和加固措施提供参考。     

时序分析在边坡位移预测中的应用

根据对边坡变形规律的研究，建立了边坡位移序列的叠合时序模型。将边坡位格分解为确定性位移和随机性位移两部分，并实现了基于误差方差最小原则的边坡位移中长期预测。     

Vaterite formation during coal liquefaction

The vaterite form of calcium carbonate seldom occurs in geological formations or during chemical processing. However, vaterite crystals form during the liquefaction of a Wyoming subbituminous coal. Gravitational separation of the coal showed vaterite to form because of the presence of some other mineral in the coal matrix. Model compound studies with calcium acetate identified silica and possibly iron pyrite to be minerals found in coal which seed vaterite crystals.     

镇安盆地泥炭,软褐煤中的氯仿沥青“A”及其族组分的荧光特征

对滇西镇安盆地泥炭、软褐煤中的稳定组成进行荧光分析测试并未获得满意参数,又对其中抽提物—氯仿沥青“A”及其族组分进行荧光光度机测定,得到一些新的认识.     

34层线性球面原始方程谱模式与模式大气对地形强迫的响应

本文建立了一个34层包括牛顿冷却、Rayleigh摩擦和非绝热加热线性原始方程谱模式。用此模式对地形强迫为下边界条件进行时间积分。结果表明,此模式计算稳定,有较好的精度及计算时间节省的特点模式的积分结果还表明,此模式对球面大气准定常行星波的形成和传播有较好的描写能力。     

天山中段及祁连山东段小冰期以来的冰川及环境

本文通过考察、航片判读、及AAR法测算了冰川变化,用地衣、文史资料、及树轮年表进行了小冰期的测年,使用实测资料分析、冰岩芯及树轮资料等估算了小冰期的气温与降水、并进而计算了地表径流的变化。在全部讨论中,还引用了一些试验性的方法和公式。     

DZSS-1型深层数字地震仪

DZSS-1型深层数字地震仪由三分量检波器CDJ-6B、数据采集单元、磁带机、编码钟和回放装置组成。它采用循环浮点放大-A/D转换技术、低噪音运算放大器、CMOS器件,使仪器噪音小于0.3μV（折合到前级放大器输入端,均值）,动态范围大于96dB,采用调相制、串码、单轨盒式数字磁带记录。仪器频带范围1-30Hz,浮点72dB。有钟差显示（±1ms）、噪音和误操作显示。仪器主要技术指标（道间一致性、漂移、噪音、串音、误码率、主放台阶精度）可用微机进行检测,能满足地震测深和其它低频数字测量之用。     

The small-scale outflow structure of embedded sources in taurus

High resolution interferometric COJ=1–0 observations of the outflows from two young embedded sources, TMC1 and TMC1A, show the high-velocity gas to have a conical structure, with a constant opening angle of 45° extending to within 1000 AU of the central stars. The correspondence of near-infrared reflection nebulosity atK band with blueshifted CO emission in both objects suggests the lobes are partially evacuated, as do position-velocity diagrams from single-dish COJ=2–1 data. We suggest that the outflows are driven by jets which impart momentum to the ambient medium through shocks, rather than through the entrainment of molecular material along the edges of the jet.The NRAO is operated by Associated Universities, Inc., under cooperative agreement with the National Science Foundation     

Smoke rings around supernova 1987a

Detailed observations of the [Oiii]5007 Å emission from the elliptical rings around SN 1987A suggest a model wherein the two faint, outer rings are due to emission from two circular toroids moving outwards (at 25 km s^–1) along a bipolar cone centred on the site of the supernova. The brighter, central ring is expanding radially outward at 8.3 km s^–1. The rings must have been created 2-3 × 10⁴ years before the supernova explosion and are thought to be a consequence of the interaction of stellar winds emanating from the progenitor system during the final stages of its evolution to a supernova.