沥青路面下多年冻土上限变化计算的探讨

以相变热传导理论为基础,利用实测路面温度资料计算了多年冻土路基中冻土上限的变化趋势,认为上限的稳定是一个时间相当长的过程．人为上限在目前条件下仍在下降,从现在的１２ｃｍ／ａ下降至５０ａ后的５ｃｍ／ａ,届时上限深度将达到９４ｍ（从路面起计算）．     

Phase shift at caustics along rays in anisotropic media

In isotropic ray tracing, the ray approximation to the wavefield undergoes a phase shift when the ray crosses a caustic. The cumulative number of such phase shifts along a ray is usually called the KMAH index. The sign of these phase shifts is prescribed by the sign of the angular frequency in combination with the sign convention used for the Fourier transformation. In isotropic media the KMAH index always increases by one or by two, depending on the type of caustic crossed. For (quasi-)shear waves in anisotropic media the KMAH index may decrease. This is the case if the associated slowness sheet is locally concave in one or two of its principal directions of curvature.     

山东刚玉及蓝宝石中天然包裹体的形态与分布特征研究

山东刚玉及蓝宝石中含有大量晶体包裹体和两相、三相包裹体，并沿特定面网和裂理面分布。单个晶体内的显微包裹体数以亿万计，其中两相和三相包裹体的形态十分复杂。     

d:\PDF\.pdf地震共中心点道集的瞬时基准面静校正和动校正

对地震野外共炮点记录进行浮动基准面静校正后的每一个共中心点道集记录而言,其基准面仍是一局部曲面,如何使之动校正后达到同相迭加,必须作所谓瞬时基准面静、动校正处理。本文从理论上阐述了共中心道集记录的瞬时基准面静、动校正的方法和技术,并用理论模型试算验证了该方法能够消除由于局部起伏对共中心点道集记录的影响,提高时间剖面的质量、速度和解释精度,确保在山区中采用地震反射波法多次覆盖技术勘探的成功。     

麻粒岩相条件下熔融反应与矿物相转变机制的实验研究

麻粒岩相条件下石榴黑云斜长片麻岩实验结果表明,含水矿物黑云母(Bi)脱水熔融、长英质矿物部分熔融的性质主要受控于温度条件;而矿物相转变不仅受控于温压条件,而且与脱水熔融、部分熔融存在密切成因联系。依据Bi脱水熔融性质和石榴石(Gi)转变反应特征,可划分以下三个阶段:(1)当温度在700℃时,Bi转变为钛铁矿(Ilm)+磁铁矿(Mt)+H_2O,Gt转变为Mt,(2)当温度在730—760℃,Bi脱水熔融为富K_2O熔体(Melt)+Ilm+Mt,Gt转变为紫苏辉石(Hy)+堇青石(Crd);(3)当温度大于790℃时,Bi脱水熔融为Melt+Hy+Ilm+Mt+H_2O,Gt则转变为Hy+尖晶石(Sp)+Crd组合。熔体比例和熔体演化特征除受温压条件控制外,与长英质矿物部分熔融程度和脱水熔融性质关系密切。实验结果显示,在麻粒岩相变质作用以及与其相伴随的重熔作用(或区域性混合岩化作用)过程中,不仅存在传统的固相+固相(或流体相)的反应和脱水熔融反应,而且存在熔体参与的变质反应(即:未熔矿物与熔体之间的反应)。该项实验对深入探讨麻粒岩相矿物演化的成因机制及其动力学意义提供可靠的实验依据。     

The relation between the response spectrum and the phase diference spectrum

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Observation of DMSO and CH3S(O)OH from the gas phase reaction between DMS and OH

Products and mechanisms have been investigated for the reactions between dimethylsulfide (DMS) and dimethylsulfoxide (DMSO) and the hydroxyl radical (OH) in the presence of NO_x. All of the experiments were performed in a 480 L reaction chamber, applying Fourier transform infrared spectroscopy (FT-IR) and ion chromatography as the analytical techniques.In addition to the sulfur containing products that are known to be produced from the gas phase reaction between DMS and OH (SO₂, dimethylsulfone, methylsulfonyl peroxynitrate, methanesulfonic acid, H₂SO₄), DMSO and methanesulfinic acid (CH₃S(O)OH) were also observed as products. Only SO₂, DMSO₂ and methylsulfonyl peroxynitrate were found as sulfur containing products in the reaction between DMSO and OH. Based on these new results we propose a mechanism for the atmospheric oxidation of DMS and DMSO by OH radical.     

激波管内水汽相变滞后效应的实验研究

本文研究了激波管中稀疏波、反射稀疏波对水汽-空气混合气体作用的非定常瞬态相变过程。利用两种不同波长光束的消光方法对水汽相变过程进行了测试。结果表明:水汽非定常瞬态相变发生的温度远远低于出现于自然大气中的凝结或冻结温度，混合气体膨胀越强，水汽瞬态相变的温度越低。非定常瞬态膨胀时的压力迅速下降是水汽瞬态相变温度远远低于自然大气中水汽相变温度的主要原因。水汽瞬态相变过程中，生成的微滴尺度均匀，但微滴的数密度却随时间发生变化。     

Clast sizes of ejecta from explosive eruptions on asteroids: implications for the fate of the basaltic products of differentiation

We use a simple model of the formation, growth, coalescence and migration of veins of basaltic melt generated by partial melting in chondritic asteroids to deduce the sizes of, and pressures within, the fluid-filled dikes reaching the surfaces of such bodies. The gas contents ( 1000 ppm of mainly CO and N₂) of the asteroids were high enough that bubbles of free gas trapped in the melt veins gave the basaltic melts significant buoyancy; expansion of these gases as a dike opened to the vacuum at the surface led to fragmentation of the melts into liquid droplets which were transported upwards by the accelerating gases to the surface. The sizes of these droplets and, hence, of the pyroclastic glass beads into which they cooled, are calculated to lie in the range 30 μm to 4 mm; this range is essentially independent of the size or gas content of the asteroid parent and only weakly dependent on the internal pressure of the erupting fluid. The fate of the pyroclasts, however, does depend on all of these factors. At very low internal pressures, significant separation of the gas and liquid in a rising dike may take place and not all of the liquid will be expelled from the dike when it opens to the surface. For relatively large ( 100 km radius) asteroids with relatively low ( 300 ppm) gas contents, the larger clasts are too heavy to be lifted from the level at which magma fragmentation takes place by the gas flow and so would also remain behind to form basaltic veins. The apparent absence of basaltic veins in meteorites then implies both that internal pressures in near-surface dikes were generally greater than 0.3 MPa and that low gas contents were not common. Finally, as long as pyroclasts are lofted from the magma fragmentation level, they will be accelerated to at least 90% of the final gas speed. If this speed exceeds the escape speed from the asteroid (as happens readily for high gas contents and small asteroids), the pyroclasts will be expelled into space and lost from the meteorite record. Otherwise (low gas contents or large asteroids), they will eventually fall back to be incorporated into the surface regolith, modifying the chemical and physical properties of meteorites subsequently derived from it.