An experimental study of structures arising in convective roll flows of magma melts in peripheral chambers of volcanoes

The morphology and internal convective structure of continuous roll flows in magma melts were experimentally studied with regard to peripheral (shallow) magma chambers and downgoing circular gravity flows in conduits. We found properties of continuous convective mixing in a magma melt in a peripheral chamber due to convective roll flows. We investigated the mechanism that is responsible for cumulus generation at the bottom of a peripheral chamber when homogeneous and heterogeneous melts are emplaced. We conducted an experimental study of how the contact surface is formed at the cumulus-melt boundary. We made a qualitative study of the mechanism that affects the composition of magma melts over time in a peripheral and a mantle (deeper) chamber owing to crystallization, as well as the special mechanism that is responsible for cumulus generation in the peripheral chamber.     

Sky brightness in the solar almucantar in the presence of thin cirrus clouds

Measurements of the sky brightness at wavelengths of 0.63 and 1.01 μm in the solar almucantar in the presence of optically thin cirrus clouds were taken at the Zvenigorod Scientific Station of the Institute of Atmospheric Physics, Russian Academy of Sciences, with the aid of a scanning photometer. The method of measurements allowed continuous monitoring of the optical state of the atmosphere and, in particular, monitoring of its optical thickness τ. Experimental values of τ are used to compare theoretical and experimental data on the sky brightness in the solar almucantar. It is shown that information about possible sizes and possible orientations of ice crystals in space can be gained only if the content of ice crystals with definite shapes and sizes in clouds is relatively high.     

Specific structure of convection currents in the system layered intrusion–feeding conduit–parental magma chamber

The structure of convection currents was experimentally studied in the model system layered intrusion–feeding conduit–parental magma chamber. Persistent hydrodynamical and thermophysical interaction between interrelated melts of the parental magma and intrusive body occurs through the feeding conduit. Being associated, they control the structure of convection currents and mechanisms of heat and mass transfer in the intrusive, conduit, and magma chamber. The existence of two convection countercurrents in the conduit has experimentally been established: inner central lifting jet and outer annular downward current along the conduit walls. At the top of the conduit, the downward current has the lowest temperature and appears to be quite in equilibrium with the earlier precipitated crystals. Moving downward along the conduit wall, the annular descending current interacts with the lifting jet and, as a result, becomes hotter and undersaturated relative to the crystals that formed before. Thus, there is no possibility for heterogeneous crystallization to occur on the walls of conduit. The experimentally simulated mechanism of melt interaction in a whole natural system rules out the possibility of formation of a zone of immobile melt with stable steady-state temperature stratification anywhere in the chamber's volume.     

Attenuation of coda waves and Q_c value beneath the Chengdu telemetered seismic network

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基于ArcGIS的中温带不同天气类型点太阳辐射分析——以佳木斯市辖区为例

考虑天气情况对入射太阳辐射的影响,研究和分析日照时数、天气类型和辐射参数的关系,并将散射模型、透射率和散射比例与4种常用天气类型相对应。以佳木斯市辖区为例,采用ArcGIS的点太阳辐射分析批处理工具,对佳木斯辐射台站进行日入射太阳辐射分析。通过将默认情况和天气类型两种模拟结果与辐射台站的实测值进行分析和验证,获得两者的相关性R2分别为0.573 4和0.899 5。研究结果表明按不同天气类型进行中温带地区点太阳辐射分析的方法切实可行,并获得更好的点日太阳辐射模拟效果,其有利于研究不同天气类型下物理和生物过程模型所受到的太阳辐射影响。     

基于改进的MT-CLIM模型的中高纬低山丘陵区太阳辐射模拟——以小兴安岭为例

将DEM、坡度和坡向作为地形因子,基于ENVI/IDL编写MT-CLIM模型批量处理程序,使用改进MTCLIM模型对小兴安岭地区的地面气象台站进行太阳辐射模拟,并将模拟结果分别与辐射台站实测数据和二次趋势面统计模型进行验证。研究结果表明:从整年上,其与辐射台站的拟合精度R2为0.813 3,其中,夏季模拟太阳辐射日值拟合精度偏低,而其与二次趋势面统计模型拟合精度R2值范围为0.571 3~0.793 3;采用改进的MT-CLIM模型模拟较大区域的太阳辐射,比统计模型具有更好的普适性和高效性,能获得较好的中高纬低山丘陵区模拟效果,且为森林生态过程模型的输入参数研究提供依据。     

Characteristics of fault rocks and paleo-earthquake source along the Koktokay-Ertai fault zone,Xinjiang,China

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Asymmetry parameter of the optical scattering phase function of a mixed-phase cloud

Basic characteristics of optical scattering in a mixed-phase cloud (asymmetry parameter of the scattering phase function and efficiency scattering factors and scattering coefficients) are considered. Theoretical consideration is based on the mixed-phase cloud model in the form of a uniform mixture of ice crystals and water droplets. Expressions allowing calculation of asymmetry parameter of the mixed-phase cloud scattering phase function are obtained as functions of the cloud temperature, average size of cloud particles, and ratios of the number densities of differently shaped ice crystals. Data calculated for the asymmetry parameter of infrared scattering in a mixed-phase cloud layer at its given temperature are presented.