BDS中长距离非差实时动态厘米级定位算法

针对BDS常规实时动态定位(RTK)中,随着流动站与参考站间的距离增加,大气延迟误差的空间相关性大大降低,影响了整周模糊度的快速解算和流动站位置信息的解算精度问题。该文研究了一种基于非差观测误差的BDS中长距离常规RTK定位算法,采用非差误差改正方法为流动站提供误差改正,利用参考站的非差误差改正数以单颗卫星为对象进行误差改正。对电离层延迟误差和相对天顶对流层延迟误差进行参数估计,处理电离层延迟误差和对流层延迟误差的影响。最后通过BDS实测数据对该算法进行了算法验证和结果分析。实验结果表明,该算法可以实现BDS中长距离常规RTK的快速定位,并获得厘米级定位精度。     

多孔介质中聚合物溶液的流变特性

为研究多孔介质中高剪切条件下聚合物溶液流变性能的影响,利用驱 替装置和 R S6000 流变仪 测试不同 的注入速度、 渗流距离和孔喉比条件下, 聚合物溶液经过多孔介质 剪切前后 流变性的 变化. 结果 表明: 聚合物 的剪切应 力、表观黏度、 储能模量、 损耗模量等参数随着注入速度、 渗流距离和孔喉比增加而减小, 且在低剪切速率 和低角频率下 表观黏度、 储能模量、 损耗模量下降更为明显, 剪切应力下降幅度较小, 而在高剪切 速率下剪 切应力下 降幅度最 大; 渗流距 离对聚合物黏弹性作用的影响最大, 其次为注入速度, 孔喉比对聚合物黏弹性作用的影响较小.     

介质横向不均匀对震后地表位移场的影响

利用三维有限元模拟两层地球模型(包括弹性层和粘弹性层)介质的横向不均匀和断层错动的复杂性对震后地表位移场的影响，其数值结果包括弹性解和粘弹性解。结果表明，震后位移场的分布特征不仅与粘弹性层的流变特性有关，还与弹性层介质的剪切模量以及断层的同震错动有关。     

一株拮抗芒果炭疽菌海洋细菌的鉴定和发酵培养基优化

从湛江近海海水和海泥分离的229株细菌中,选出对芒果炭疽菌(Colletotrichum gloeosporioides)具有较强拮抗作用的海洋细菌BSW03,抑菌圈直径为14.0 mm。根据菌体形态、生理生化特性和16s rDNA序列分析,BSW03鉴定为枯草芽孢杆菌(Bacillus subtilis)。从9种培养基中筛选出BDPB作为BSW03的发酵培养基,通过单因子碳源、氮源试验和L9(34)正交试验对发酵培养基成分进行优化。结果表明:发酵培养基最佳配方为乳糖20 g/L,牛肉膏15 g/L,K2HPO3.3H2O 0.75 g/L,MgSO4 0.75 g/L,pH自然。转速170 r/min、温度28℃的恒温摇床培养3 d后的无菌发酵液抑菌效果最佳,抑菌圈直径为27.3 mm。     

沼泽生红冬孢酵母的固体培养条件

以麸皮、豆粕和红糖为基料,固态培养沼泽生红冬孢酵母(Rhodosporidium paludigenum),研究沼泽生红冬孢酵母的固体培养条件和培养基。结果表明,优化的固体培养基和培养条件为:豆粕、麸皮和红糖的最佳质量比为3∶1∶1;每10 g基料,各组分添加量分别为酵母膏0.2 g,硫酸铵0.2 g,水12 mL,接种1.5 mL菌液;培养基厚度2.35 cm。在此条件下培养60 h,红酵母的细胞产量最高达101.9×108g-1。     

基于GNSS的单波束测深系统在大中型水库水下地形测量中的应用

随着水库在经济社会发展中所起的作用日趋明显,对水库的开发、治理更加重视,获取高精度的水库水下地形数据变得更加急迫.随着测深技术、差分GNSS技术以及姿态传感器的不断发展,基于GNSS的测深系统为水下地形测量提供了全新的解决方案.通过合理规划测线,经过声速改正、吃水改正,利用船载GNSS导航定位和测深仪采集测深数据,经转...     

The radio and X-ray properties of Abell 2319

New radio and X-ray data are reported for the rich cluster Abell 2319. This object is known from optical data to consist of two separate clusters, which are displaced by about 10′ in the NW direction, and could be in a pre-merger state.

In the radio domain, the cluster is characterized by the presence of a central diffuse halo source, more extended and powerful than the prototype halo in the Coma cluster. The radio halo shows an irregular structure, elongated in the NE-SW direction, and also extended towards the NW. We also report data on the extended radio galaxies located within the halo, or in its proximity.

The cluster X-ray brightness distribution shows an elongated structure towards the NW, in the radial region between 6′–12′, i.e. in the direction of the subcluster. This feature is exactly coincident with the NW extension of the radio halo. In addition, more substructural features are identified which could be due to an ongoing merger of the cluster with yet another mass component.

The radio halo morphology is correlated with the X-ray structure and the existence of merger processes in the cluster. The cluster merger can provide energy to maintain the radio halo, while the origin of the relativistic particles seems more problematic.     

Chandra measurements of the distribution of mass in the luminous lensing cluster Abell 2390

We present spatially resolved X-ray spectroscopy of the luminous lensing cluster Abell 2390, using observations made with the Chandra observatory. The temperature of the X-ray gas rises with increasing radius within the central ∼ 200 kpc of the cluster, and then remains approximately isothermal, with kT =11.5_−1.6^+1.5 keV , out to the limits of the observations at r ∼1.0 Mpc . The total mass profile determined from the Chandra data has a form in good agreement with the predictions from numerical simulations. Using the parametrization of Navarro, Frenk and White, we measure a scale radius r _s∼0.8 Mpc and a concentration parameter c ∼3 . The best-fitting X-ray mass model is in good agreement with independent gravitational lensing results and optical measurements of the galaxy velocity dispersion in the cluster. The X-ray gas to total mass ratio rises with increasing radius with f _gas∼21 per cent at r =0.9 Mpc . The azimuthally averaged 0.3–7.0 keV surface brightness profile exhibits a small core radius and a clear 'break' at r ∼500 kpc , where the slope changes from S _X ∼^∝  r ^−1.5 to S _X ∼^∝  r ^−3.6 . The data for the central region of the cluster indicate the presence of a cooling flow with a mass deposition rate of 200–300 M_⊙ yr⁻¹ and an effective age of 2–3 Gyr .