电偶源频率磁测深二维层状模型参数化反演

本大地电磁测深松驰反演理论方法的基础上，探讨了电偶源频率电磁深阻抗阻率的二维反演问题。     

利用地面深空激光测距检验相对论的引力时延

讨论了广义相对论的引力时延。根据Mini－ASTROD空间计划方案，利用地面深空激光测距来检验引力时延，给出了测量值与理论值直接比对的方案，并拟合出空间曲率参数γ的值。文中采用非同步的激光应答器、皮秒事件记数器等设备，可以提高测量的精度和稳定性。在地面站和行星探测器之间直接进行激光测距，不仅可以验证广义相对论的引力时延，而且还可以使γ的精度提高至少1－2个量级。这对于宇宙学和引力理论具有十分重要的意义。     

Estimates of AGN Black Hole Mass and Minimum Variability Timescale

Black hole mass is one of the fundamental physical parameters of active galactic nuclei (AGNs), for which many methods of estimation have been proposed. One set of methods assumes that the broad-line region (BLR) is gravitationally bound by the central black hole potential, so the black hole mass can be estimated from the orbital radius and the Doppler velocity. Another set of methods assumes the observed variability timescale is determined by the orbital timescale near the innermost stable orbit around the Schwarzschild black hole or the Kerr black hole, or by the characteristic timescale of the accretion disk. We collect a sample of 21 AGNs, for which the minimum variability timescales have been obtained and their black hole masses (Mσ) have been well estimated from the stellar velocity dispersion or the BLR size-luminosity relation. Using the minimum variability timescales we estimated the black hole masses for 21 objects by the three different methods, the results are denoted by Ms, Mk and Md, respectively. We compared each of them with Mσindividually and found that: (1) using the minimum variability timescale with the Kerr black hole theory leads to small differences between Mσand Mk, none exceeding one order of magnitude, and the mean difference between them is about 0.53 dex; (2) using the minimum variability timescale with the Schwarzschild black hole theory leads to somewhat larger difference between Mσand Ms: larger than one order of magnitude for 6 of the 21 sources, and the mean difference is 0.74 dex; (3) using the minimum variability timescale with the accretion disk theory leads to much larger differences between Mσand Md, for 13 of the 21 sources the differences are larger than two orders of magnitude; and the mean difference is as high as about 2.01 dex.     

Physical Parameters of a Flare Dervied from Multi—line 2D Spectroscopy

Time series of 2D spectra of Hα and CaⅡ λ8542 for a flare of 1999 December 22 are obtained and analyzed with a new fitting technique. The method we proposed can simultaneously yield the four parameters: the line source function, the optical thickness at line center, the line-of-sight velocity and the Doppler width. We present the spatial distributions of the physical parameters and their temporal evolutions determined from the 2D spectra. Our results are consistent with the general picture predicted by the flare dynamic models.     

油田水地球化学的φ（logMi，L）规律及其应用

Samples of oil-field waters taken frown ten major oil-gas-bearing basins and more than fifty oil fields in China were studied on the basis of various bond parameters.It was found that the concentrations of Na^ , Ca^ 2 and Mg^ 2 (ppm)show a logarithmic correlation with the bond parameters. This correlation was treated with the quantitative formula log Mi=α bL for φ(lvg Mi, L). Additionally, the relations between the variation of φ(leg Mi, L) and the origin of oil-field waters and between that and the nature of crude oils are explored. For the convenience of solution of the formula nomography is recommended in this paper.     

孕镶金刚石钻头合理运用的研究

介绍了孕镶金刚石钻头结构参数的选择和正确使用的有关工艺方法。建议钻头生产厂家与用户开展岩性测定工作;推荐出计算钻头综合技术经济效果的公式。