带相敏检波器的线性可变差动变压器(LVDT)读出电路的设计

本文简单介绍了LVDT、相敏检波器和三角波发生器的工作原理及自行设计的一种实用的LVDT相敏检波读出电路。     

Ab initio study of the high-pressure behavior of CaSiO3 perovskite

Using density functional simulations, within the generalized gradient approximation and projector-augmented wave method, we study structures and energetics of CaSiO₃ perovskite in the pressure range of the Earths lower mantle (0–150 GPa). At zero Kelvin temperature the cubic CaSiO₃ perovskite structure is unstable in the whole pressure range, at low pressures the orthorhombic (Pnam) structure is preferred. At 14.2 GPa there is a phase transition to the tetragonal (I4/mcm) phase. The CaIrO₃-type structure is not stable for CaSiO₃. Our results also rule out the possibility of decomposition into oxides.

Mercury's integral phase curve: Phase reddening and wavelength dependence of photometric quantities

We present results of a five-filter photometric study of Mercury's integral phase curve in the Johnson-Cousins UBVRI system, performed with the 0.90-m Westerlund Telescope in Uppsala, Sweden. CCD observations were made of the integrated disk for the phase angle range 22-152°, and the study is the first to cover the extended visible spectrum of Mercury. The observations are analyzed with Hapke's semi-empirical radiative transfer-based light-scattering model and photometric quantities are derived. A statistically significant phase reddening effect of is determined for Mercury based on color index observations, which is similar to that of the Moon. Phase coefficients fit to integral absolute magnitude data and Hapke models in combination with color index data provide a phase reddening effect of which does however not provide statistically significant evidence for its presence. Phase coefficients indicate that phase reddening may be decreasing in magnitude with wavelength. As for the case with the Moon, the value of the phase integral increases with wavelength, but at an eight times higher rate. This value is consistent with the difference in the rate of change in the spectral slope-emission angle relation for the two bodies. We attribute these differences with Mercury's redder spectral slope and an increase with wavelength of the backscattering lobe amplitude in the double Henyey-Greenstein particle phase function formulation. The normal albedo of integral Mercury at 1064 nm, pertinent to the return pulse energy of the BepiColombo laser altimeter (BELA), is estimated to 0.23±0.06 with a range of 0.13-0.33 for 99% of the surface.     

葡萄石的热膨胀性与压缩性及其地质意义

利用同步辐射X射线衍射及拉曼光谱技术对葡萄石分别进行了原位高温及原位高压实验。原位高温实验结果表明葡萄石的热膨胀系数为K=1. 77(3)×10~(-5)K~(-1),轴向热膨胀系数具有各向异性(α_aα_bα_c),葡萄石在1073K时开始发生脱水反应,分解为钙长石及硅灰石。原位高压X射线衍射实验结果表明,在大于12. 4GPa时,葡萄石的晶胞参数发生不连续变化,可能发生了相变;在24. 0GPa左右,葡萄石发生不可逆的非晶化转变。原位高压拉曼光谱表明,葡萄石在12. 6GPa左右发生相变,这一相变很可能与其[(Si,Al)O_4]四面体中的Si发生有序排列有关。结合葡萄石的热膨胀性及压缩性,我们确定了葡萄石在高温高压下的稳定范围,这一结果对认识上地幔中含水矿物的状态以及地幔中水的来源有重要意义。     

Crust and upper mantle heterogeneities in the southwest Pacific from surface wave phase velocity analysis

Direct earthquake-to-station Rayleigh and Love wave data observed on high gain broadband records are analyzed in order to improve the lateral resolution of the uppermost mantle in the southwest Pacific region. We used data of nine permanent Geoscope and Iris stations located in the southern hemisphere and nine other stations as part of two temporary networks, the first one installed in New Caledonia and Vanuatu (hereafter named Cavascope network) by ORSTOM and the EOST from Louis Pasteur University in Strasbourg (France) and the second one installed in the Fiji, Tonga and Niue islands (hereafter named Spase network) by Washington University in St. Louis (USA). In order to collect more significant details on the surficial structures, we included the analysis of short period waves down to 8 s. A multiple frequency filtering technique has been used to recover phase velocities of Rayleigh and Love waves for selected earthquakes with magnitude greater than 5.5 and with known centroid moment tensor (CMT). About 1100 well-distributed seismograms have been processed in the period range 8–100 s and corrections for topography and water depth have been applied to the observed phase velocities. The geographical distribution of phase velocity anomalies have then been computed using the tomographic method developed by Montagner [Montagner, J.P., 1986a. Regional three-dimensional structures using long-period surface waves. Ann. Geophys. 4 (B3), 283–294]. Due to a poor knowledge of dense, well-distributed, crustal thickness values and corresponding velocity models, we did not perform or speculate on the construction of an S-wave 3D velocity model; therefore, we limited this study to the interpretation of the phase velocity distribution. The location of phase velocity anomalies are well determined and the deviations are discussed within the framework of the geological context and compared with other tomographic models. At long periods, from 40 s to 100 s, our results agree well with most of previous studies: the tomographic imaging shows a large contrast between low and high phase velocities along the Solomon, New Hebrides and Fiji–Tonga trenches. The lowest phase velocity anomalies are distributed beneath northern and southern Fiji basins and the Lau basin (corresponding to the volume situated just above the dipping slabs), whereas the highest values are displayed beneath the Pacific plate and the eastern part of Indian plate downgoing under the North Fiji basin. At shorter periods, our results show that the phase velocity distributions are well correlated with the large structural crustal domains. The use of local temporary broadband stations in the central part of the studied area gives us the opportunity to observe surface waves showing well-dispersed trains, allowing extended velocity measurements down to 8 s although aliasing due to multipaths become important. The continental regions (Eastern Australia, New Guinea, Fiji islands and New Zealand) show low velocities which are likely due to thick continental crust, whereas the Tasmanian, D'Entrecasteaux, and the Northern and Southern Fiji basins are characterized by higher velocities suggesting thinner oceanic crust. Additional analysis including the anisotropic case and S-wave velocity inversion with depth is in progress.     

非线性时间序列分析的最新进展及其在地球科学中的应用前景

评述了非线性时间序列分析的最新进展,包括相空间重构、序列性质的鉴别、建模与预报,同时介绍了非线性时间序列分析在地球科学中的应用概况。     

青藏高原东北缘及周边地区基于程函方程的面波层析成像

利用"中国地震科学台阵探测"在南北地震带北段布设的670套宽频带地震台站记录到的面波资料,使用新近发展的程函方程面波层析成像方法,获得了青藏高原东北缘及周边地区12~60 s周期范围比以往成像结果具有更高分辨率的瑞利面波相速度分布图像.青藏高原东北缘的祁连褶皱系西段、秦岭褶皱系西段和松潘一甘孜褶皱系,在16~60s周期范围内均显示出明显的低速异常分布,表明该地区的地壳力学强度较低,在强烈的构造应力作用下易发生形变.与西段不同,祁连褶皱系东段和秦岭褶皱系中段的相速度分布特征揭示,其中下地壳的速度明显高于高原内部区域.鄂尔多斯块体整体上表现为稳定块体具有的高速特征,但其西部边缘在中上地壳的速度比块体中部地区偏低,且存在一定的不均匀性.鄂尔多斯块体西北缘的临河断陷盆地和西缘的银川断陷盆地,在较短的周期范围内(12~20 s)表现为局部低速特征,但与银川断陷盆地不同,临河断陷盆地的低速特征可一直延续至60 s周期以上,表明该盆地下方地壳及上地幔速度明显偏低,可能与深部热作用有关.阿拉善块体与其北部地区的速度差异主要表现在中上地壳,这一现象值得今后进一步探讨.基于程函方程面波层析成像方法给出了青藏高原东北缘及周边地区高分辨率的成像结果,揭示了以往面波层析成像难以获得的深部细节特征,为该地区的深部构造研究提供了新的信息.     

基于TIE方程的空间域相位恢复迭代算法

利用同步辐射X射线同轴显微层析(CT)方法对页岩进行扫描成像是一种无损的,对研究页岩孔裂隙大小、形态、三维结构及连通性等微观结构特征有重要意义的方法.同步辐射的引入将在物理上为提高页岩成像的分辨率提供了可能,在相位-吸收二重性假设下利用光强传递TIE(transport-of-intensity)方程可以较好地抑制由于相位信息带来的"边缘增强"效应,但该问题本质上是不适定的反演问题.本文根据实际问题构造模型,提出了一种与传统基于频域方法不同的,基于空间域的相位恢复迭代算法,并采用迭代Tikhonov正则化在数值上解决了噪声干扰下的不稳定性·问题.研究结果表明,新方法的残差仅为频域方法的1%左右,该方法可用于未来实际数据的处理.