潜体在非均质流体中的平衡位置与平衡过程

以探空气球为例,讨论潜体在非均质流体中的平衡位置与平衡过程.     

虚拟震源测深法及其在INDEPTH-3台阵中的应用

基于中美合作项目INDEPTH第3期在青藏高原布设的台站,使用虚拟震源测深法研究青藏高原中部的地壳厚度。结果显示,拉萨地体和羌塘地体的地壳结构存在巨大差异。拉萨地体的地壳厚度大约为57 km,与艾里均衡说预测的地壳厚度基本一致,说明拉萨地体的地壳结构比较简单。羌塘地体的地壳厚度为60~75 km,向北有增厚趋势,明显较艾里均衡说预测的地壳厚,说明羌塘地体地壳结构比较复杂,原因有可能是羌塘地体下存在高温流体和低速带,或者与印度板块岩石圈在班公湖-怒江缝合带以北向下俯冲有关。     

Study on the impact of polar stratospheric clouds on high resolution mid-IR limb emission spectra

Satellite observations of polar stratospheric clouds (PSCs) in the mid-infrared by high resolution limb emission spectrometers like the Michelson Interferometer for Passive Atmospheric Sounding have been simulated. For particles with radius the scattered tropospheric radiance accounts for a significant part of the continuum signal and leads to absorption line features overlaid over the stratospheric emission spectrum. The scattered radiance shows a strong dependence on particle size up to about radius with a maximum around 3-4. The contribution of scattered radiation depends heavily on tropospheric cloud coverage and earth surface temperature. Distinction of PSCs of different composition is possible for small particles due to differences in the imaginary part of the refractive index. For particles with radii between 1 and the simulated spectra for various PSC compositions differ due to different real parts of the refractive index. For larger particles no distinction is possible any more. Solar radiance scattered by PSCs is important for wavenumbers larger than about . For a forward scattering geometry with 30° between the position of the sun and the limb viewing direction solar contribution exceeds the terrestrial scattered radiation by about a factor of 10.     

A method for continuous control of the refractive index of liquids in capillaries

An interference method for controlling the refractive index of liquids pumped through a capillary is considered. The liquid is sounded by two systems of interference bands, the period of which differs by an insignificant value prescribed by the condition of nonius coincidence. An analytical expression is obtained to calculate the refractive index of the liquid controlled in automatic reading of the interference patterns. Institute of Electronics, National Academy of Sciences of Belarus, 22 Logoiskii Trakt, Minsk, 220841, Belarus. Translated from Zhurnal Prikladnoi Spektroskopii, Vol. 66, No. 6, pp. 832–835, November–December, 1999.     

DYNAMIC PROPERTIES OF ASSISTANT SOUNDER IN BLACK CICADA (C.atrata FABRICIUS)

The dynamic properties of the assistant sounders in the black cicada are given and the twitching properties of Contraction in the sounding muscle are revealed in this paper.For the operculum, tymbal cover and joint membrane, each of their vibration periods consists of three subgroup vibrations (SGV_(a,b,c)) corresponding to amplitude-modulation pulse trains (AMPT_(1,2,3)) in every syllable of synchro song. In comparison with the vibration at dorsum, the SGV_(a-c) have a subband with the function of regulating the tone. During calling song continuously, the pressure change inside the resonant cavity and the airspeed through the spiracles on both sides are about 7. 94—15.88 Paand 0.59—0.84 cm~3/s respectively, and they increase by about 7 and 2.6 times as the abdomen is moved. When the contraction motion of the sounding muscle comes up to the critical Sounding state, it further produces the twitching process, and drives the sounding membrane and the toning plate-membrane to produce AMPT_(1-3) and SGV_(a     

Comparison of single and multiple scattering approaches for the simulation of limb-emission observations in the mid-IR

The validity of single scattering radiative transfer calculations for simulation of limb-emission measurements of clouds in the mid-infrared spectral region was investigated by comparison with a multiple scattering model. For in limb direction optically thin clouds, like polar stratospheric clouds, errors of the single scattering scheme range below 3%. For optically thick clouds deviations are below 3% in case of low single scattering albedo (ω₀=0.24) increasing up to 10-30% for ω₀=0.84. Clouds which are optically thick in limb, but thin in nadir direction, can cause limb radiances which are by a factor of 1.7 higher than the blackbody radiance at cloud altitude.     

基于VXI总线的电离层探测系统信号源的设计

根据新型电离层斜向返回探测系统的编码调相脉冲压缩、间隔收发体制，采用FPGA和数字上变频器实现了一种适合该体制的、基于VXI总线的信号源模块．具体描述了该模块的设计方法、主要逻辑和时序关系，试验表明，该模块运行可靠，工作方式和参数调整灵活，实现了符合体制要求的射频信号和时序控制信号，满足了新型电离层斜向返回探测系统抗干扰、开放性和易升级的要求。     

电测深确定最佳井位的数学模型及其应用

在电测深确定最佳井位过程中 ,本文运用模糊数学和灰色关联度理论建立确定最佳井位的数学模型 ,并通过实例验证了该数学模型的科学性和实用性     

A unified framework for constructing globally convergent algorithms for multidimensional coefficient inverse problems

We present a unified framework for constructing the globally convergent algorithms for a broad class of multidimensional coefficient inverse problems arising in natural science and industry. Based on the convexification approach, the unified framework substantiates the numerical solution of the corresponding problem of nonconvex optimization. A globally convergent iterative algorithm for an inverse problem of diffuse optical mammography is constructed. It utilizes the contraction property of a nonlinear operator resulting from applying the convexification approach. The effectiveness of this algorithm is demonstrated in computational experiments.     

利用空间外差光谱技术进行紫外高分辨率大气散射信号探测

羟基OH对于人类理解中间层化学成分非常重要,它是大气光化学反应中重要的氧化剂,OH在308 nm波段受到太阳能量激发,发射出OH A2Σ＋-X２Π（0,0）荧光信号。为了探测中间层大气中OH自由基的紫外共振荧光发射信号,从复杂背景信号中分离目标信号,研制了中高层大气OH自由基超分辨空间外差光谱仪,光谱范围为308.2～309.8 nm,光谱分辨率为0.008 25 nm。临边观测主要探测大气散射信号,能量来源为大气中的粒子,包括大气分子与气溶胶、云等对太阳能量的散射作用。中高层大气OH自由基超分辨空间外差光谱仪基于空间外差光谱技术,可以在设计的闪耀波长范围内获得极高的光谱分辨率,适用于大气成分的精细探测。通过在前置或后置光学系统中加入柱面镜,总视场内的场景被分成多个视场切片,每一个视场切片的干涉图分别成像到对应的探测器行上。利用空间外差光谱仪具有空间维分层成像功能,临边观测时可以同时获取不同高度层大气吸收光谱的散射辐射信号,无需像传统临边探测遥感器在不同高度层进行扫描来获取大气高度维的廓线信息。为了验证中高层大气OH自由基超分辨空间外差光谱仪的临边散射信号探测能力与对观测几何的敏感性,进行了地面临边观测实验,探测紫外308 nm波段大气散射信号。模拟临边观测几何,选取晴朗无云的一天,在空旷场地对大气散射信号进行观测。由于仪器基于空间外差光谱技术,需要对干涉数据进行干涉误差修正与光谱复原。对一段观测时间内间隔10分钟的干涉数据进行光谱复原并定标,得到最终临边观测光谱。由于散射信号的主要来源为大气分子对太阳光的散射作用,因此光谱中应包含太阳光谱高分辨率精细特征信息。从高分辨率太阳光谱中选取三个特征信息窗,分析观测光谱中对应波段,三个特征信息窗完全匹配,验证了中高层大气OH自由基超分辨空间外差光谱仪的超高分辨率光谱探测能力和光谱精细信息提取能力。将太阳辐射计实时测量获得的气溶胶光学厚度及根据观测时间计算的太阳天顶角与太阳方位角输入辐射传输模型SCIATRAN,结合对应日期与经纬度的大气廓线数据库,得到模拟光谱,将实测结果与辐射传输模型结果进行比对,两者残差较小。实测结果与模拟结果存在的残差,可能是由于大气环境参数并没有完全符合实测状态,后续可使用当地实时温湿压廓线对模拟数据库进行替换,使辐射传输模型更接近实际状态。与辐射传输模型对比的结果验证了中高层大气OH自由基超分辨空间外差光谱仪的散射信号探测能力与对观测几何的敏感性,验证了在轨探测多谱段、宽谱段大气散射光谱与OH目标信号的可行性,为在轨探测OH目标信号提供了理论与实验基础。