自相关回归法在地震地面运动功率谱分析中的应用

本文通过数值分析，对几个著名的地震记录的功率谱ARM解的特性作了讨论，并与高速富里衰变换（FFT）法的解进行了比较，讨论了ARM应用于各类地震记录的谱分析的适用性。比较结果表明：对于不同的地震记录，其功率谱的ARM解等价于按一定谱窗宽度平滑化的FFT法解。本研究还对赤池氏推荐的自相关回归次数的经验公式提出了修正意见。本研究的成果对于高层建筑抗震设计有一定的参考价值。     

Observations of Vertical Reflections from the Topside Martian Ionosphere

The Martian ionosphere has for the first time been probed by a low frequency topside radio wave sounder experiment (MARSIS) (Gurnett et al., 2005). The density profiles in the Martian ionosphere have for the first time been observed for solar zenith angles less than 48 degrees. The sounder spectrograms typically have a single trace of echoes, which are controlled by reflections from the ionosphere in the direction of nadir. With the local density at the spacecraft derived from the sounder measurements and using the lamination technique the spectrograms are inverted to electron density profiles. The measurements yield electron density profiles from the sub-solar region to past the terminator. The maximum density varies in time with the solar rotation period, indicating control of the densities by solar ionizing radiation. Electron density increases associated with solar flares were observed. The maximum electron density varies with solar zenith angle as predicted by theory. The altitude profile of electron densities between the maximum density and about 170m altitude is well approximated by a classic Chapman layer. The neutral scale height is close to 10 to 13 km. At altitudes above 180 km the densities deviate from and are larger than inferred by the Chapman layer. At altitudes above the exobase the density decrease was approximated by an exponential function with scale heights between 24 and 65 km. The densities in the top side ionosphere above the exobase tends to be larger than the densities extrapolated from the Chapman layer fitted to the measurements at lower altitudes, implying more efficient upward diffusion above the collision dominated photo equilibrium region.     

Detector of Micrometeoroid and Artificial Space Debris Particles

The mathematical model of a space debris detector based on inflatable metal-dielectric-metal (MDM) film structure is presented. The efficiency of its implementation for detection of space debris particles at different altitudes is estimated, and the information obtained by the detector is investigated.     

ARJ21复杂双曲面长桁零件弯扭复合冷成型方法

通过对零件几何特征和计算机辅助软件的分析，在掌握零件变化规律的基础上，确定了零件的成型方法，以及实验确定成型过程中各参数值。     

Vertical TEC in the equatorial anomaly region from satellite altimetry data

The high-precision demands imposed by the ocean altimetry community of the late 1980 resulted in the TOPEX/Poseidon mission. This mission was the first to carry as its main instrument a dual-frequency sea-altimeter on board a satellite. This instrument together with other state-of-the-art technologies involved in the mission, led to sea-height determinations with precision better than 2 cm. As a by-product, the TOPEX/Poseidon mission provided vertical TEC determinations that since they became available, have demonstrated to be a powerful tool for ionospheric studies.     

Solar wind electron density and temperature over solar cycle 23: Thermal noise measurements on Wind

We present the solar wind plasma parameters obtained from the Wind spacecraft during more than nine years, encompassing almost the whole solar cycle 23. Since its launch in November 1994 Wind has frequently observed the in-ecliptic solar wind upstream of the Earth’s bow shock. The WIND/WAVES thermal noise receiver was specially designed to measure the in situ plasma thermal noise spectra, from which the electron density and temperature can be accurately determined. We present and discuss histograms of such measurements performed from 1994 to 2003. Using these large data sets, we study the density and core temperature variations with solar activity cycle and with different regimes of the solar wind. We confirm the anticorrelation of the electron density with the sunspot number, and obtain a positive correlation of the core temperature, with the sunspot number.     

利用电离层参量推断电子浓度剖面的一种简单方法

由武汉电离层观象台实测的电离层F2层临界频率foF2、3000km传播因子M(3000)F2的月中值资料，统计分析分别得出它们的经验模式，模式结果能够较好地再现这些参数的观测值．利用foF2、M(3000)F2以及TEC的经验模式，获得F2层的峰值参数，输入到电子浓度的Chapman α函数中，推断出了电子浓度的高度剖面；将剖面在一定的高度范围内积分，得到该区域内的电子含量并与实际观测TEC相比较，结果表明，在100-1000km高度范围内积分的电子含量与观测结果能够较好的符合．     

Thermospheric neutral density response to solar forcing

Recent measurements by the Solar EUV (Extreme Ultra Violet) Experiment (SEE) aboard the Thermosphere–Ionosphere–Mesosphere Energetics and Dynamics satellite (TIMED) provide solar EUV spectral irradiance with adequate spectral and temporal resolution, and thus the opportunity to use solar measurements directly in upper atmospheric general circulation models. Thermospheric neutral density is simulated with the NCAR Thermosphere–Ionosphere–Electrodynamic General Circulation Model (TIEGCM) using TIMED/SEE measurements and using the EUVAC solar proxy model. Neutral density is also calculated using the NRLMSISE-00 empirical model. These modeled densities are then compared to density measurements derived from satellite drag data. It is found that using measured solar irradiance in the general circulation model can improve density calculations compared to using the solar proxy model. It is also found that the general circulation model can improve upon the empirical model in simulating geomagnetic storm effects and the solar cycle variation of neutral density.     

深冷组合发动机吸气模态最大状态控制规律研究

为了研究深冷组合循环发动机吸气模态最大状态控制规律,基于部件法建立了发动机热力学计算模型,依据整机共同工作条件确定了发动机非设计点计算的变量与平衡方程。根据工质间的相互影响关系,提出了以氦压气机转速和氦涡轮前温度为控制变量的双变量控制规律。在考虑发动机机械负荷、气动负荷、热负荷及压气机稳定裕度等限制的条件下,根据制定的最大状态控制规律,完成了高度特性和速度特性的计算。根据限制条件计算得到了发动机的工作包线,并指出了最大状态控制规律的区域划分。最后,将控制规律应用于工作包线内,获得了压气机转速、换算转速及工质流量等参数的分布规律。结果表明：工作包线上下边界分别取决于氦压气机喘振裕度限制和空气压气机换算转速下限,右边界限制取决于换热器1氦气出口温度上限。深冷组合循环发动机最大状态控制规律应划分为2个区域,分界线满足以下条件：空气压气机和氦压气机换算转速同时达到最大值。分界线以上空气压气机达到最大工作状态,分界线以下氦压气机达到最大工作状态。空气压气机进口参数是决定控制规律分界线的主要因素。     

基于CPHD的双层粒子滤波目标跟踪算法

常规基于势概率假设密度滤波(Cardinalized Probability Hypothesis Density,CPHD)的粒子滤波(Particle Fil? ter,PF)跟踪算法应用于多目标跟踪时,容易遇到因粒子数量增加而带来的运算效率下降、目标数目估计不准的问题。文章基于常规粒子滤波 CPHD跟踪算法,通过部署双层粒子,提出基于势概率假设密度滤波的双层粒子滤波 (Two-Layer Particle Filter-CPHD,TLPF-CPHD)算法,以便提高目标数目及状态估计精度。仿真实验结果证明,相比于常规 PF-CPHD算法,新算法具有更好的目标数目和状态估计准确性。