火星进入器壁面脉动压力环境数值模拟

为研究跨超声速阶段来流马赫数、来流攻角及配平翼展开角的变化对进入器壁面脉动压力环境的影响规律，本文采用脱体涡方法对火星进入器模型开展非定常数值模拟，获取壁面不同位置处的脉动压力信息。研究表明：在跨超声速阶段，进入器壁面脉动压力环境随马赫数的增加而趋于减缓。配平翼迎风面分离区受脱体激波影响明显，当来流马赫数较小时，可压缩效应较弱，分离区涡流运动剧烈，诱导的脉动压力环境较强；随着来流马赫数的增加，脱体激波对分离区抑制作用增强，分离区运动受到限制，诱导的脉动压力环境趋于平缓。此外，随着来流攻角增加，配平翼迎风面上再附点的位置向翼根方向转移，从而使翼根处的脉动压力环境趋于恶劣。当配平翼展开180°时，分离区再附点位置基本固定，配平翼迎风面脉动压力环境得到一定程度的减缓。功率谱分析表明，在配平翼迎风面上诱导的脉动压力能量主要集中在中低频区域。     

Multi-input multi-output random vibration control using Tikhonov filter

Noises always disturb the control effect of an environment test especially in multi-input multi-output (MIMO) systems. If the frequency response function matrices are ill-conditioned, the noises in the driving forces will be amplified and the response spectral lines may awfully exceed their tolerances. Most of the major biases between the response spectra and the reference spectra are pro-duced by the amplified noises. However, ordinary control algorithms can hardly reduce the level of noises. The influences of the noises on both the auto-and cross-power spectra are analyzed in this paper. As a conventional frequency domain method on the inverse problem, the Tikhonov filter is adopted in the environment test to suppress the exceeding spectral lines. By altering regularization parameters gradually, the auto-power spectra can be improved in a closed control loop. Instead of using the traditional way of selecting regularization parameters, we observe the coherence change to estimate noise eliminations. Incidentally, the requirement of coherence control can be realized. The errors of the phase are then studied and a phase control algorithm is introduced at the end as a sup-plement of cross-power spectra control. The Tikhonov filter and the proposed phase control algo-rithm are tested numerically and experimentally. The results show that the noises in the vicinity of lightly damped resonant peaks are more stubborn. The response spectra are able to be greatly improved by the combination of these two methods.     

软开关弧焊逆变器的研制

本文介绍了软开关弧焊逆变器的控制技术，研制了一台弧焊软开关逆变器。给出了主电路的具体结构及其控制方式，研究了软开关的实现过程。试验结果表明，相移ＰＷＭ软开关技术能够进一步提高弧焊逆变电源的整体性能。     

群时延测试技术研究

群时延是描述信号相位失真的参数，群时延参数直接影响统一载波测控系统的跟踪测量、遥测、遥控、通信等功能，并对电视图像传输质量产生重大影响。本文论述了群时延的测试原理，并结合实际具体介绍了群时延测试方法在工程中的应用。     

一种用于出舱活动的相变储热／辐射器式热沉

首先讨论了出舱活动中的各种散热方案；然后介绍了一种相变储热／辐射器式热沉。给出了闭式散热系统设计的性能要求及相变材料的选取标准和计算方法。     

Comparative ISS accelerometric analyses

Two accelerometric records coming from the SAMSes es08 sensor in the Columbus module, the so-called Runs 14 and 33 in terms of the IVIDIL experiment, has been studied here using standard digital signal analysis techniques. The principal difference between both records is the vibrational state of the IVIDIL experiment, that is to say, during Run 14 the shaking motor of the experiment is active while that in Run 33 this motor is stopped. Identical procedures have been applied to a third record coming from the SAMSII 121f03 sensor located in the Destiny module during an IVIDIL quiescent period. All records have been downloaded from the corresponding public binary accelerometric files from the NASA Principal Investigator Microgravity Services, PIMS website and, in order to be properly compared, have the same number of data. Results detect clear differences in the accelerometric behavior, with or without shaking, despite the care of the designers to ensure the achievement of the ISS μg-vibrational requirements all along the experiments.     

On the measurements of the moon’s infrared temperature and its relation to the phase angle

Radiometric measurements of the thermal radiation originating from the moon’s surface were obtained using an infrared detector operating at wavelengths between 8 and 14 μm. The measurements cover a full moon cycle. The variation of the moon’s temperature with the lunar phase angle was established. The lunar temperatures were 391 ± 2.0 K for the full moon, 240 ± 3.5 K for the first quarter, and 236 ± 3 K for the last quarter. For the rest of the phase angles, the lunar temperature varied between 170 and 380 K. Our results are comparable with those obtained previously at these phase angles. For the new moon phase, the obtained temperature was between 120 and 133 K. With the exception of the new moon phase, our measurements at all the phase angles were consistent with those obtained using Earth-based data and those obtained by the Diviner experiment and the Clementine spacecraft. At the new phase, our measurements were comparable with those obtained from the ground but were significantly higher than those obtained by the Diviner and Clementine data. We attribute this inconsistency to either the calibration curve of our detector, which does not perform well at very low temperatures, or to infrared emission from the atmosphere. A simple linear model to predict the lunar temperature as a function of the phase angle was proposed. The experimental errors that affect the measured temperatures are discussed.     

火星进入器作强迫震荡运动壁面脉动压力数值模拟

为研究超声速阶段进入器作强迫震荡运动对壁面脉动压力环境的影响规律，本文耦合进入器刚体运动方程与流体力学方程，采用动网格技术，对火星进入器模型开展非定常数值模拟，获取壁面不同位置处的脉动压力信息。研究表明：在超声速阶段，进入器作强迫震荡运动诱导的脉动压力远大于进入器保持相对静止时仅由非定常流动诱导的脉动压力。来流马赫数为1.2时，进入器作强迫震荡运动对脱体激波影响较小，脱体激波强度较弱且形态变化较小，攻角的震荡导致同一测点距离脱体激波的位置发生周期性改变，舱体迎风面及配平翼迎风面的脉动压力环境主要受攻角变化的影响；来流马赫数为3时，进入器作强迫震荡运动对脱体激波的影响较大，脱体激波震荡剧烈，诱导舱体迎风面及配平翼迎风面产生极其恶劣的脉动压力环境，功率谱分析表明激波震荡诱导的脉动压力能量主要集中在30 Hz左右。     

Simulator of pyroshock environment and effect rules of its adjustable parameters

During the launching of spacecraft, the on-board devices will undergo a series of pyroshock environments. In order to verify the reliability of these devices under these pyroshock environments, all of them are needed to take the shock test before launching. This paper has carried out an in-depth research on the simulation method of the pyroshock based on the true explosive excitation. In this study, a simulator containing multiple adjustment parameters is presented and the safety is considered by the design of the protective cover. And the working process of this setup is simulated with the explicit dynamic codes LS-DYNA. What’s more, the effects of the adjustment parameters on the three factors of shock Response Spectrum (SRS) of the resonant board are explored carefully. The rules achieved in this paper are verified by a typical example. The results indicate that the improved simulator can avoid the danger of explosive and make full use of the advantage of actual explosive excitation. And the test condition can be quickly realized at the simulator according to the effect rules of the three adjustable parameters.