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111.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2020,65(2):831-849
The far-infrared (FIR) regime is one of the few wavelength ranges where no astronomical data with sub-arcsecond spatial resolution exist yet. Neither of the medium-term satellite projects like SPICA, Millimetron or OST will resolve this malady. For many research areas, however, information at high spatial and spectral resolution in the FIR, taken from atomic fine-structure lines, from highly excited carbon monoxide (CO) and especially from water lines would open the door for transformative science. These demands call for interferometric concepts. We present here first results of our feasibility study IRASSI (Infrared Astronomy Satellite Swarm Interferometry) for an FIR space interferometer. Extending on the principal concept of the previous study ESPRIT, it features heterodyne interferometry within a swarm of five satellite elements. The satellites can drift in and out within a range of several hundred meters, thereby achieving spatial resolutions of <0.1 arcsec over the whole wavelength range of 1–6 THz. Precise knowledge on the baselines will be ensured by metrology methods employing laser-based optical frequency combs, for which preliminary ground-based tests have been designed by members of our study team. We first give a motivation on how the science requirements translate into operational and design parameters for IRASSI. Our consortium has put much emphasis on the navigational aspects of such a free-flying swarm of satellites operating in relatively close vicinity. We hence present work on the formation geometry, the relative dynamics of the swarm, and aspects of our investigation towards attitude estimation. Furthermore, we discuss issues regarding the real-time capability of the autonomous relative positioning system, which is an important aspect for IRASSI where, due to the large raw data rates expected, the interferometric correlation has to be done onboard, in quasi-real-time. We also address questions regarding the spacecraft architecture and how a first thermomechanical model is used to study the effect of thermal perturbations on the spacecraft. This will have implications for the necessary internal calibration of the local tie between the laser metrology and the phase centres of the science signals and will ultimately affect the accuracy of the baseline estimations. 相似文献
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This paper proposes a neural network-based fault diagnosis scheme to address the problem of fault isolation and estimation for the Single-Gimbal Control Moment Gyroscopes(SGCMGs) of spacecraft in a periodic orbit. To this end, a disturbance observer based on neural network is developed for active anti-disturbance, so as to improve the accuracy of fault diagnosis.The periodic disturbance on orbit can be decoupled with fault by resorting to the fitting and memory ability of neural network. Subsequ... 相似文献
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The laser beam used to establish a communication channel between satellite and ground segments has a small divergence angle and a tiny spot on the Earth’s surface, which may lead to the fail of the system. So it’s important to study the deflection of laser beam by the Earth’s atmosphere and find a way to calibrate this error. Both theoretical analysis and real data processing method are used to obtain the mathematical model for divergence angle of laser communication beam and its correction function. Then the model has been applied to the data, which was used to describe the atmosphere state by traditional ground segments to obtain the critical elevation angle. According to the results of calculation, our conclusion will be that the correction should be done when the critical elevation happens. 相似文献
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激光测高仪回波分解算法 总被引:1,自引:0,他引:1
开发了一种激光测高仪回波基本信息提取算法,对回波数据进行了高斯波分解,获取了高斯波分量的个数,及每个高斯波分量的波中心位置、宽度和幅度等参数.该算法首先根据回波拐点的数目和位置确定出高斯分量的个数及每个高斯分量的波中心位置和宽度初始值,随后利用线性最小二乘法计算出每个高斯分量的幅度,最后将经过选择和标记的高斯分量针对实际回波采用Levenberg-Marquardt方法进行拟合,得到优化后的高斯波基本参数.通过这些基本参数信息,能够进一步推导出激光测高仪光斑内各个反射表面的垂直分布、起伏程度和反射率等基本信息. 相似文献
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为弥补水下运载器(AUV,Autonomous Underwater Vehicle)中传统舵面控制机构的低速控制的不足,改善其操纵性能,引入单框架控制力矩陀螺(SGCMG,Single Gimbal Control Moment Gyro)作为控制机构进行姿态稳定与控制.把AUV简化为刚体,加入SGCMG,考虑水下环境的特点,建立基于SGCMG的AUV动力学模型,并仿真分析AUV的动力学、姿态运动、SGCMG的框架运动以及环境之间的相互作用.仿真结果说明:基于SGCMG控制的AUV的姿态机动快速、准确,低速性能理想,为操纵律设计及姿态控制算法研究提供基础. 相似文献
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针对传统Allan方差法分析激光陀螺误差特性过程中,不能合理解释方差中部分噪声项出现负值的情况,而采用阻尼振荡的分析方法能够对此给出合理解释,却又损失了辨识精度的问题,提出了一种基于动态Allan方差法理论的改进Allan方差法。该方法将阻尼振荡模型与动态Allan方差模型相结合,使得辨识结果的分析过程更加合理。激光陀螺零偏误差的辨识与分析结果表明:改进Allan方差法的辨识结果精度略高些,在改进Allan方差的三维分析图中可以显示出零偏中存在的数据突变情况,能够反应激光陀螺误差的动态特性。因此,改进Allan方差法更适用于激光陀螺误差特性的分析。 相似文献