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941.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2023,71(6):2759-2769
In this study, predictions of the E-CHAIM ionospheric model are compared with measurements by the incoherent scatter radars RISR at Resolute Bay, Canada, in the northern polar cap. Reasonable coverage was available for all seasons except winter for which no conclusions were drawn. It is shown that ratios of the model-to measured electron densities are close to unity in the central part of the F layer, around its peak. This is particularly evident for summer daytime. Distributions of the ratios are wider for other seasons indicating larger number of cases when the model underestimates or overestimates. E-CHAIM underestimates the electron density at ionospheric topside and bottomside by ~ 10–20 %. At the bottomside, the underestimations are strongest in summer and equinoctial nighttime. At the topside, the underestimations are strongest in autumn nighttime. Model overestimations are noticeable in the middle part of the F layer during dawn hours in autumn. Overall, the model tends to not predict highest-observed peak electron densities and the largest-observed heights of the peak. 相似文献
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943.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2023,71(1):744-755
In this paper, the high precision attitude control for satellite with large misaligned rotational component is investigated, proposing a novel model-free prescribed performance adaptive control (MF-PPAC) method. Based on the model-free adaptive control (MFAC) strategy, high-precision attitude control is achieved depending on the system measurement rather than the spacecraft mathematical model, which demonstrates the superiority in handling nonlinearity and uncertainty of the spacecraft system, especially for those with unbalance of the rotational component. Furthermore, the transient and the stable-state behavior of the tracking error using MFAC is constrained in the prescribed performance bounds and converges to zero gradually with the utilization of prescribed performance function (PPF) and error transformation method. Finally, the convergence and boundedness of the system error, the bounded-input bounded-output (BIBO) stability of the proposed MF-PPAC is demonstrated by the contraction mapping theory. Simulation and comparison with disturbance-observer-based PD control and MFAC illustrate the effectiveness of the proposed method. 相似文献
944.
F. Vigier A. Le Postollec G. Coussot D. Chaput H. Cottin T. Berger S. Incerti S. Triqueneaux M. Dobrijevic O. Vandenabeele-Trambouze 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
Biochips might be suited for planetary exploration. Indeed, they present great potential for the search for biomarkers – molecules that are the sign of past or present life in space – thanks to their size (miniaturized devices) and sensitivity. Their detection principle is based on the recognition of a target molecule by affinity receptors fixed on a solid surface. Consequently, one of the main concerns when developing such a system is the behavior of the biological receptors in a space environment. In this paper, we describe the preparation of an experiment planned to be part of the EXPOSE-R2 mission, which will be conducted on the EXPOSE-R facility, outside the International Space Station (ISS), in order to study the resistance of biochip models to space constraints (especially cosmic radiation and thermal cycling). This experiment overcomes the limits of ground tests which do not reproduce exactly the space parameters. Indeed, contrary to ground experiments where constraints are applied individually and in a limited time, the biochip models on the ISS will be exposed to cumulated constraints during several months. Finally, this ISS experiment is a necessary step towards planetary exploration as it will help assessing whether a biochip can be used for future exploration missions. 相似文献
945.
为了分析太阳同步轨道卫星的光学特性,对FY-1卫星的可见光和红外波段光学信号进行了仿真计算和模拟试验验证.通过对外部辐射及内部热源的分析,计算了卫星的温度场,采用随机起伏表面算法模拟表面覆盖材料外表面,通过阴影遮挡判断及双向反射分布函数(BRDF, Bi-directional Reflectance Distribution Function)模型计算卫星对外部辐射的反射特性,编程计算得到在可见光0.4~1.0μm和红外8~14 μm,14~16 μm波段下卫星的光学特性.结果表明红外辐射亮度与表面温度相关,8~14 μm最大约90 W/(m2·sr)、14~16 μm最大约20 W/(m2·sr).空间可见光辐射强度具有明显的镜面反射效应,卫星主体峰值2 200 W/sr.通过地面模拟测量空间目标的温度和红外辐射验证了温度及红外辐射仿真计算模型,可见光辐射强度仿真计算结果与地面模型卫星测量结果误差在20%以内. 相似文献
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948.
针对航天器总装测试试验任务的新形势,提炼出项目管理中质量、进度、成本、风险等各要素,简要介绍了其管理过程、方法和工具。旨在突破技术、设备、人员、保障条件等资源瓶颈的制约,规范航天器总装测试试验过程中项目管理的组织流程和方法,为组织决策提供具有实际价值的理论支持,使多型号航天器项目总装、测试、试验按照最优计划进行。 相似文献
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