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61.
采用逆向蒙特卡罗(RMC)计算方法,在给定的飞行状态下分别计算出亚声速与超声速导弹蒙皮辐射源在不同方位角的2~μm、8~14 μm波段红外光谱辐射强度及强度场分布.结果表明:对亚声速导弹,相对于8~14 μm,其2~μm的辐射可忽略不计;对超声速导弹,相对于2~μm,其8~14 μm的辐射只有0%左右,但其绝对值较大而不可忽略不计.导弹的红外辐射在0°~90°探测位置内增加,在90°~180°内减小.大气对低空亚声速导弹辐射衰减作用强,对高空超声速导弹辐射衰减作用弱.超声速导弹的最大辐射强度是亚声速的18倍. 相似文献
62.
63.
天基紫外预警是反弹道导弹武器的重要手段。文章从地球日盲紫外空间背景和导弹紫外辐射特性两方面进行分析,论证天基紫外空间预警系统可以获得较高的信噪比和信杂比,能够实现低虚警率的空间预警。同时提出了天基紫外空间预警系统可能的3种工作体制:单一基于紫外波段的天基预警系统存在发现目标较晚的问题;紫外—红外双波段天基预警系统可以实现更低的空间预警虚警率;红外—紫外光谱复合天基预警系统可通过紫外光谱观测辨别导弹种类。最后,文章对现有紫外探测技术进行分析,论证了AlGaN和SiC探测器用于天基紫外预警的可行性,并对其工作模式进行了分析。 相似文献
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65.
利用45 keV,1 MeV和2 MeV电子分别对聚乙烯热缩套管进行辐照实验,研究不同能量电子辐照对聚乙烯热缩套管力学性能的影响,并分析电子辐照下材料的损伤效应机理,建立力学性能退化规律。结果表明:实验选定的3种能量电子辐照都会造成聚乙烯的降解,材料脆化产生裂纹,从而导致其力学性能下降;但是由于这3种能量电子穿透深度不同,45 keV电子只能造成聚乙烯热缩套管表层材料损伤,力学性能最大下降量只有30%~40%,而1 MeV和2 MeV电子却会导致套管力学性能完全丧失,力学性能下降接近100%。 相似文献
66.
Corey S. Jamieson Agnes H.H. Chang Ralf I. Kaiser 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
Mixtures of molecular nitrogen and methane have been identified in numerous outer Solar Systemices including the icy surfaces of Pluto and Triton. We have simulated the interaction of ionizing radiation in the Solar System by carrying out a radiolysis experiment on a methane – molecular nitrogen ice mixture with energetic electrons. We have identified the hydrogen cyanide molecule as the most prominent carbon–nitrogen-bearing reaction product formed. Upon warming the irradiated sample, we followed for the first time the kinetics and temporal evolution of the underlying acid–base chemistry which resulted in the formation of the cyanide ion from hydrogen cyanide. On the surfaces of Triton and Pluto and on comets in Oort’s cloud this sort of complex chemistry is likely to occur. In particular, hydrogen cyanide can be produced in low temperature environments (Oort cloud comets) and may be converted into cyanide ions once the comets reach the warmer regions of the Solar System. 相似文献
67.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2020,65(1):435-445
Strong earthquakes have an impact on the regional thermal radiation background, which has been both observed and confirmed. This effect produces anomalies in the thermal radiation background (TRBA) and increases the difficulty of extracting a thermal radiation anomaly (TRA) that is associated with an earthquake occurring during the same time period. The extraction and identification of such anomalies has been ignored by previous studies. In this study, we investigate the time-frequency analysis (TFA) method, together with the wavelet filtering of the Daubechies method and the relative power spectrum analysis of the Fourier Welch method to extract and analyse the TRBA caused by the 2008 Wenchuan Ms 8.0 earthquake and the TRA of the 2013 Minxian-Zhangxian Ms 6.6 earthquake using data concerning the brightness temperature of a black body (TBB) from the Fengyun-2 series of geostationary meteorological satellites developed by China. The result showed that this method can effectively extract and analyse the TRBA caused by the Wenchuan earthquake and the TRA of the Minxian-Zhangxian earthquake form a complex background environment. Furthermore, we discussed the impact of the earthquake on the TRBA and segmented the process. The impact is mainly reflected by three aspects; the characteristic period of the TRBA changes, the TRBA occurs at the same time every year, which is identical to the time at which the earthquake anomaly occurred, and the impact process is in stages. We also summarized the correlation between the characteristic parameters of a TRA and the regional thermal radiation background, geography, and climatic factors. 相似文献
68.
Bingbing Duan Urs Hugentobler Inga Selmke 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(5):1803-1812
Solar Radiation Pressure (SRP) is the dominant non-gravitational perturbation for GNSS (Global Navigation Satellite System) satellites. In the absence of precise surface models, the Empirical CODE Orbit Models (ECOM, ECOM2) are widely used in GNSS satellite orbit determination. Based on previous studies, the use of an a priori box-wing model enhances the ECOM model, especially if the spacecraft is a stretched body satellite. However, so far not all the GNSS system providers have published their metadata. To ensure a precise use of the a priori box-wing model, we estimate the optical parameters of all the Galileo, BeiDou-2, and QZS-1 (Quasi Zenith Satellite System) satellites based on the physical processes from SRP to acceleration. Validation using orbit prediction proves that the adjusted parameters of Galileo and QZS-1 satellites exhibit almost the same performance as the corresponding published and “best guess” values. Whereas, the estimated parameters of BeiDou-2 satellites demonstrate an improvement of more than 60% over the initial “guess” values. The resulting optical parameters of all the satellites are introduced into an a priori box-wing model, which is jointly used with ECOM and ECOM2 model in the orbit determination. Results show that the pure ECOM2 model exhibits better performance than the pure ECOM model for Galileo, BeiDou-2 GEO and QZS-1 orbits. Combined with the a priori box-wing model the ECOM model (ECOM+BW) results in the best Galileo, BeiDou-2 GEO and QZS-1 orbits. The standard deviation (STD) of satellite laser ranging residuals reduce by about 20% and 5% with respect to the pure ECOM2 model for Galileo and BeiDou-2 GEO orbits, while the reductions are about 40% and 60% for QZS-1 orbits in yaw-steering and orbit-normal mode respectively. BeiDou-2 IGSO and MEO satellite orbits do not benefit much from the a priori box-wing model. In summary, we suggest setting up a unified SRP model of ECOM+BW for Galileo, QZS-1, and BeiDou-2 orbits based on the adjusted metadata. In addition, we estimate the optical parameters of BeiDou-3e and QZS-2 satellites using a limited number of tracking stations. Results regarding the unified SRP model indicate the same advantages, the STD of satellite laser ranging residuals reduces by about 30% and 20% for QZS-2 and BeiDou-3e orbits respectively over orbit products without a priori model. The estimation procedure is effective and easy to apply to the new emerging satellites in the future. 相似文献
69.
Samy El-Jaby Leena Tomi Lembit Sihver Tatsuhiko Sato Richard B. Richardson Brent J. Lewis 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
This paper describes a methodology for assessing the pre-mission exposure of space crew aboard the International Space Station (ISS) in terms of an effective dose equivalent. In this approach, the PHITS Monte Carlo code was used to assess the particle transport of galactic cosmic radiation (GCR) and trapped radiation for solar maximum and minimum conditions through an aluminum shield thickness. From these predicted spectra, and using fluence-to-dose conversion factors, a scaling ratio of the effective dose equivalent rate to the ICRU ambient dose equivalent rate at a 10 mm depth was determined. Only contributions from secondary neutrons, protons, and alpha particles were considered in this analysis. 相似文献
70.
GTEM电磁敏感度测试系统的研制 总被引:1,自引:0,他引:1
90年代以来 ,GTEM以其独特的优越性在电磁兼容测试领域中得到了广泛的应用。许多先进国家的军用工业标准均推荐采用此项技术。文中给出了一套适合我航天型号电磁兼容测试要求的 GTEM电磁敏感度测试系统。该测试系统由 GTEM、双定向耦合器、功率计、功率放大器、射频开关矩阵、信号源、计算机组成。其工作原理是 ,按照辐射电磁敏感度的测试要求 ,系统应在试样所在区域产生幅度和频率均已知的连续波电磁场 ,当系统集成完成后 ,只需调整GTEM端口的馈入信号功率、频率以及试样安放的位置 ,即可在试样所在区域产生测试所需的连续波电磁场。系统测控软件兼顾系统的安全性及可操作性 ,采用人机对话的方式 ,在WINDOWS3.1环境下运行。该系统测试操作直观简便 。 相似文献