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排序方式: 共有508条查询结果,搜索用时 15 毫秒
1.
Luo Xucheng 《宇航学报》1990,(3)
本文研究了入射波电场为任意线极化时,平直地面反射波中左旋圆极化分量和右旋圆极化分量的数学描述,引入了地面对这类波的等效反射系数的概念,并给予了物理解释,讨论了应用的有关问题。 相似文献
2.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2007,39(5):661-667
Monthly median values of foF2, hmF2 and M(3000)F2 parameters, with hourly time interval resolution for the diurnal variation, obtained with DPS-4 digisonde observations at Hainan (19.4°N, 109.0°E) are used to study the low latitude ionospheric variation behavior. The observational results are compared with the International Reference Ionospheric Model (IRI) predictions. The time period coverage of the data used for the present study is from March 2002 to February 2005. Our present study showed that: (1) In general, IRI predictions using CCIR and URSI coefficients follow well the diurnal and seasonal variation patterns of the experimental values of foF2. However, CCIR foF2 and URSI foF2 IRI predictions systematically underestimate the observed results during most time period of the day, with the percentage difference ΔfoF2 (%) values changing between about −5% and −25%, whereas for a few hours around pre-sunrise, the IRI predictions generally overestimate the observational ones with ΔfoF2 (%) sometimes reaching as large as ∼30%. The agreement between the IRI results and the observational ones is better for the year 2002 than for the other years. The best agreement between the IRI results and the observational ones is obtained in summer when using URSI coefficients, with the seasonal average values of ΔfoF2 (%) being within the limits of ±10%. (2) In general, the IRI predicted hmF2 values using CCIR M(3000)F2 option shows a poor agreement with the observational results. However, when using the measured M(3000)F2 as input, the diurnal variation pattern of hmF2 given by IRI2001 has a much better agreement with the observational one with the detailed fine structures including the pre-sunrise and post-sunset peaks reproduced reasonably well. The agreement between the IRI predicted hmF2 values using CCIR M(30,000)F2 option and the observational ones is worst for the afternoon to post-midnight hours for the high solar activity year 2002. During daytime hours the agreement between the hmF2 values obtained with CCIR M(30,000)F2 option and the observational ones is best for summer season. The discrepancy between the observational hmF2 and that obtained with CCIR M(30,000)F2 option stem from the CCIR M(3000)F2 model, which does not produce the small scale structures observed in the measured M(3000)F2. 相似文献
3.
Yang Yi Shi Baochang He Yanyan 《遥测遥控》2007,(4)
基于自相关理想序列和正交矩阵建立一类统一的具有零(低)相关区的扩频序列构造方法,并对其相关特性进行分析和证明。该类方法可通过序列和矩阵的任意选取,统一地构造二元、三元、多相、复数的ZCZ(LCZ)序列集,且构造简单、形式统一,通用性更好,适用于准同步CDMA(QS-CDMA)系统。 相似文献
4.
5.
文章针对中国遥感高分辨率传输型相机的发展趋势,提出了一种高速低噪声的遥感CCD相机信号处理电路的设计方案。从信号完整性理论出发,利用Cadence软件进行了仿真与验证,取得了良好的效果。 相似文献
6.
基于特征点的地形数据存储模型 总被引:2,自引:1,他引:2
低空突防在现代战争中发挥着越来越重要的作用,而机载数字地图是现代自主式低空突防系统的一个关键子系统。突防区域内的三维地形数据是数字地图最重要的信息源,故数字地图子系统的成功构筑有赖于在机载环境下有效地存储三维地形数据。本文提出了一种基于地形特征点的三维地形存储模型,其中给出了地形特征点的提取方法及地形特征点的存储编码方式。研究表明,该存储模型可大大减小地形数据的存储空间,并有利于提高三维地形的显示速度。 相似文献
7.
8.
利用液态浸渗技术制备了氧化铝纤维增强铝基复合材料。结果表明,在低压下使液态合金浸渗纤维预制件制备铝基复合材料是可行的,在浸渗过程中,液态合金的温度对浸渗压力有较大影响。所制备的复合材料组织均匀,基体中的共晶组织可依附在纤维表面形核生长。 相似文献
9.
孙红卫%凌英%顾兆旃%刘兰 《宇航材料工艺》2001,31(3):33-36
通过对延长硅橡胶密度烧蚀材料体系施工期的研究,发现酸酐固化剂可以将环氧改性硅橡胶低密度烧蚀材料的施工期延长到24h以上,从而可能实现真空热压罐大面积灌注密度烧蚀材料的成型工艺。通过对固化材料进行红外分析,发现加入酸酐固化剂后并未改变硅橡胶和环氧树脂各自的反应,没有新的反应特征峰出现,说明环氧和硅橡胶之间无反应,只是物理共混,从材料拉伸断面的扫描电镜观察可以证实硅橡胶和环氧树脂以海-岛结构存在。 相似文献
10.
V.D. Kuznetsov I.I. Sobelman I.A. Zhitnik S.V. Kuzin Yu.D. Kotov Yu.E. Charikov S.N. Kuznetsov E.P. Mazets A.A. Nusinov A.M. Pankov J. Sylwester 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The CORONAS-F mission experiments and results have been reviewed. The observations with the DIFOS multi-channel photometer in a broad spectral range from 350 to 1500 nm have revealed the dependence of the relative amplitudes of p-modes of the global solar oscillations on the wavelength that agrees perfectly well with the earlier data obtained in a narrower spectral ranges. The SPIRIT EUV observations have enabled the study of various manifestations of solar activity and high-temperature events on the Sun. The data from the X-ray spectrometer RESIK, gamma spectrometer HELICON, flare spectrometer IRIS, amplitude–temporal spectrometer AVS-F, and X-ray spectrometer RPS-1 have been used to analyze the X- and gamma-ray emission from solar flares and for diagnostics of the flaring plasma. The absolute and relative content of various elements (such as potassium, argon, and sulfur) of solar plasma in flares has been determined for the first time with the X-ray spectrometer RESIK. The Solar Cosmic Ray Complex monitored the solar flare effects in the Earth’s environment. The UV emission variations recorded during solar flares in the vicinity of the 120-nm wavelength have been analyzed and the amplitude of relative variations has been determined. 相似文献