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排序方式: 共有245条查询结果,搜索用时 48 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.
李大耀 《运载火箭与返回技术》2005,26(3):1-4
在中国第一个实用探空火箭系列——T-7系列探空火箭首次发射成功45周年之际,回顾了该系列火箭的研制由来和基本情况,论述了该系列火箭对中国开发中层大气和太空所起到的探路作用。 相似文献
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深空探测火箭的发展及应用 总被引:1,自引:0,他引:1
阐述了国外深空探测火箭的种类、结构及技术性能,对其、发展现状及趋势进行了论述,并简要介绍了国内探测火箭的发展状况。 相似文献
6.
在单天线横截面方向图计算公式的基础上,计算了圆柱体导弹引信双天线、三天线和四天线布局的方向图。讨论了不同布局下引信载频、弹体直径及天线布局与作用盲点的关系。双天线布局的实际测试表明,测试值与计算结果较为吻合,所用的计算方法正确,可为引信天线布局与引信工作频率确定提供设计依据。 相似文献
7.
Paul Withers T.J. Stubbs E. Mazarico 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(12):4099-4109
The existence of a “dense” lunar ionosphere has been controversial for decades. Positive ions produced from the lunar surface and exosphere are inferred to have densities that are – m?3 near the surface and smaller at higher altitudes, yet electron densities derived from radio occultation measurements occasionally exceed these values by orders of magnitude. For example, about 4% of the single-spacecraft radio occultation measurements from Kaguya/SELENE were consistent with peak electron densities of m?3. Space plasmas should be neutral on macroscopic scales, so this represents a substantial discrepancy. Aditional observations of electron densities in the lunar ionosphere are critical to resolving this longstanding paradox. Here we theoretically assess whether radio occultation observations using two-way coherent S-band radio signals from the Lunar Reconnaissance Orbiter (LRO) spacecraft could provide useful measurements of electron densities in the lunar ionosphere. We predict the uncertainty in a single LRO radio occultation measurement of electron density to be m?3, comparable to occasional observations by Kaguya/SELENE of a dense lunar ionosphere. Thus an individual profile from LRO is unlikely to reliably detect the lunar ionosphere; however, averages of multiple (10) LRO profiles acquired under similar geophysical and viewing conditions should be able to make reliable detections. An observing rate of six ingress occultations per day (2000 per year) could be achieved with minimal impact on current LRO operations. This rate compares favorably with the 378 observations reported from the single-spacecraft experiment on Kaguya/SELENE between November 2007 and June 2009. The large number of observations possible for LRO would be sufficient to permit wide-ranging investigations of spatial and temporal variations in the poorly understood lunar ionosphere. These findings strengthen efforts to conduct such observations with LRO. 相似文献
8.
T. S. Bastian 《Space Science Reviews》1994,68(1-4):261-274
Radio and X-ray observations of stellar flares provide the most direct probes of energy relaase particle acceleration, and energy transport on stars other than the Sun. In this review, the observational basis for our understanding of the flare phenomenon on other stars is briefly described and outstanding interpretive and theoretical issues are discussed. I shall confine my attention to objects which are solar-like, to the extent that they possess deep convective envelopes and display activity which is presumed to be magnetic in origin. These include pre-main sequence objects, classical flare stars, and close binaries. Future directions are briefly discussed. 相似文献
9.
在鸭式布局的基础上 ,对飞行器各部件及部件间的连接方式进行了外形隐身设计。对初步形成的鸭翼 -翼身融合体改变机身头部形状和立尾配置等进行 RCS优化。给出了飞行器各种状态下的 RCS平均值和迎头± 45°区内的 RCS值。测试结果表明 ,尖头机身、 30°双立尾 (立尾与垂直平面成± 30°角 )的鸭翼 -翼身融合体的 RCS值最小。对 RCS优化后的外形 ,风洞测力试验表明其气动性能也较好 (最大升阻比达到 8,失速迎角超过 2 6°) 相似文献
10.
Guojun Wang Jiankui Shi Weihua Bai Ivan Galkin Zeng Wang Yueqian Sun 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(10):3119-3130
Global observations of S4 amplitude scintillation index by the GPS Occultation Sounder (GNOS) on FengYun-3 C (FY3C) satellite reveal global dynamic patterns of a strong pre-midnight scintillations in F-region of the ionosphere during the St. Patrick’s Day geomagnetic super storm of 17–19 March 2015. The observed strong scintillations mainly occurred in the low latitudes, caused by equatorial plasma bubbles. During the main storm phase (March 17), the scintillations were first triggered in the New Zealand sector near 160°E longitudes, extending beyond 40°S dip latitude. They were also enhanced in the Indian sector, but significantly suppressed in East Asia near 120°E longitude and in Africa around 30°E longitude. During the initial recovery phase (March 18–19), the global scintillations were seldom observed in GNOS data. During the later recovery phase (after March 19), the scintillations recovered to the pre-storm level in Indian, African, and American sectors, but not in East Asian and any of Pacific sectors. These results closely correlate with observations of the density depletion structures by the Communication/Navigation Outage Forecasting System (C/NOFS) satellite, and ground-based instruments. Such consistency indicates reliability of our scintillation sensing approach even in a case-by-case comparison study. The prompt penetration electric field and disturbance dynamo electric field are suggested as the main factors that control the enhancement and inhibition of the scintillations during the storm, respectively. 相似文献