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131.
由于发送端和接收端时钟的不一致性,导致低信噪比下阵列天线卫星移动通信的逐通道相关标校有很大的难度。在考虑易实现性和简易性基础上,提出了一种可以解决低信噪比下通道校正的多周期长时累积方法。该校准信号为由地面标校站产生的BPSK调制扩频信号,可以减少卫星设计的复杂度,且在不中断用户数据传输的基础上实现在线标校。该方法通过对接收信号打标、速率匹配等措施来解决收发时钟不一致导致的码偏和频偏问题。研究结果可以为阵列天线卫星通信技术提供支持。 相似文献
132.
H.S. Ahluwalia 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
The common methodologies used to predict the smooth sunspot number (SSN) at peak (Rmax) and the rise time (Tr) for a cycle are noted. The estimates based on geomagnetic precursors give the best prediction of Rmax for five SSN cycles (20–24). In particular, an empirical technique invoking three-cycle quasi-periodicity (TCQP) in Ap index has made accurate predictions of Rmax and Tr for two consecutive SSN cycles (23 and 24). The dynamo theories are unable to account for TCQP. If it endures in the 21st century the Sun shall enter a Dalton-like grand minimum. It was a period of global cooling. The current status of the ascending phase of cycle 24 is described and the delayed reversal of the solar polar field reversal in the southern hemisphere in September 2013 is noted. 相似文献
133.
利用CAIV技术分别建立反舰导弹的作战效能模型和总拥有费用模型,并以权衡空间为约束条件,以费用最低为目标,建立保障性指标权衡优化模型。该方法可以为导弹武器装备保障性指标论证工作提供必要的理论基础和技术支持。 相似文献
134.
135.
火箭引射模态下主火箭总压与RBCC发动机的匹配性 总被引:4,自引:0,他引:4
基于传统的"等压面假设"理论,建立了RBCC发动机主火箭的引射性能分析模型,研究了主火箭总压与RBCC发动机的匹配性。研究结果表明,若隔离段通道面积比小于0.65,在主火箭总压较低条件下,隔离段内二次流容易达到壅塞,无法进一步提高空气流量;在地面静止状态下,随主火箭总压增加,空气流量逐步增大,等压面上形成Fabri壅塞后,进一步增加主火箭总压,反而会降低空气流量;在火箭引射模态下,RBCC发动机的工作状态可细分为引射作用占主导地位的进气道亚临界状态和临界状态、冲压作用占主导地位的进气道超临界状态,其分界马赫数分别约为0.7和1.5。 相似文献
136.
《中国航空学报》2021,34(10):282-292
The accurate measurement of surfaces of large aviation components is vital for the assessment of manufacturing and assembly quality of such components. To satisfy the measurement requirement of large-size components, most current researches pay more attention to combined measurement methods utilizing different measuring instruments, but the related researches on error analysis and optimization methods are not taken enough attention. This paper proposes a combined laser-assisted measurement method with feature enhancement techniques, and it also develops an error propagation model of the main factors affecting the overall measurement error in detail. Firstly, the surface of a large-size component is measured by the measurement system at multiple stations. Secondly, a control point coordinate system is established as a bridge to unify all local measurement data into the global coordinate system. To improve the overall measurement accuracy, the pixel extraction error as a key factor causing the overall measurement error is analyzed in detail. Next, the error propagation model is established, and some optimization strategies of layout for minimizing measurement error and transformation error are researched. Finally, experiments are carried out to verify the effectiveness of the proposed method. The results show that the measurement error of the proposed method reaches 0.073% and 0.14% with a 1D standard ruler and a flat plate, respectively. 相似文献
137.
138.
内并联式TBCC进气道模态转换过程流动特性分析 总被引:4,自引:0,他引:4
针对组合动力(TBCC)进气道模态转换过程中出现的非定常气动现象,采用稳态/非稳态数值模拟方法对相关流动特性及其影响因素与流动机理开展了研究。结果表明:由涡轮发动机工作状态向冲压发动机工作模态转换过程中,进气道内出现结尾激波沿流向前后振荡现象,振荡频率约为130Hz;当冲压流道反压引起的激波未前传至模态转换分流板前时,冲压发动机工作状态对结尾激波振荡不产生影响。在相同的发动机工作状态下,随着模态转换速度的增加,结尾激波振荡频率逐渐增大。文中研究的进气道内结尾激波振荡现象可通过亚声速管道内波的传播理论进行解释和分析。 相似文献
139.
空气预冷发动机及微小通道流动传热研究综述 总被引:1,自引:0,他引:1
首先针对发动机空气预冷系统的特点,将现有的预冷机制分为四种类型,包括燃料预冷、质量喷注预压缩冷却、燃料预冷和质量喷注预压缩冷却组合预冷以及其他流体预冷,并分别介绍了每种预冷机制的代表性发动机循环以及技术特点。调研发现,微小通道结构的预冷器具有很高的散热能力和紧凑度,优势显著。英国Skylon空天飞机的预冷却组合循环发动机(SABRE)其微通道结构预冷器具有极高换热能力。对SABRE的预冷器及相关研究进行详细分析,强调微小通道强化换热对提高发动机性能的重要作用。通过对微小通道中单相气态流动换热研究的调研发现,微尺度流动传热机理仍存在诸多分歧,理论发展不完善,需要深入开展微小通道强化传热研究,尤其对于高速高内外温差条件下微小尺度复杂结构空间内流动传热机理需要深入探索。 相似文献
140.
Sneha Yadav R.S. Dabas Rupesh M. Das A.K. Upadhayaya A.K. Gwal 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
The paper deals with the study of temporal and spatial variation of equatorial ionization anomaly (EIA) phenomenon along with its dependence on solar activity and season during the 19th solar cycle by using seven Indian ionosonde stations. Present study is an attempt to carry out the comprehensive study of EIA by using the limited number of ground based instruments. This has been achieved by performing the Gaussian fitting over the latitudinal distribution of F2-region critical frequency (foF2) data. Results reveal that the phenomenon of EIA has a strong dependence on solar activity and seasons. The EIA crest exhibits the feature of latitudinal shifting and expansion with increasing solar activity. It is found out that the effect of solar cycle and seasons on EIA is local time dependent. The observations were also compared with the IRI-2001 model predictions and results reveal that the model values are in general agreement with the observed values with some discrepancies, particularly during the high solar activity period and morning sector. The results have been discussed in the light of relative contribution from transequatorial interhemispheric neutral wind and strength of equatorial fountain process during different local time, season and solar activity levels. Furthermore, an attempt is made to parameterize the location and foF2 of the EIA crest by using the regression analysis. These results can be used to predict the latitudinal position and foF2 of the EIA crest for any given 12-month running average sunspot number (R12). 相似文献