一种应用于半闭环低刚度TVC伺服系统的力矩反馈控制方法

针对新型火箭发动机喷管刚度低、伺服系统呈半闭环结构导致的伺服系统谐振和快速性之间难以调和的问题,以上面级电动伺服系统为研究对象,对机构参数与系统性能之间的关系进行了仿真研究,提出了一种新的谐振抑制控制方法,引入力矩反馈使伺服机构具有力矩控制能力。仿真结果表明,提出的力矩反馈控制方法具有比陷波算法更优的谐振抑制能力,运算量并未增加,且涉及的参数均可通过测试得到,调试难度有所降低。     

非热压罐预浸料成型技术研究进展

非热压罐成型(out of autoclave process,OoA)技术是实现结构复合材料低成本制造的有效途径,是当前复合材料研究领域的热点之一。本文介绍了OoA成型复合材料国内外的研究前沿以及在航空航天领域的应用现状,从材料体系和成型工艺两大方面总结了OoA成型过程中的缺陷控制方法。在OoA预浸料成型技术中,可通过尽量减少树脂体系中挥发物含量、精细调控树脂体系反应和流变特性、控制预浸料中纤维和树脂的浸润程度、优化成型工艺等手段有效降低复合材料的孔隙率等缺陷。     

低轨卫星可控式冗余分包遥测技术

随着卫星功能日趋复杂,遥测参数越来越多,处理要求越来越快,遥测设计面临越来越大的压力,必须拓展新的设计思路.本文讨论了一种低轨卫星可控式冗余分包遥测技术,更好地缓解遥测信道“瓶颈”,满足用户多样化的遥测需求,提高卫星遥测能力.该设计采用PCM（Pulse Code Modulation,脉冲编码调制）遥测和分包遥测相结合的方案,在信道资源有限,遥测参数庞大、用户需求多样的约束条件下,通过星载软件模式控制的方法实现了动态可编程遥测处理和遥测数传通道的冗余处理,提高了遥测信道的资源利用率、遥测设计的灵活性和系统的可靠性,该技术已成功应用于某在轨卫星,并被多颗在研卫星所采用.     

低轨星座/惯导紧组合导航技术研究CSCD

现有低轨(LEO)卫星导航研究主要以低轨星座独立导航定位和增强全球卫星导航系统(GNSS)导航定位为主,对低轨卫星和惯性导航系统(INS)组合导航技术研究较少。本文面向应用较小规模低轨星座资源实现米级定位精度的需求,提出了一种低轨星座/惯导紧组合导航方法,系统性地分析了不同规模低轨星座、不同精度级别惯导器件以及不同导航信号播发频度下组合导航定位的性能,并利用构建的仿真试验系统进行了低轨星座/惯导紧组合导航方法的仿真试验验证。试验结果表明,相较于低轨星座独立导航,低轨星座/惯导紧组合导航在星座不满足四重覆盖时仍能达到米级定位精度,并且在低轨星座规模较小和导航信号播发频度较低时,惯导测量精度对组合导航定位精度影响明显。研究结果表明,在利用低轨卫星进行导航时,通过引入惯性观测辅助低轨卫星导航,可有效提高导航效能和精度,为低轨星座和导航信号播发方式设计带来更多的选择。     

AP/HTPB复合推进剂低压燃烧特性数值研究

为研究AP/HTPB复合推进剂低压燃烧特性,使用二维三明治模型进行了数值仿真研究。该模型使用简化的四步总包反应机理,考虑燃烧过程中的燃面退移,计算时大粒径AP取平均粒径,小粒径AP采用“均质黏合剂假设”,认为其与HTPB组成“均质黏合剂”。在0.02MPa-0.08MPa的压强下进行了仿真,并与高压（5MPa）下的燃烧仿真进行对比。结果表明,低压下固相AP对黏合剂的传热导致了交界面处燃面的下陷,下陷程度随压强减小而增大;随着燃烧的进行燃面各点燃速趋于一致,燃面形状不再改变。低压下气相反应表现为预混燃烧,初焰为主导反应。低压下燃速仿真与实验值基本一致,压强指数小于高压下的压强指数。     

热敏电阻低温测量方法研究

介绍了低温热敏电阻传感器低温标定的测量方法,分析了测量电路的引线绝缘电阻对热敏电阻传感器测量结果的影响,阐述了几种测量方法的优缺点。     

在轨航天器动力学参数辨识技术研究

针对在轨航天器低频密集和辨识时激励源有限且难于测量等特点,开展了适用于低频密集模态且不需激励信息的在轨航天器动力学参数辨识方法的研究,探讨了直接利用在轨响应数据在频域内辨识航天器动力学参数的技术;并根据在轨航天器低频密集特点,设计了在轨航天器动力学参数辨识仿真试验系统,对该辨识方法进行了试验验证。     

Global validation of IRI TEC for high and medium solar activity conditions

The IRI model offers a choice of options for the computation of the electron density profile and electron content (TEC). Recently new options for the topside electron density profile have been developed, which have a strong impact on TEC. Therefore it is important to test massively the IRI and the new options with experimental data. A large number of permanent stations record dual frequency GPS data from which it is possible to obtain TEC values. Thirty-one worldwide distributed stations have been selected to investigate the capabilities of the IRI to reproduce experimental TEC. Data for years 2000 (high solar activity) and 2004 (medium solar activity) have been analyzed computing modeled values with the IRI-2001 and the IRI-2007-NeQuick topside options. It is found that IRI-2007-NeQuick option generally improves the estimate of the slant TEC, especially in the case of high latitudes stations during high solar activity.     

低频超声检测探头的研制

介绍了低频超声检测探头的结构，设计方法，制作工艺。对研制的探头性能指标进行了测量，指出了改进其性能还待研究的问题。     

Rapid ionospheric variations at high latitudes: Focusing on Greenland

The Helheim glacier, located in southeast Greenland, has more than ten campaign-type Global Positioning System (GPS) sites; data processing led to the observation of a very rapid change in the ionospheric delay. To identify the cause of these sporadic disturbances, we analyzed the slant total electron content (STEC), single-differenced STEC (SD-STEC) and scintillation proxy index called the delta phase rate (DPR). From this analysis, the abrupt change of those ionospheric indicators was attributed to the line-of-sight direction to the satellite and the temporal sequence of the event was found to be highly correlated with the geometry of the GPS sites. In addition, the disturbance based on the result of SD-STEC occurred mostly during the night, from 17 UTC through 7 UTC, and across a band spanning the east-west direction. Based on the DPR indices obtained from GPS stations distributed across all of Greenland, Iceland, and northeastern Canada, the rapid ionospheric variation was found to be correlated with the time of the day and the geomagnetic latitude of the station. The disturbance was larger at the relatively low geomagnetic latitudes at night but was more significant at higher latitudes in the daytime. These rapid ionospheric variations tended to appear in band shapes parallel to the geomagnetic field. These results allow us to attribute such disturbance observed at the Helheim glacier to aurora-related phenomena.