大阻尼高刚度复合材料仪表板的设计结构与工艺研究

设计了一种五层夹芯多层阻尼薄膜嵌入的复合材料仪表板结构,并采用多次热压罐固化成型工艺来制作该大阻尼高刚度复合材料仪表板.它们分别是:上、下蒙皮和中心层的制作,上、下蒙皮和中心层与泡沫塑料的粘接与紧固件的预埋,孔的修正及仪表板的包边加工.通过成形质量检验和加载试验,验证了成形工艺的可行性和合理性.     

基于VALOR NPI的航空电子模块DFM分析实现

为有效解决设计缺陷造成的航空电子模块可制造性问题,结合航空电子模块产品特点和工艺技术水平,提出建设基于VALOR的航空电子模块可制造性设计自动化设计平台,实现DFM自动化分析与设计,阐述了DFM设计的必要性、技术原理和实现过程,提出了“三库”构建方法和基于物料清单的印制电路板数据分析方法,应用结果表明,提出的方法能够覆盖PCB可制造性问题,提高分析效率。     

高效湿法缠绕用环氧树脂配方及其复合材料性能

针对高质固体火箭发动机壳体高效的生产要求对不同官能度环氧树脂复配体系的工艺性进行研究,重点开展了多官能团环氧树脂复配体系配方设计及力学性能研究,分别采用DSC(差示扫描分析)、黏度测试进行固化特征温度、固化反应动力学及工艺适用期研究,并最终制备单向层合板及NOL(the Naval Ordnance Laboratory)环进行复合材料性能的测试分析。研究结果表明:三官能度复配的环氧树脂能满足高效湿法缠绕要求。当三官能度的TDE-85质量分数为25%时,综合性能达到最优,适用期仅为120 min,拉伸强度为973 MPa,弯曲强度为115 MPa,玻璃化转变温度高达466 K,较最低值分别提高363%、159%、258%。该树脂体系与纤维匹配性好,复合材料性能优良,NOL环拉伸强度与层间剪切强度分别为256 GPa、744 MPa,纤维强度利用率达766%,适用于固体火箭发动机湿法缠绕成形。     

不同酚醛树脂对芳纶纸蜂窝性能的影响

为研究酚醛树脂对芳纶纸蜂窝性能的影响,本文采用两种不同的酚醛树脂制备芳纶纸蜂窝芯材,对所制备蜂窝芯材的压缩性能和剪切性能进行测试,同时结合蜂窝端面树脂分布观察、树脂与芳纶纸接触角测量等方法,分析了两种树脂所制备蜂窝芯材性能出现差异的原因,结果表明：树脂中溶剂水的挥发速度、树脂与芳纶纸之间的表面张力会影响树脂在蜂窝壁上的树脂分布;蜂窝芯材树脂含量相同时,其节点两侧的树脂胶柱有利于提高蜂窝芯材压缩强度,但树脂堆积在节点后会降低蜂窝壁厚,造成蜂窝的剪切强度和模量下降。     

Median filtering algorithms for multichannel detectors

Particle detectors of worldwide networks are continuously measuring various secondary particle fluxes incident on Earth surface. At the Aragats Space Environmental Center (ASEC), the data of 12 cosmic ray particle detectors with a total of ∼280 measuring channels (count rates of electrons, muons and neutrons channels) are sent each minute via wireless bridges to a MySQL database. These time series are used for the different tasks of off-line physical analysis and for online forewarning services. Usually long time series contain several types of errors (gaps due to failures of high or low voltage power supply, spurious spikes due to radio interferences, abrupt changes of mean values of several channels or/and slowly trends in mean values due to aging of electronics components, etc.). To avoid erroneous physical inference and false alarms of alerting systems we introduce offline and online filters to “purify” multiple time-series. In the presented paper we classify possible mistakes in time series and introduce median filtering algorithms for online and off-line “purification” of multiple time-series.     

坐标测量机的验收检测标准及校准规范的再探讨

发现GB/T 16857 eqv ISO 10360《产品几何量技术规范(GPS)坐标测量机的验收检测和复检检测》及JJF 1064—2004《坐标测量机校准规范》存在的不足。提出在GB/T 16857 eqv ISO 10360系列标准中增补测量软件包的质量要求和测试标准的建议。以实现对测量软件质量的评价,达到测量机性能的全面验收检测。     

Comparison of peak characteristics of F2 ionospheric layer over Tehran region at a low solar activity period with IRI-2001 and IRI-2007 models predictions

In the present work values of peak electron density (NmF2) and height of F2 ionospheric layer (hmF2) over Tehran region at a low solar activity period are compared with the predictions of the International Reference Ionosphere models (IRI-2001 and IRI-2007). Data measured by a digital ionosonde at the ionospheric station of the Institute of Geophysics, University of Tehran from July 2006 to June 2007 are used to perform the calculations. Formulations proposed by  and  are utilized to calculate the hmF2. The International Union of Radio Science (URSI) and International Radio Consultative Committee (CCIR) options are employed to run the IRI-2001 and IRI-2007 models. Results show that both IRI-2007 and IRI-2001 can successfully predict the NmF2 and hmF2 over Tehran region. In addition, the study shows that predictions of IRI-2007 model with CCIR coefficient has closer values to the observations. Furthermore, it is found that the monthly average of the percentage deviation between the IRI models predictions and the values of hmF2 and NmF2 parameters are less than 10% and 21%, respectively.     

CCSDS在我国航天领域的应用展望

CCSDS(空间数据系统咨询委员会)建议有利于增强测控系统互联互通互支持能力,满足未来航天任务对空间信息高速传输及灵活高效信息调度机制的要求,应当作为我国构建天地一体化信息网络的首选标准。提出了加强顶层设计、循序渐进地推进CCSDS建议在我国实现工程化应用的总体思路,并提出在应用过程中应当注重创新任务操作模式、关注信息安全、深化关键技术研究与验证。     

Longitudinal variation of the equatorial ionosphere: Modeling and experimental results

We describe a new version of the Parameterized Regional Ionospheric Model (PARIM) which has been modified to include the longitudinal dependences. This model has been reconstructed using multidimensional Fourier series. To validate PARIM results, the South America maps of critical frequencies for the E (foE) and F (foF2) regions were compared with the values calculated by Sheffield Plasmasphere-Ionosphere Model (SUPIM) and IRI representations. PARIM presents very good results, the general characteristics of both regions, mainly the presence of the equatorial ionization anomaly, were well reproduced for equinoctial conditions of solar minimum and maximum. The values of foF2 and hmF2 recorded over Jicamarca (12°S; 77°W; dip lat. 1°N; mag. declination 0.3°) and sites of the conjugate point equatorial experiment (COPEX) campaign Boa Vista (2.8°N; 60.7°W; dip lat. 11.4°; mag. declination −13.1°), Cachimbo (9.5°S; 54.8°W; dip lat. −1.8°; mag. declination −15.5°), and Campo Grande (20.4°S; 54.6°W; dip lat. −11.1°; mag. declination −14.0°) have been used in this work. foF2 calculated by PARIM show good agreement with the observations, except during morning over Boa Vista and midnight-morning over Campo Grande. Some discrepancies were also found for the F-region peak height (hmF2) near the geomagnetic equator during times of F₃ layer occurrences. IRI has underestimated both foF2 and hmF2 over equatorial and low latitude sectors during evening-nighttimes, except for Jicamarca where foF2 values were overestimated.     

Variation in the ionospheric propagating factor M(3000)F2 at Ouagadougou,Burkina Faso

We use hourly monthly median values of propagation factor M(3000)F2 data observed at Ouagadougou Ionospheric Observatory (geographic12.4°N, 1.5°W; 5.9^o dip), Burkina Faso (West Africa) during the years Januar1987–December1988 (average F10.7 < 130 × 10⁻²² W/m²/Hz, representative of low solar flux conditions) and for January 1989–December1990 (average F10.7 ? 130 × 10⁻²² W/m²/Hz, representative of high solar epoch) for magnetically quiet conditions to describe local time, seasonal and solar cycle variations of equatorial ionospheric propagation factor M(3000)F2 in the African region. We show that that seasonal trend between solar maximum and solar minimum curves display simple patterns for all seasons and exhibits reasonable disparity with root mean square error (RMSE) of about 0.31, 0.29 and 0.26 for December solstice, June solstice and equinox, respectively. Variability Σ defined by the percentage ratio of the absolute standard deviation to the mean indicates significant dissimilarity for the two solar flux levels. Solar maximum day (10–14 LT) and night (22–02 LT) values show considerable variations than the solar minimum day and night values. We compare our observations with those of the IRI 2007 to validate the prediction capacity of the empirical model. We find that the IRI model tends to underestimate and overestimate the observed values of M(3000)F2, in particular, during June solstice season. There are large discrepancies, mainly during high solar flux equinox and December solstice between dawn and local midnight. On the other hand, IRI provides a slightly better predictions for M(3000)F2 between 0900 and 1500 LT during equinox low and high solar activity and equinox high sunspot number. Our data are of great importance in the area of short-wave telecommunication and ionospheric modeling.