智慧温室群远程监控系统通信设计

温室监控系统是对温室环境中温度、湿度、光照度等环境因子实施监测与调控的农业设施,可确保农作物获得最适宜的生长发育环境。针对现有温室监控系统在通信上存在距离受限、组网复杂、能耗高且基本仅能实现单个温室控制的问题,设计了一种基于LoRa和NB-IoT相结合的智慧温室群远程监控系统通信模式。该模式以STM32F103C8T6单片机为核心控制器件,采用ATK-LoRa SX1278和NB-IoT模块自组无线通信网实现数据的远程交互。测试结果表明：采用该通信模式可实现温室群中各温室间距离在2km范围内的数据采集、处理和传输,其通信距离远、功耗低,数据传输可靠性符合现代化农业物联网的需求。     

考虑滑流影响的埋入式进气道气动特性分析与流动控制研究

研究滑流对埋入式进气道性能的影响机理对于发动机的稳定性具有重要意义。针对某型涡桨发动机 滑油散热器进排气道系统,基于 CFD技术建立系统的螺旋桨滑流与滑油散热器内流一体化数值模拟方法,进 行考虑滑流影响的滑油散热系统埋入式进气道气动设计仿真分析;针对埋入式进气道由于吸入边界层低能气 流导致通过散热器流量低的问题,设计4组涡流发生器进行主动流动控制。结果表明:滑流使得进气道中的气 流偏离,难以形成稳定漩涡,容易发生流动分离;而合理设计的涡流发生器可以有效改善埋入式进气道内流场 特性,并使通过散热器的流量提高12%。     

某测试台谐波摇摆运动的控制

某测试台主要运动方式为三自由度正弦摇摆Asinωt,三次谐波摇摆。本文详细阐述了该设备三次谐波谱的精密运动控制、在线实时轨迹显示和静态FFT分析。     

基于混合编程技术的AOCC应用软件快速仿真平台

介绍基于混合编程技术的AOCC应用软件的快速仿真平台的整体框架设计以及具体实现．基于该方法构建的快速仿真平台，能够满足软件开发人员对基于8086汇编语言开发的AOCC应用软件开、闭环调试和测试的要求，对提高软件的开发效率和保证软件的质量有积极意义．     

Matching suitable feature construction for SAR images based on evolutionary synthesis strategy

In the paper,a set of algorithms to construct synthetic aperture radar（SAR）matching suitable features are frstly proposed based on the evolutionary synthesis strategy.During the process,on the one hand,the indexes of primary matching suitable features（PMSFs）are designed based on the characteristics of image texture,SAR imaging and SAR matching algorithm,which is a process involving expertise;on the other hand,by designing a synthesized operation expression tree based on PMSFs,a much more flexible expression form of synthesized features is built,which greatly expands the construction space.Then,the genetic algorithm-based optimized searching process is employed to search the synthesized matching suitable feature（SMSF）with the highest effciency,largely improving the optimized searching effciency.In addition,the experimental results of the airborne synthetic aperture radar ortho-images of C-band and P-band show that the SMSFs gained via the algorithms can reflect the matching suitability of SAR images accurately and the matching probabilities of selected matching suitable areas of ortho-images could reach 99±0.5%.     

航天器共因失效分析与预防初探

简要介绍了共因失效相关概念及分析方法,通过共因失效案例分析,对航天器如何开展共因失效分析以及如何预防共因失效进行了初步探讨,提出了航天器开展共因失效分析的定性和定量方法以及预防共因失效的措施。     

频域盲源分离的非圆信号推广

作为盲源分离（BSS）问题的最有效解决方法之一,独立分量分析（ICA）算法可以分为时域和频域算法两类.将时域盲源分离的快速算法推广到频域,通过在频域中应用非圆信号的伪协方差矩阵,推导出一个新的固定点算法来解决线性瞬时混合的非圆信号盲源分离（BNSS）问题.仿真实验验证了该算法的有效性.     

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。     

酸性磺酞类染料共振Rayleigh散射光谱法测定奈替米星

用共振Rayleigh散射（RRS）光谱研究了酸性磺酞类染料溴甲酚绿和溴酚蓝分别与奈替米星的相互作用.溴甲酚绿和溴酚蓝在酸性介质中分别与奈替米星相互作用,导致RRS光谱显著增强,最大的RRS峰分别位于606nm和572nm处,散射强度与奈替米星的质量浓度在一定的范围内成正比.此方法具有很高的灵敏度,对于奈替米星的检测限（3σ）分别为30ng/mL和10ng/mL,据此发展了一种测定奈替米星的新方法.     

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.