高空气球太阳能电池标定用太阳跟踪控制技术

高空气球标定的太阳能电池是可被用于地面太阳模拟器和太阳光光强检测的标准电池。首先,给出了由飞行气球搭载的高空太阳能电池标定所使用的太阳跟踪控制系统设计方法,包括基于STM32的太阳跟踪控制系统硬件设计方案、混合自动追踪控制策略、软件开发与实现方法、高空跟踪控制技术问题解决方案以及高空标定试验等。同时,解决了高空气球电池标定用太阳跟踪控制系统在极端环境下高可靠性、连续追踪和防抖动等关键技术问题。试验结果为气球飞行高度32km,平飘时间超过2h,太阳跟踪偏差小于1°。经初步分析,高空太阳跟踪控制系统标定测试结果合理可靠,工作性能稳定,为中国高空气球太阳能电池AM0标定用太阳跟踪控制系统的研究提供了新思路。     

微小型数据采集系统优化设计方法研究

微小型数据采集系统一般是基于微控制器进行设计的,存储设备主要为SD卡,由于微控制器资源有限,因此很难在保证微小型数据采集系统较高采集速度的同时保证采集系统的可靠性.针对该问题,本文分析了影响数据采集系统采集速率及可靠性的主要影响因素,推导了DMA缓冲区设置大小与数据采集系统采集速率及可靠性之间的模型,并设计了数据采集系统主要参数标定与验证试验.试验结果表明,本文提出的数据采集系统设计方法合理、可根据数据采集处理器内存大小、SD卡文件系统性能指标设计数据采集系统,确保数据采集系统的可靠性,对提高系统设计效率、降低微小型数据采集系统的设计成本以及后续改进完善数据采集系统奠定了重要的理论基础.     

基于STM32的电池不正确使用检测装置设计

鉴于电池错误使用检测中,存在燃烧和爆炸的危险,为了测试人员和设备的安全,采用了STM32F103 VET6微控制器平台作为下位机,个人电脑作为上位机,在电流检测中采用霍尔电流传感器,设计了一种的分离式电池错误使用数据采集处理装置,上位机通过串口通讯,对下位机发送过来的检测的电压、电流数据进行采集和处理,在上位机中显示各个电池通道的数据并进行存储。通过软硬件设计制作,实现了装置功能,保证了测试人员的安全。     

PIC16F877实现CAN总线分布式数据采集系统

叙述了一种采用CAN总线通信来实现分布式数据采集的设计方法;介绍了用PIC16F877通过SPI方式直接对MCP2510进行操作,与带智能适配卡的PC机实现CAN通信,并对CAN控制器MCP2510作了分析;给出了系统结构框图与部分硬件图,以及给出了软件设计思路。该基于CAN总线的分布式数据采集系统是一种高可靠性、实时性的系统。     

基于SOC的ACAS无线电高度信号激励测试的设计

本文介绍了一种以SOC为核心芯片用于机载防撞系统(ACAS)中符合ARINC552A标准无线电高度信号激励测试的软硬件设计方法.采用C8051F020型SOC芯片及OPA552等芯片搭建仿真电路,利用PDIUSBD12接口芯片建立与工控机的通讯,依据ARINC552A标准,用C51编写仿真控制程序,将仿真的ACAS无线...     

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.     

生物质催化热解油的GC-MS分析

通过酸洗脱灰及脱灰后添加催化剂DHC-32等不同预处理方式处理的玉米秸秆为原料,在小型固定床反应器上制取生物油,用GC-MS分析技术对生物油的成分进行分析。研究结果表明：矿物质的存在降低了热解油的产率,矿物质和催化剂对生物油中化学组分具有显著影响。     

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.     

重量的一种遥测式监测系统

本文提出一种重量信号的无线传输和测量方法。重量信号经传感顺转换成电信号，再经Ｖ／Ｆ变换后调频发射，接收信号解调后单片机处理。单片机的信号处理采用电子计数器测频方法，经过计算送显示单元，实现重量信号的遥测。     

Effects of TADs on the F region of the mid-latitude ionosphere during an intense geomagnetic storm

Based on observations of two ionosondes at Wuhan and Kokubunji, this paper presents effects of TADs on the daytime mid-latitude ionosphere during the intense geomagnetic storm on March 31, 2001. During a positive ionospheric storm, the start of the enhancement of the foF2 (F2 peak plasma frequency) at Wuhan lags that at Kokubunji by 15 min, which corresponds to the time interval of traveling atmospheric disturbances (TADs’) propagation from Kokubunji to Wuhan. Associated with the uplifting of the hmF2 (height of F2 peak) caused by TADs, it is observed by the two ionosondes that the F1 cusp becomes better developed. Therefore, during a geomagnetic storm, TADs originating from the auroral oval may have a strong influence on the shape of the electron density profile in the F1 region ionosphere at middle latitudes. It is highly likely that TADs are responsible for the evolution of the F1 cusp.