磁场影响葡萄糖氧化酶活性的研究

以尼龙网作载体，用戊二醛交联将区区糖氧化酶（ＧＯＤ）固定装成酶柱并联结于流动体系中，采用流动注射分光光度法研究磁场对固定化ＧＯＤ催化活性的影响。结果表明，在０℃、５℃、４５℃下以１．０×１０＾－２ｍｏｌ．Ｌ＾－１的葡萄糖为底物及５５℃下以０．１ｍｏｌ＾－１的葡萄糖为底物时，０．２２Ｔ静有显著提高固定化ＧＯＤ的反应速度，且磁场效应与底物浓度及磁场作用时间有关。用动力学方法考察了不同强度的磁场对溶解Ｇ     

电液伺服加载的神经网络内部反馈控制

 针对电液伺服加载系统多余力问题,提出了一种反馈加载系统内部力差信号减少多余力的控制方法。为了消除液压非线性及参数变化等影响,进一步提出基于神经网络内部参考模型调节方法。该参考模型为无舵机扰动时的液压油缸负载压力方程,在加载过程中,将油缸的负载压力与参考模型输出比较,利用神经网络自适应调节能力,消除加载中舵机运动的速度和加速度干扰,同时也克服液压系统非线性,时变参数和扰动的影响,该方法有较好的适用性。     

KM6水平舱改造测控系统研制

宇航员出舱活动是我国载人航天发展战略的第二步——空间实验室工程的一项基本任务。为满足完成“SZ-7人-船-服”出舱活动联合试验任务的需要,必须需要对原有KM6水平舱进行适应性的功能改造。为了确保宇航员的生命安全,必须尽可能的提高整个控制系统的可靠性,。测控系统在总体结构上采用SIEMENS PCS7冗余集散控制系统的方式,对所有关键测控环节（包括控制计算机、CPU、电源、网络、I/O模块等）都进行了冗余备份,以确保宇航员出舱活动试验流程的顺利进行,并对重要操作中关键参数互联、互锁,杜绝误操作,确保有完善的系统监控和故障报警功能,。改造后通过多次调试和多种试验模式演练,各分系统和总控系统测控功能均达到设计指标要求。为人-舱-服联合试验提供了坚强的后盾。     

基于AOV图及二叉树的梯形图与指令表互换算法

通过对可编程逻辑控制器(Programma blelogic contro ller,PLC)的梯形图语言及指令表语言的分析,提出了基于AOV(Activity on vertex)有向图和二叉树实现梯形图与指令表程序相互转换的算法。转换算法将梯形图映射为AOV图,并由其建立二叉树来表示指令间的逻辑关系,通过遍历二叉树实现PLC梯形图与指令表的转换。文中给出一个转换实例,介绍了算法思想及其实现步骤。该算法具有通用性,适于复杂控制逻辑的梯形图,已成功用于水电自动化监控系统中的PLC编程软件平台。     

Variation of ionospheric electron and ion temperatures during periods of minimum to maximum solar activity by the SROSS-C2 satellite over Indian low and equatorial latitudes

To study the variation of ionospheric electron and ion temperatures with solar activity the data of electron and ion temperatures were recorded with the help of Retarding Potential Analyzer payload aboard Indian SROSS-C2 satellite at an average altitude of ∼500 km. The main focuses of the paper is to see the diurnal, seasonal and latitudinal variations of electron and ion temperatures during periods of minimum to maximum solar activity. The ionospheric temperatures in the topside show strong variations with altitude, latitude, season and solar activity. In present study, the temperature variations with latitude, season and solar activity have been studied at an average altitude ∼500 km. The peak at sunrise has been observed during all seasons, in both electron and ion temperatures. Further, the ionospheric temperatures vary with latitude in day time. The latitudinal variation is more pronounced for low solar activity than for high solar activity.     

Ionospheric variation at Thailand equatorial latitude station: Comparison between observations and IRI-2001 model predictions

In this paper, the F2-layer critical frequency (foF2) and peak height (hmF2) measured by the FM/CW ionosonde at Thailand equatorial latitude station, namely Chumphon (10.72°N, 99.37°E, dip 3.22) are presented. The measurement data during low solar activity from January 2004 to December 2006 are analyzed based on the diurnal, seasonal variation. The results are then compared with IRI-2001 model predictions. Our study shows that: (1) In general, both the URSI and CCIR options of the IRI model give foF2 close to the measured ones, but the CCIR option produces a smaller range of deviation than the URSI option. The agreement during daytime is generally better than during nighttime. Overestimation mostly occurs in 2004 and 2006, while underestimation is during pre-sunrise hours in June solstice in 2005. The peak foF2 around sunset is higher during March equinox and September equinox than the other seasons, with longer duration of maximum levels in March equinox than September equinox. Large coefficients of variability foF2 occur during pre-sunrise hours. Meanwhile, the best agreement between the observed foF2 and the IRI model is obtained in June solstice. (2) In general, The IRI (CCIR) model predicts the observed hmF2 well during daytime in June solstice from 2004–2006, but it overestimates during March equinox, September equinox and December solstice. For nighttime, the model overestimates hmF2 values for all seasons especially during March equinox and September equinox. However, the model underestimates hmF2 values during September equinox and for some cases during June solstice and December solstice at pre-sunrise. The agreement between the IRI model and the hmF2(M3000_OBS) is worst around noontime, post-sunset and pre-sunrise hours. All comparative studies give feedback for new improvements of CCIR and URSI IRI models.     

Antioxidant capacity reduced in scallions grown under elevated CO2 independent of assayed light intensity

Long-duration manned space missions mandate the development of a sustainable life support system and effective countermeasures against damaging space radiation. To mitigate the risk of inevitable exposure to space radiation, cultivation of fresh fruits and vegetables rich in antioxidants is an attractive alternative to pharmacological agents. However it has yet to be established whether antioxidant properties of crops can be preserved or enhanced in a space environment where environmental conditions differ from that which plants have acclimated to on earth. Scallion (Allium fistulosum) rich in antioxidant vitamins C and A, and flavonoids was used as a model plant to study the impact of a range of CO₂ concentrations and light intensities that are likely encountered in a space habitat on food quality traits. Scallions were hydroponically grown in controlled environmental chambers under a combination of 3 CO₂ concentrations of 400, 1200 and 4000 μmol mol⁻¹ and 3 light intensity levels of 150, 300, 450 μmol m⁻² s⁻¹. Total antioxidant activity (TAA) of scallion extracts was determined using a radical cation scavenging assay. Both elevated CO₂ and increasing light intensity enhanced biomass accumulation, but effects on TAA (based on dry weight) differed. TAA was reduced for plants grown under elevated CO₂, but remained unchanged with increases in light intensity. Elevated CO₂ stimulated greater biomass production than antioxidants, while an increase in photosynthetic photo flux promoted the synthesis of antioxidant compounds at a rate similar to that of biomass. Consequently light is a more effective stimulus than CO₂ for antioxidant production.     

基于扩展的UML活动图的质量工作流建模

本文使用了UML类图表达了工作流参考模型,统一了UML活动图与工作流过程模型的概念,并根据工作流的概念扩展了UML活动图,弥补了活动图的不足,并以实例说明。     

原子氧对航天器表面的剥蚀效应及其预报研究

文章论述了一个航天器表面原子氧通量和遭遇量预报模式的建立,并对影响航天器表面原子氧遭遇量的主要因素进行了讨论。最后用模式计算了2003～2006年间太阳同步轨道卫星表面原子氧遭遇量的情况。     

The longitudinal and hemispherical variation of the IRI’s foF2 estimates at ±40° dip angle around 95°E and 130°E sector under fluctuating solar flux conditions

The deviation of the IRI estimates of the monthly mean foF2 in the low mid latitude of 95°E–130°E longitude sector is investigated using simultaneous ground measurements at four stations during 2010–2014. The stations form two conjugate pairs of the same geo-magnetic latitude at two fixed longitudes enabling direct longitudinal and hemispheric comparison. The temporal, spatial, seasonal and solar activity variations of the deviations are discussed with reference to the longitudinal density variation in the transition region between low and midlatitudes. Cases of underestimation/overestimation as well as good estimate are noted. Underestimation (overestimation) in the daytime and overestimation (underestimation) in the nighttime of 95°E (130°E) are common. The longitudinal difference in the measurements suggests negative (positive) foF2 gradient from west to east in daytime (nighttime). In contrast, the IRI predicts flatter or increasing longitudinal profiles from 95°E to 130°E. The local time and longitudinal variation of the IRI deviations can be attributed to the combined role of the longitudinal EIA structure as well as midlatitude zonal wind-magnetic declination effect. The station/season independent deviations relate the role of solar activity representation in the IRI. These deviations may be attributed to the weak IRI response to rapid solar flux fluctuations.