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1.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2007,39(5):661-667
Monthly median values of foF2, hmF2 and M(3000)F2 parameters, with hourly time interval resolution for the diurnal variation, obtained with DPS-4 digisonde observations at Hainan (19.4°N, 109.0°E) are used to study the low latitude ionospheric variation behavior. The observational results are compared with the International Reference Ionospheric Model (IRI) predictions. The time period coverage of the data used for the present study is from March 2002 to February 2005. Our present study showed that: (1) In general, IRI predictions using CCIR and URSI coefficients follow well the diurnal and seasonal variation patterns of the experimental values of foF2. However, CCIR foF2 and URSI foF2 IRI predictions systematically underestimate the observed results during most time period of the day, with the percentage difference ΔfoF2 (%) values changing between about −5% and −25%, whereas for a few hours around pre-sunrise, the IRI predictions generally overestimate the observational ones with ΔfoF2 (%) sometimes reaching as large as ∼30%. The agreement between the IRI results and the observational ones is better for the year 2002 than for the other years. The best agreement between the IRI results and the observational ones is obtained in summer when using URSI coefficients, with the seasonal average values of ΔfoF2 (%) being within the limits of ±10%. (2) In general, the IRI predicted hmF2 values using CCIR M(3000)F2 option shows a poor agreement with the observational results. However, when using the measured M(3000)F2 as input, the diurnal variation pattern of hmF2 given by IRI2001 has a much better agreement with the observational one with the detailed fine structures including the pre-sunrise and post-sunset peaks reproduced reasonably well. The agreement between the IRI predicted hmF2 values using CCIR M(30,000)F2 option and the observational ones is worst for the afternoon to post-midnight hours for the high solar activity year 2002. During daytime hours the agreement between the hmF2 values obtained with CCIR M(30,000)F2 option and the observational ones is best for summer season. The discrepancy between the observational hmF2 and that obtained with CCIR M(30,000)F2 option stem from the CCIR M(3000)F2 model, which does not produce the small scale structures observed in the measured M(3000)F2. 相似文献
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介绍了一种基于V/F变换的高精度干式变压器数据采集与控制系统 ,采用LM2 3 1A/F变换芯片和89C5 2单片机实现工业现场测量对象的A/D转换。V/F变换器具有高精度 ,高线形度 ,且外围电路简单的特点。采用单片机直接与V/F变换器连接进行A/D转换 ,不需要额外的硬件电路 ,充分利用硬件资源 ,精心设计软件 ,系统分辨率可达 12位 ,转换精度可达 0 .0 2 %。当传感器与上位机距离较远时 ,可以采用RS -4 85接口或无线数据发送 /接收模块实现远距离的数据通信 相似文献
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王百亚%张康助%雷海锋%方东红 《宇航材料工艺》2003,33(4):39-42
研究讨论了缠绕过程中几种主要工艺参数对F— 12纤维 /RE14配方Φ15 0mm压力容器复合材料性能的影响。结果表明 :采用“交替”铺层方式缠绕成型 ,含胶量控制在 30 %~ 4 0 % (质量分数 ) ,缠绕张力控制在 15 0N~ 2 0 0N ,采用GPC谱图控制固化时机 ,得到的复合材料综合性能较好 ;用优化出的工艺参数进行了Φ4 80mm压力容器试验 ,结果表明其容器特性系数PV/W值为 37.0 2km ,纤维强度转化率高达73.2 6 %。 相似文献
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用扫描隧道显微镜(STM)对粘胶基碳纤维(RCF)表面的微观结构进行了研究,首次获得了原子级的RCF图像,对其原子间距作了精确地量化,并且尝试着将所得到的图像与高定向降解石墨(HOPG)相比较,以期对RCF的微观结构有更深入的了解,在原子级尺度上,发现了原子排列并不规则的石墨状结构,二维视图量化结果表明:相邻原子间距为0.142nm,最近六圆环中心的距离是0.253nm。 相似文献
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通过采用两片PIC18F448及其外围器件实现了机载环控地面检测系统的数字化设计。通过I^2C总线实现两片单片机之间的数据传输与协调,并利用其CAN接口模块实现多套检测系统的网络化和远程控制操作。 相似文献
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利用广州台站(23.2°N,113.3°E)的实测数据和IRI-2012模型提供的预测数据,对比分析了2013年广州地区f_0F2的变化特征.结果表明,IRI-2012模型能够较好预测该地区f_0F_2的变化趋势,并且CCIR参数得到的预测值比URSI参数更接近实测值;预测值与实测值存在系统偏差,在11:00 LT-06:00 LT时段,观测值均比预测值大,其他时段则相反.在日落后至午夜前时段,预测值与实测值有较大差距.绝对偏差的极值点通常出现在20:00 LT左右,最大超过4 MHz.相对偏差变化比较明显的时段是午夜后至凌晨;在02:00 LT或04:00 LT及06:00 LT附近,可能会出现双误差峰值点,最大超过0.4;但在σ变化很大的20:00 LT附近,相对偏差却变化不大.夜间增强现象会使得偏差增大,导致预测值不能很好反映实测f_0F2的变化. 相似文献
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对基于STM32系统低速(工作主频72MHz)视频流处理显示更新方案的研究。结合图像处理基本理论,分析传统的显示方法的不足,并提出一种新的视频流图像更新的方法,通过一定的实验数据和理论结果,验证该方法可行性。 相似文献
10.
Jia Luo Fangfang Sun Xiaohua Xu Han Wang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(1):327-336
In this paper, we compared the F2-Layer critical frequency (foF2) derived from FORMOSAT-3/COSMIC radio occultation (RO) and ionosondes at Chiang Mai, Chumphon and Kototabang during the years 2008–2015 to evaluate the performance of COSMIC RO over Southeast Asia region. The results show that the time development of foF2 values derived from COSMIC RO generally agrees well with those from ionosonde measurements. However, the differences between the foF2 derived from COSMIC RO and that derived from ionosonde observations display latitudinal dependence. COSMIC RO tends to underestimate foF2 at Chiang Mai and Kototabang, which is near to the north EIA crest and the south one, respectively, while a little overestimate foF2 at Chumphon, which is close to the geomagnetic equator. COSMIC RO agrees best with ionosonde at Chumphon and worst at Chiang Mai. At each ionosonde station, the quality of COSMIC RO data degrades with the increase of solar activity. In addition, at the station Chiang Mai and Kototabang, COSMIC RO performs better in summer than in equinox and winter. Furthermore, the differences in foF2 derived from COSMIC RO and that from ionosonde measurements vary with local time, i.e., the differences in foF2 are generally smaller at night and larger in noontime when equatorial ionization anomaly (EIA) is well developed. 相似文献