台阶式变深水槽造波的解析研究

利用特征函数展开法对台阶式变深水槽中推板式造波机造波问题进行了研究,建立了相应速度势和波面的解析表达式。与高阶边界元方法(HOBEM)数值结果进行了对比,验证了本解析解的正确性。通过数值试验,研究了台阶对入射波的影响,同时分析了造波板所在位置(上部台阶)水深、水槽工作区(下部台阶)水深、造波板运动周期和造波板水平位置等因素对生成波浪高度的影响。由此选择合适的造波板所在位置及水深来得到所需要的波浪高度,进而根据需要生成波浪的周期和波幅来反演造波板的运动。     

锦州25—1南油气田主电站的选型设计

主电站作为海洋石油开采平台最重要的核心组成,为整个平台提供动力来源,是保证平台能够正常运转的心脏器官。从机组类型、特点,以及相应的工作原理等几个方面对海洋石油开采平台上的主电站作了简要的描述;依据相关基础数据,结合锦州25—1南油气田的特点,对油气田进行了电负荷分析,得出油气田设计所需要的典型电负荷量以及相关的数据;通过对机组容量、负荷率、备用率、机组占用平台面积、机组重量等几个参数的比对,从往复式发动机电站机组和燃气透平机电站机组中优选出了主电站机组方案。通过对锦州25—1南油气田主电站方案优选的详细阐述,为海洋石油开采平台主电站的选型设计提供参考和借鉴。     

基于FPGA的风廓线雷达信号定时器的设计和实现

详细介绍了信号定时器的特点和工作原理,并给出一种基于现场可编程门阵列(FPGA)的风廓线雷达信号定时器的设计方法.该信号定时器在某风廓线雷达中成功应用,且运行可靠,效果良好.     

恒湿盐湿度发生器的研制

具有连续循环系统和恒温系统的恒湿盐湿度发生器，首次在国内研制成功。该文介绍了恒湿盐湿度发生器的工作原理、误差分析、检定过程和标定结果。     

Microphysical Effects of Cloud Seeding in Supercooled Stratiform Clouds Observed from NOAA Satellite

Based on the satellite retrieval methodology, the spectral characteristics and cloud microphysical properties were analyzed that included brightness temperatures of Channels 4 and 5, and their brightness temperature difference (BTD), the particle effective radius of seeded cloud track caused by an operational cloud seeding and the microphysical effects of cloud seeding were revealed by the comparisons of their differences inside and outside the seeded track. The cloud track was actually a cloud channel reaching 1.5-km deep and 14-km wide lasting for more than 80 min. The effective radius of ambient clouds was 10-15μm, while that within the cloud track ranged from 15 to 26μm. The ambient clouds were composed of supercooled droplets, and the composition of the cloud within the seeding track was ice. With respect to the rather stable reflectance of two ambient sides around the track, the visible spectral reflectance in the cloud track varied at least 10%, and reached a maximum of 35%, the reflectance of 3.7μm in the seeded track relatively decreased at least 10%. As cloud seeding advanced, the width and depth were gradually increased. Simultaneously the cloud top temperature within the track became progressively warmer with respect to the ambient clouds, and the maximum temperature differences reached 4.2 and 3.9℃at the first seeding position for Channels 4 and 5. In addition, the BTD in the track also increased steadily to a maximum of 1.4℃, compared with 0.2-0.4℃of the ambient clouds. The evidence that the seeded cloud became thinner comes from the visible image showing a channel, the warming of the cloud tops, and the increase of BTD in the seeded track. The seeded cloud became thinner mainly because the cloud top descended and it lost water to precipitation throughout its depth. For this cloud seeding case, the glaciation became apparent at cloud tops about 22 min after seeding. The formation of a cloud track in the supercooled stratiform clouds was mainly because that the seeded cloud volume glaciated into ice hydrometeors that precipitated and so lowered cloud top height. A thin line of new water clouds formed in the middle of the seeded track between 38 and 63 min after seeding, probably as a result of rising motion induced by the released latent heat of freezing. These clouds disappeared in the earlier segments of the seeded track, which suggested that the maturation of the seeding track was associated with its narrowing and eventual dissipation due to expansion of the tops of the ambient clouds from the sides inward.     

The Effect of Relative Sunspot Numbers,Solar Flare Numbers and Variable Component of 10.7 cm Solar Flux on The Seasonal Variation of 6300 Å Line Intensity at Calcutta

The paper presents the seasonal variation of 6300 Å line intensity at Calcutta with relative sunspot number, solar flare number and variable component of 10.7 cm solar flux. A study has been made and important results have been obtained which are as follows. (i) Intensity of 6300 Å line shows periodic variation with relative sunspot number, solar flare number and variable component of 10.7 cm solar flux during the period 1984–1986 which is the secondary peak of the descending phase of 21st solar cycle. (ii) 6300 Å line intensity at Cachoeira Paulista station, taken by Sahai et al. (1988), also shows periodic variation with solar parameters during the period 1978–1980 which is the peak phase of the solar cycle. (iii) A possible explanation of such a type of variation is also presented.     

气候变化对我国小麦发育及产量可能影响的模拟研究

利用随机天气模型, 将气候模式对大气中CO₂倍增时预测的气候情景与CERES-小麦模式相连接, 研究了气候变化对我国冬小麦和春小麦生产的可能影响.结果表明, 气候变化后小麦发育将加快, 生育期缩短, 冬小麦平均缩短7.3天, 春小麦平均缩短10.5天, 春小麦生育期缩短的绝对数和相对数均大于冬小麦.籽粒产量呈下降趋势, 冬小麦平均减产7%~8%, 雨养条件下比水分适宜时减产幅度略大.春小麦的减产幅度大于冬小麦, 水分适宜时平均减产17.7%, 雨养时平均减产31.4%.     

地磁太阴日变化L的M2和O1潮

介绍Ｍ２和Ｏ１潮引起的地磁太阳日变化Ｌ谐波分析方法,计算了佘山地磁台的磁偏角,水平和垂直分量Ｌ的谐波系数,分析了Ｌ变化的基本特征,季节变化和场源性质,并与国外其它台站的结果进行对比分析。     

太阳耀斑爆发对京津冀地区云——地闪电活动的影响

太阳活动能否影响地球天气气候是一个全球关心的问题［１,２］．目前大多数研究者认为,太阳活动影响短期天气变化最可能的途径是通过调制大气电环境来实现的［３－５］,太阳耀斑爆发及其伴随事件均可对地球电环境产生明显的影响［１－５］,并通过磁层－电离层－中性大气层的耦合作用影响大气电场,再通过云中电性质的改变影响云的微物理结构［６,７］,并直接产生动力作用［８－１０］,从而影响雷雨云的发展,造成短期天气变化．２０多年来已有大量有关太阳耀斑与地球雷暴间的相关统计工作［３－５］．Ｍａｒｋｓｏｎ［１１］、Ｂｏｓ…