The Canadian Meteor Orbit Radar Meteor Stream Catalogue

The Canadian Meteor Orbit Radar is a multi-frequency backscatter radar which has been in routine operation since 1999, with an orbit measurement capability since 2002. In total, CMOR has measured over 2 million orbits of meteoroids with masses greater than 10 μg, while recording more than 18 million meteor echoes in total. We have applied a two stage comparative technique for identifying meteor streams in this dataset by making use of clustering in radiants and velocities without employing orbital element comparisons directly. From the large dataset of single station echoes, combined radiant activity maps have been constructed by binning and then stacking each years data per degree of solar longitude. Using the single-station mapping technique described in Jones and Jones (Mon Not R Astron Soc 367:1050–1056, 2006) we have identified probable streams from these single station observations. Additionally, using individual radiant and velocity data from the multi-station velocity determination routines, we have utilized a wavelet search algorithm in radiant and velocity space to construct a list of probable streams. These two lists were then compared and only streams detected by both techniques, on multiple frequencies and in multiple years were assigned stream status. From this analysis we have identified 45 annual minor and major streams with high reliability.     

Radar topography of domes on planetary surfaces

We investigate the possibility of measuring the heights and morphology of viscously emplaced domes using radar imagery. We accurately reproduce the known height and shape of a terrestrial salt dome, and estimate the heights of several venusian pancake domes to within a factor of two. The terrestrial salt dome is consistent with a Bingham flow, while the much larger venusian pancake domes are consistent with a Newtonian flow. Applying the same techniques to Ganesa Macula, a potential cryovolcanic dome on Titan, we estimate a height between 2.0-4.9 km. Additional factors such as variable roughness and composition might account for some of the discrepancies observed.     

基于分数阶Fourier变换的高性能SAR成像算法

传统距离多普勒算法（RD）较低精度的SAR成像质量越来越不能满足当前实际应用的需要。为解决传统距离多普勒算法成像性能低的问题,本文提出基于分数阶Fourier变换的高性能SAR成像算法（FrFT-RD）。本文详细推导SAR距离向信号运用分数阶Fourier变换时最佳阶数的计算表达式,同时给出方位向相应的计算式。理论分析表明距离（方位）向最佳阶数均取决于SAR成像参数并具有唯一性,无须迭代运算,可极大提高FrFT-RD算法的工程实用性。根据计算得到的距离向和方位向上最优阶数,在分数阶Fourier变换域完成FrFT-RD算法的构建。机载SAR模拟数据和星载SAR实测数据测试表明,FrFT-RD算法在分辨率、峰值旁瓣比（PSLR）成像性能方面比传统RD算法均得到显著提高,其中距离向和方位向分辨率提高比值分别为45.92%和48.06%;距离向PSLR和ISLR降低幅度为1.45 dB和2.59 dB,而FrFT-RD算法在方位向PSLR和ISLR成像性能方面与传统RD算法相当。     

雷暴单体合并进行中雷达回波参数演变及闪电活动的特征分析

雷暴单体合并是促使对流系统成长、增强、持久的重要因素,合并与灾害性天气有着密切的关系。针对23次合并样本（其中有闪电活动的样本10例）,利用多普勒雷达和Safir3000闪电定位系统的探测数据,基于雷达回波参数的构建与计算,分别以一次冰雹暴雨过程和一次强降水过程为例,对合并及雷暴系统的演变进行了物理过程分析,对所有样本特征进行了统计归纳。最后发现并验证了雷达回波参数F_V40up-6（即6 km以上对流单体大于40 dBz体积的变率）常常在合并进行中出现突然减小现象,简称为"突降";同时揭示了合并进行中闪电活动的特征。具体结论如下:（1）就合并最初开始位置而言,高度在5 km之下的样本最多,比例达86%。从合并用时看（即RHI图中30 dBz回波开始衔接至最强回波合为一体为止）,全都在6-36 min,其中用时在12 min以内的占56.5%;达到30 min的仅占16%。合并开始后,在97%的样本中,回波参数V₄₀（即大于40 dBz的总体积）、V_40up-6（即6 km以上大于40 dBz的总体积）出现增大;V₄₀增幅为7%-590%,V_40up-6增幅为3%-638%;V_40up-6最大值出现时刻距合并开始时刻12-18 min的,占总样本的60.1%;24-36 min的,占总样本的34.8%。（2）在雷暴单体合并进行中有"突降"现象的,占总样本的87%;其中又有77%的"突降"出现在距合并开始后的6-18 min内。（3）在10个闪电活动样本中,有9个样本在合并开始后,闪电频数出现了"跃增",甚至出现峰值;全部样本中参与放电的主正电荷区高度随着"突降"均有下降,降幅在1-4 km,而此时的闪电频数几乎没有变化。      

Where do planes fly past overhead? Determining departure and arrival routes from radar traces

This paper questions the main techniques of mapping in the context of aircraft noise in the vicinity of airports, and compares these techniques in terms of their purpose, benefits and limitations. Then the paper describes a method to summarise radar traces of a given air transport departure or arrival route into a median route and its envelope containing 80% of flights. This makes it possible to map global and easy-to-read maps of current air procedures around airports based on actual pathways flown by the aircraft. It also makes it possible to investigate the impact of change in aeronautical procedures on the actual geography of air routes around airports. Such maps complement noise contour maps and offer a good basis for debating aeronautical procedures at airports whose operations expose the population to noise.     

江西强雷电天气形势场及雷达回波特征分析

利用常规天气资料、地面观测资料、江西WebGIS雷达拼图和雷电监测资料,对2014—2016年江西出现的22次强雷电天气过程进行统计和对比分析。结果表明:江西强雷电天气易出现在赣北北部、南昌附近、上饶地区和吉安西部等区域;强雷电天气出现的环境背景场可分为副热带高压边缘型、副热带高压控制型、低涡切变型和台风外围型,最显著的特征是中高空经常伴有干冷舌侵入低层暖湿区;多项对流指数可以预测出现强雷电天气的可能性;雷达回波和雷电强度关系密切,回波类型以带状和块状为主;雷电强度和雷达回波强度有很好的对应关系,但产生强雷电的回波要具备强度大于50 dBz、强回波中心密实、强回波边缘梯度大等条件。     

定量测量降水量的回波结构自适应算法研究

为提高临近预报中对流性降水估测的准确性,分析了统计法估算降水的局限性。依据降水物理机制和降水回波结构,研究雷达反射率因子定量测量降水量(QPE-Qualitative Precipitation Estimate)的自适应算法,旨在减少由于雨滴谱变化导致的Z-I关系不稳定所引起的降水量测量误差。同时考虑组合反射率因子RC和垂直液态水含量VIL两个参量对降水的影响,建立适于城市区域的动态自适应的Z-I关系,改进对强降水严重低估的问题。     

RPGCA程序的改进

RPGCA程序负责将CINRAD/CD型雷达的archive基数据标准化命名后压缩上传,此数据是新一代天气雷达站的业务考核内容,同时也是雷达拼图、GR2等短临预报软件的必要数据。但实际使用下来发现RPGCA程序有传输时效性不高,系统资源占用较大等弊端。因此,本站使用C#开发了RPGCA改进版,此改进版不仅具有RPGCA程序的所有功能,并且改进了原版的弊端,同时增加了一些实用功能,提高了数据上传的时效性和稳定性。     

EnSRF雷达资料同化对一次强对流天气模拟的影响研究

利用ARPS(Advanced Regional Prediction System)模式和具有流依赖背景误差协方差的集合均方根滤波(Ensemble Square Root Filter,简称En SRF)方法,通过同化多部多普勒雷达资料,对2013年6月23日的强对流天气过程进行了研究。首先对比同化试验和观测的组合反射率因子,检验了同化效果。通过计算均方根误差和离散度,进一步定量评估了同化结果。再对比模式变量,综合分析了En SRF雷达资料同化对模式热力、动力、湿度和微物理量等变量的影响。最后对集合平均场进行1 km的高分辨率数值模拟。结果表明:En SRF能够同化出与观测类似的对流系统,且减弱了南北部的虚假回波。径向风和反射率因子的均方根误差明显减少。En SRF雷达同化能够明显优化模式的初始场,同化试验的回波在垂直方向上范围增加,强度偏弱。在强对流区域,低层的冷池温度最多降低6 K,相对湿度最多增加30%。对流区域的雨水、冰晶和雪的混合比均有明显增加。模拟发现同化试验能够较好地模拟出对流系统的结构和位置。     

Renewed uplift at the Yellowstone Caldera measured by leveling surveys and satellite radar interferometry

 A first-order leveling survey across the northeast part of the Yellowstone caldera in September 1998 showed that the central caldera floor near Le Hardy Rapids rose 24±5 mm relative to the caldera rim at Lake Butte since the previous survey in September 1995. Annual surveys along the same traverse from 1985 to 1995 tracked progressive subsidence near Le Hardy Rapids at an average rate of –19±1 mm/year. Earlier, less frequent surveys measured net uplift in the same area during 1923–1976 (14±1 mm/year) and 1976–1984 (22±1 mm/year). The resumption of uplift following a decade of subsidence was first detected by satellite synthetic aperture radar interferometry, which revealed approximately 15 mm of uplift in the vicinity of Le Hardy Rapids from July 1995 to June 1997. Radar interferograms show that the center of subsidence shifted from the Sour Creek resurgent dome in the northeast part of the caldera during August 1992 to June 1993 to the Mallard Lake resurgent dome in the southwest part during June 1993 to August 1995. Uplift began at the Sour Creek dome during August 1995 to September 1996 and spread to the Mallard Lake dome by June 1997. The rapidity of these changes and the spatial pattern of surface deformation suggest that ground movements are caused at least in part by accumulation and migration of fluids in two sill-like bodies at 5–10 km depth, near the interface between Yellowstone's magmatic and deep hydrothermal systems. Received: 30 November 1998 / Accepted: 16 April 1999