“SZ-4”飞船高度计天线指向角反演方法   总被引：1，自引：0，他引：1  

张有广  林明森 《海洋学报》2007,29(3):47-50

利用2003年2月7到8日“SZ-4”高度计的波形数据,经过波形数据预处理(波形为1 s的平均、去除热噪声和波形归一化)后,对海面回波波形后沿进行拟合,计算出了高度计天线的指向角,结果表明,“SZ-4”飞船高度计天线的指向角几乎全部在0.024°以内,天线指向在计算时间内比较稳定.  相似文献   

Arecibo radar observations of Phobos and Deimos     

Michael W. Busch  Steven J. Ostro  Jon D. Giorgini  Ellen S. Howell  Alice A. Hine  Irwin I. Shapiro 《Icarus》2007,186(2):581-584

In November 2005, we observed the moons of Mars using the Arecibo 2380-MHz (13-cm) radar, obtaining a result for the OC radar albedo of Phobos (0.056±0.014) consistent with its previously reported radar albedo and implying an upper bound on its near-surface bulk density of . We detected Deimos by radar for the first time, finding its OC radar albedo to be 0.021±0.006, implying an upper bound on its near-surface density of , consistent with a high-porosity regolith. We briefly discuss reasons for these low radar albedos, Deimos' being possibly the lowest of any Solar System body yet observed by radar.  相似文献   

Truncated dunes as evidence of the 2004 tsunami in North Sumatra and environmental recovery post‐tsunami     

Claire Kain  Christopher Gomez  Patrick Wassmer  Franck Lavigne  Deirdre Hart 《New Zealand geographer》2014,70(3):165-178

The 2004 tsunami transformed the coast of Indonesia. This research investigates a sand dune area in Lampuuk, Sumatra, that was scoured by tsunami flow. We assessed geomorphology one‐year post‐event and examine the timescale of vegetation recovery. Ground Penetrating Radar (GPR) evidence shows an eroded succession of thin dipping units, overlain by aeolian layers 0 to 50 cm thick. Incipient dunes were absent, indicating limited dune rebuilding at one‐year post‐tsunami, possibly resulting from channelised airflow and the absence of vegetation. Recolonisation by vegetation was initially limited but progressed rapidly between 2005 and 2011, highlighting the temporal non‐linearity of recovery processes.  相似文献   

基于不同海拔高度的雷达降水估测试验   总被引：3，自引：2，他引：1  

范江琳  青泉  马力 《气象科学》2014,34(1):66-71

在国内外雷达定量估测区域降水量一些方法基础上,将降水类型、地理位置和海拔高度同时纳入考虑范畴,在成都CINRAD/SC雷达站(海拔高度596.5 m)200 km范围内选择实验区,并按海拔高度将所选区域分为3区。然后利用2010年7—8月的雷达体扫资料以及同时段、同时次的雨量计数据,采用最优化算法分别在每个区域内修订传统Z-I关系中的"A,b"系数,以得到不同海拔地区的Z-I关系和每小时雨量估测值。研究表明,与直接采用传统的Z-I关系定量测量降水相比,各个区域内,经改善后的Z-I关系准确率提高了20%左右,算法相对简单,适合业务使用。  相似文献   

一次强雷暴中的多灾种天气特征对比分析     

王洪生  钟颖颖  吴海英  高晓静  刘燕 《气象科学》2014,34(4):465-471

用Micaps和NCEP再分析资料对2012年7月3日发生在淮河以南地区的大范围强雷暴天气进行了分析,得出高、低空急流配置,形成低空辐合,高空辐散,槽线由高到低前倾,有利增强大气不稳定层结,中尺度切变线南北摆动具有触发对流作用等,为该区强雷暴多灾种天气的发生,提供了动力和热力条件。从云图、雷达参数和地闪特征对比分析得出冰雹、雷击、强降水,分别发生在强对流云团发展的不同时间和不同部位。其云团的形态、强度和范围等也不同。冰雹所表现出的回波强度、回波顶高和垂直积分液态水含量为最强,雷击次之,强降水最弱。在地闪出现的各个阶段都有可能出现雷击事故,但多为负地闪,强度均较强。强降水过程多为负地闪,强度较弱,降水集中时段,地闪频次高。冰雹发生时地闪频数明显下降,且多为正闪。雷击过程强度和陡度变化最平缓,冰雹过程突变最明显。雷击发生在整个地闪过程中强度和陡度都相对较大的时刻;冰雹发生前约半小时有强度和陡度的骤增;强降水阶段地闪平均强度和陡度都最小。  相似文献   

Sporadic meteor sources as observed by the Jicamarca high-power large-aperture VHF radar     

Jorge L. Chau  Ronald F. Woodman  Freddy Galindo 《Icarus》2007,188(1):162-174

We present, for the first time, the main sources of sporadic meteors as inferred from meteor-head echoes obtained by a high-power large-aperture radar (HPLAR). Such results have been obtained at the Jicamarca HPLAR (11.95° S, 76.87° W, 1° dip angle). Observations are based on close to 170,000 meteors detected in less than 90 h spread over 14 days, between November 2001 and February 2006. Meteors with solar orbits are observed to come from basically six previously known sources, i.e., North and South Apex, Helion, Anti-Helion, and North and South Toroidal, representing ∼91% of the observations. The other ∼9% represents meteors with observed velocities greater than the Sun's escape velocity at 1 AU, most of them of extra-solar origin. Results are given before and after removing the Earth's velocity and the sources are modeled with two-dimensional Gaussian distributions. In general, our results are in very good agreement with previously known sources reported by Jones and Brown [Jones, J., Brown, P.G., 1993. Mon. Not. R. Astron. Soc. 265, 524-532] using mainly specular meteor radar (SMR) data gathered over many years and different sites. However, we find slightly different locations and widths, that could be explained on the basis of different sensitivities of the two techniques and/or corrections needed to our results. For example, we find that the North and South Apex sources are well defined and composed each of them of two collocated Gaussian distributions, one almost isotropic with ∼10° width and the other very narrow in ecliptic longitude and wide in ecliptic latitude. This is the first time these narrow-width sources are reported. A careful quantitative analysis is needed to be able to compare the strengths of meteor sources as observed with different techniques. We also present speed and initial altitude distributions for selected sources. Using a simple angular sensitivity function of the combined Earth-atmosphere-radar instrument, and an altitude selection criteria, the resulting meteor sources are in better qualitative agreement with the results obtained with SMRs.  相似文献   

流星雷达测距精度的改进     

Yang Kejun  Wang Yahong 《时间频率学报》1995,(1)

针对目前流星雷达测距误差大的问题，本文提出了提高流星雷达测距精度的新方法，即提高采样速率，用相关分析确定回波脉冲参考点的方法。该方法使流星雷达的测距精度提高一个数量级，测距误差降到±１４ｍ，使流星雷达不仅可以用来观测研究流星，还可用于监测飞机、火箭的飞行等，扩大流星雷达的应用。  相似文献   

用雷达回波资料识别雹云的最新进展     

李祚泳  刘少侬  邓新民  张辉军 《成都信息工程学院学报》1993,(1)

本文评述了当前国内外利用雷达回波资料识别雹云的现状,着重介绍了笔者近年来利用雷达回波资料建立雹云识别模式的研究工作,并展望了雹云识别的未来发展前景。  相似文献   

A technique for calculating meteor plasma density and meteoroid mass from radar head echo scattering     

S. Close  M. Oppenheim  A. Coster 《Icarus》2004,168(1):43-52

Large-aperture radars detect the high-density plasma that forms in the vicinity of a meteoroid and moves approximately at its velocity; reflections from these plasmas are called head echoes. To determine the head plasma density and configuration, we model the interaction of a radar wave with the plasma without using assumptions about plasma density. This paper presents a scattering method that enables us to convert measurements of radar cross-section (RCS) from a head echo into plasma density by applying a spherical scattering model. We use three methods to validate our model. First, we compare the maximum plasma densities determined from the spherical solution using 30 head echoes detected simultaneously at VHF and UHF. Second, we use a head echo detected simultaneously at VHF, UHF and L-band to compare plasma densities at all frequencies. Finally, we apply our spherical solution to 723 VHF head echoes and calculate plasma density, line density and meteoroid mass in order to compare these values with those obtained from a meteoroid ablation and ionization model. In all three comparisons, our results show that the spherical solution produces consistent results across a wide frequency range and agrees well with the single-body ablation model.  相似文献   

高度计测距精度对沿轨迹重力异常反演的影响     

李洋  张润宁 《测绘学报》2015,44(4):363-369

应用求解沿轨迹重力异常的垂线偏差法以及求解空间分辨率的交叉谱分析法,建立了高度计测距精度与沿轨迹重力异常反演精度以及空间分辨率的关联性模型。首先依据卫星测高原理,给出了沿轨迹重力异常的误差传播公式,然后以此为基础通过推导交叉谱分析中一致性系数与信噪比的数学表达式,建立了高度计测距精度与空间分辨率的解析关系。数值仿真结果表明:雷达高度计测距精度与沿轨迹重力异常反演精度成正比关系,与空间分辨率成幂函数关系,即高度计测距精度提高m倍,沿轨迹重力异常反演精度提高m倍,全球海域平均空间分辨率提高m0.464 4倍。将数值仿真结果与相关文献中对实际测高数据的处理结果进行比较,验证了理论分析及模型的正确性。  相似文献