丘陵地区边界层风廓线雷达数据统计特性分析   总被引：3，自引：2，他引：1  

汪学渊  汪波  文明章  吴昌叨  张磊 《气象科学》2015,35(3):328-333

采用数据获取率来分析和评价风廓线雷达的探测能力, 对通过2012年的风廓线数据进行统计分析。结果表明:数据获取率和信噪比都随季节变化, 夏季探测能力大于冬季。按照数据获取率达到80%的要求, 确定边界层风廓线雷达无降雨天气有效探测高度为3 km, 并确定低模和高模最佳衔接高度为0.6 km, 能够获得更好的数据获取率。在无降雨天气, 信噪比随高度呈现对数函数单调递减的变化规律, 夏季信噪比的衰减程度比冬季大;在降雨天气, 信噪比随高度呈现一次函数的变化规律, 其斜率范围在-10.44~-2.47之间, 而夏季信噪比的衰减程度比冬季小。  相似文献   

虚拟天文台数据访问系统(VO-DAS)任务调度设计与实现     

田海俊  刘超  高丹  路勇  杨阳  崔辰州  赵永恒  郑小平 《天文研究与技术》2011,8(1)

为解决异地、异构、海量天文数据无缝透明地统一访问,中国虚拟天文台(China-VO)研究小组自主设计并开发了一套解决方案——虚拟天文台数据访问系统(VO-DAS)。着重从执行流程、设计模式、Session机制、生命周期、资源销毁、异常处理等模块详细阐述了该系统的任务调度设计。为了验证该系统的可行性和性能,最后描述了多个天文科学范例。  相似文献   

Pencil-beam surveys for trans-neptunian objects: Limits on distant populations     

Alex H. Parker  J.J. Kavelaars 《Icarus》2010,209(2):766-770

Two populations of minor bodies in the outer Solar System remain particularly elusive: Scattered Disk Objects and Sedna-like objects. These populations are important dynamical tracers, and understanding the details of their spatial- and size-distributions will enhance our understanding of the formation and on-going evolution of the Solar System. By using newly-derived limits on the maximum heliocentric distances that recent pencil-beam surveys for trans-neptunian objects were sensitive to, we determine new upper limits on the total numbers of distant SDOs and Sedna-like objects. While generally consistent with populations estimated from wide-area surveys, we show that for magnitude-distribution slopes of α ? 0.7-1.0, these pencil-beam surveys provide stronger upper limits than current estimates in literature.  相似文献   

Retrieval algorithm for atmospheric dust properties from Mars Global Surveyor Thermal Emission Spectrometer data during global dust storm 2001A     

Attila Elteto  Owen B. Toon 《Icarus》2010,210(2):566-588

We present a new parameter retrieval algorithm for Mars Global Surveyor Thermal Emission Spectrometer data. The algorithm uses Newtonian first-order sensitivity functions of the infrared spectrum in response to variations in physical parameters to fit a model spectrum to the data at 499, 1099, and 1301 cm⁻¹. The algorithm iteratively fits the model spectrum to data to simultaneously retrieve dust extinction optical depth, effective radius, and surface temperature. There are several sources of uncertainty in the results. The assumed dust vertical distribution can introduce errors in retrieved optical depth of a few tens of percent. The assumed dust optical constants can introduce errors in both optical depth and effective radius, although the systematic nature of these errors will not affect retrieval of trends in these parameters. The algorithm does not include the spectral signature of water ice, and hence data needs to be filtered against this parameter before the algorithm is applied. The algorithm also needs sufficient dust spectral signature, and hence surface-to-atmosphere temperature contrast, to successfully retrieve the parameters. After the application of data filters the algorithm is both relatively accurate and very fast, successfully retrieving parameters, as well as meaningful parameter variability and trends from tens of thousands of individual spectra on a global scale (Elteto, A., Toon, O.B. [2010]. Icarus, this issue). Our results for optical depth compare well with TES archive values when corrected by the single scattering albedo. Our results are on average 1–4 K higher in surface temperatures from the TES archive values, with greater differences at higher optical depths. Our retrieval of dust effective radii compare well with the retrievals of Wolff and Clancy (Wolff, M.J., Clancy, R.T. [2003]. J. Geophys. Res. 108 (E9), 5097) for the corresponding data selections from the same orbits.  相似文献   

Analysis of Jupiter’s Oval BA: A streamlined approach     

Michael G. Sussman  Nancy J. Chanover  Ashwin R. Vasavada 《Icarus》2010,210(1):202-210

We present a novel method of constructing streamlines to derive wind speeds within jovian vortices and demonstrate its application to Oval BA for 2001 pre-reddened Cassini flyby data, 2007 post-reddened New Horizons flyby data, and 1998 Galileo data of precursor Oval DE. Our method, while automated, attempts to combine the advantages of both automated and manual cloud tracking methods. The southern maximum wind speed of Oval BA does not show significant changes between these data sets to within our measurement uncertainty. The northern maximum does appear to have increased in strength during this time interval, which likely correlates with the oval’s return to a symmetric shape. We demonstrate how the use of closed streamlines can provide measurements of vorticity averaged over the encircled area with no a priori assumptions concerning oval shape. We find increased averaged interior vorticity between pre- and post-reddened Oval BA, with the precursor Oval DE occupying a middle value of vorticity between these two.  相似文献   

Determination of asteroid masses from their close encounters with Mars     

L. Somenzi  A. Fienga  J. Laskar 《Planetary and Space Science》2010,58(5):858-863

An obstacle to the asteroid mass determination lies in the difficulty in isolating the gravitational perturbation exerted by a single asteroid on the planets, being strongly correlated and mixed up with those of many other asteroids. This hindrance may be avoided by the method of analysis presented here: an asteroid mass is estimated in correspondence with its close encounters with Mars where the acceleration it induces on the planet can be sufficiently disentangled from those generated by the remaining asteroid masses to calculate. We test this technique in the analysis of range observations to Mars Global Surveyor and Mars Express performed from 1999 to 2007. For this purpose, we adopt the dynamical model of the planetary ephemeris INPOP06 (Fienga et al., 2008), which includes the gravitational influences of the 300 most perturbing asteroids of the Martian orbit. We obtain the solutions of 10 asteroid masses that have the largest effects on this orbit over the period examined: they are generally in good agreement with determinations recently published.  相似文献   

基于GIS的地震安全性评价数据管理的研究     

田勤虎  李晓聪  魏电信 《陕西地质》2010,28(2):111-115

目前的地震安全性评价数据管理方法过于陈旧,不利于数据的查询和再利用。通过对这一问题的深入分析,针对安评数据的多元性特点,结合GIS的优势,提出了利用GIS技术对地震安全性评价数据进行管理的方法,并设计出了数据库管理系统的基本框架。该系统的建立,将为地震安全性评价数据管理、查询和再利用提供便利。  相似文献   

保山西邑铅锌矿采选工程RQD与RBI对比研究   总被引：2，自引：0，他引：2  

王建国  刘德安  徐世光  张世涛  李洪伟 《云南地质》2010,29(2):220-223,214

用岩石质量指标和岩体块度指数的理论,对钻孔岩心实测资料进行分析和对比研究,对钻孔周围岩体进行分级。结果表明:岩体块度指数在岩石质量评价中能更准确地反映其优越性,具有更为显著的工程意义。  相似文献   

云南惠民铁矿遥感近矿找矿标志及成矿预测     

赵志芳  郭富达 《云南地质》2010,29(4):434-437

分析总结惠民铁矿区赋矿地层惠民组火山岩、弧形构造内缘北西向构造交汇部位、铁染羟基异常等成矿、控矿条件的遥感影纹、色调等标志,根据矿化遥感异常信息圈定3处找矿远景地段。  相似文献   

多金属成矿区深地震反射剖面数据处理技术实验研究——以庐枞矿集区为例   总被引：2，自引：1，他引：1  

刘金凯  匡朝阳  高锐  薛爱民  卢占武  侯贺晟  王海燕 《岩石学报》2010,26(9):2561-2576

针对庐枞多金属矿集区地震资料特点及浅、深多重探测目标,对深地震反射数据进行了处理技术实验研究。在区域长剖面上,为了获得矿集区地壳与上地幔结构的精细图像,解释成矿深部过程,开展了循序渐进的常规处理技术实验和精细处理技术实验。在矿区剖面,为了获得了浅层精细结构,针对变观测系统接收等特点,进一步开展了特殊处理实验。经过区域剖面与矿区剖面的多重处理实验,集成了一套矿集区深地震反射剖面数据处理方法与处理技术流程,为我国进一步的深部探测积累了技术与经验。  相似文献