高空探测资料气球空间经纬度偏差算法     

李宛桐  刘磊  张伟星  张玉存  高太长 《气象科技》2015,43(3):405-409

随着数值预报的发展,模式的分辨率逐渐提高,探空气球在施放过程中受高空气流影响造成的漂移已大大超出了数值预报模式分辨率,其影响不能忽视。鉴于现有气球空间位置经纬度偏差计算方法基于站心坐标系,忽略地球曲率影响,文章从探测系统原理出发,推导出精确的基于地心坐标系的气球空间位置经纬度偏差计算公式,并通过探空数据文件对原有算法进行误差分析。  相似文献   

像平面坐标到经纬度坐标的转换   总被引：2，自引：2，他引：0  

张金金  梁洪有  陈兴峰  顾行发  余涛  葛慧斌 《地理空间信息》2010,8(1):63-66

坐标转换是所有的遥感、GIS、航测等软件都必须具备的一个基本功能,在功能实现中会遇到大规模的矩阵运算问题,而灵活运用IDL编程工具中的结构数组运算能大大地简化计算步骤,加快图像处理的速度。本文运用IDL设计了坐标转行算法,对于一幅row(行)、col(列)的图像,在已知该幅图像其中一个像元点在图像中的像元位置和经纬度坐标的情况下,利用该算法能够实现整幅图像中所有点的经纬度坐标的计算,并验证了其正确性。  相似文献   

Regional and temporal changes in bivalve diversity off the south coast of Portugal     

M.M. Rufino  M.B. Gaspar  F. Maynou  C.C. Monteiro 《Estuarine, Coastal and Shelf Science》2008,80(4):517-528

From 2000 to 2006, a total of 75 bivalve species were identified, varying from 29 (spring 2001) to 54 species (spring 2005) per year. Seasonal tendencies in diversity varied according the year, thus the interpretation of long-term and regional scales is essential before drawing any conclusions in other studies. Richness and diversity consistently decreased with depth and increased with sediment grain size (from low in very coarse sand to high in coarse silt). Diversity decreased progressively from 3 to 16 m depth, thus the harsher shallower environments (due to waves and tidal air exposure) showed greater diversity than the most stable areas. Communities in finer sediments were more diverse than those in coarser sand. Evenness showed patterns opposite to diversity, overall.Diversity and evenness maps (produced with multivariate universal kriging), showed that most geographic areas with greater diversity were farer from river outflows and wastewater treatment plants. Two types of geographic pattern were observed: areas with persistently greater bivalve diversity through time and areas that changed locally from year to year. This spatial analysis can be used to establish priority conservation areas for management purposes, and to analyse the persistency of regional diversity patterns. The area with most habitat heterogeneity (Sotavento) corresponded to greatest diversity.There was a positive relationship between Spisula solida and Chamelea gallina landings and bivalve diversity 2 years and 1 year later, respectively. Possibly, local fisheries, by selectively withdrawing the commercial numerically dominant species from the ecosystem, increased diversity 1 to 2 years later, as the ecological niches of the dominants are quickly filled by several other species thereby creating a more even community. On regional scales, no significant impact was found on long-term bivalve diversity in local fisheries,  相似文献   

基于闪电定位数据的地闪密度修订     

彭国平 《气象科技》2017,45(5):876-881

利用湖北省闪电定位系统(Lightning Location System,LLS)资料,用网格地闪密度数据表征地闪的空间分布,测站距离因子表征探测站布局,对2015年地闪空间分布特征进行分析,结果表明,其密度与因子之间存在负相关,其中雷电流幅值5~30kA的密度分量与因子之间存在显著性相关,大于30kA的密度分量与因子相关不显著。同时发现探测站布局对地闪空间分布的疏密程度有一定的影响,因此有必要对密度进行修订,以消除测站布局的影响。运用线性回归方法及其残差理论,建立了网格地闪密度的修订模型和相对探测效率的统计模型。验证了密度分段修订和不分段修订结果的一致性。通过对理论探测效率和相对探测效率的对比分析,论证了地闪密度修订方法和相对探测效率统计方法的可行性。  相似文献   

Report of the International Astronomical Union Division I Working Group on Precession and the Ecliptic   总被引：1，自引：0，他引：1  

J. L. Hilton  N. Capitaine  J. Chapront  J. M. Ferrandiz  A. Fienga  T. Fukushima  J. Getino  P. Mathews  J.-L. Simon  M. Soffel  J. Vondrak  P. Wallace  J. Williams 《Celestial Mechanics and Dynamical Astronomy》2006,94(3):351-367

The IAU Working Group on Precession and the Equinox looked at several solutions for replacing the precession part of the IAU 2000A precession–nutation model, which is not consistent with dynamical theory. These comparisons show that the (Capitaine et al., Astron. Astrophys., 412, 2003a) precession theory, P03, is both consistent with dynamical theory and the solution most compatible with the IAU 2000A nutation model. Thus, the working group recommends the adoption of the P03 precession theory for use with the IAU 2000A nutation. The two greatest sources of uncertainty in the precession theory are the rate of change of the Earth’s dynamical flattening, ΔJ₂, and the precession rates (i.e. the constants of integration used in deriving the precession). The combined uncertainties limit the accuracy in the precession theory to approximately 2 mas cent⁻². Given that there are difficulties with the traditional angles used to parameterize the precession, z_A, ζ_A, and θ_A, the working group has decided that the choice of parameters should be left to the user. We provide a consistent set of parameters that may be used with either the traditional rotation matrix, or those rotation matrices described in (Capitaine et al., Astron. Astrophys., 412, 2003a) and (Fukushima Astron. J., 126, 2003). We recommend that the ecliptic pole be explicitly defined by the mean orbital angular momentum vector of the Earth–Moon barycenter in the Barycentric Celestial Reference System (BCRS), and explicitly state that this definition is being used to avoid confusion with previous definitions of the ecliptic. Finally, we recommend that the terms precession of the equator and precession of the ecliptic replace the terms lunisolar precession and planetary precession, respectively.  相似文献   

SOFTWARE REVIEWS     

《The Professional geographer》1988,40(1):106-116

software reviews are in this article BMDP/PC CONCEPTS COMPUTERIZED ATLAS EVALUATION OF ALTERNATE PROPOSALS (EAP) EXTRA: EXPRESS TRANSIT ANALYSIS MATC CAD MOTORS TRANSPORTATION PACKAGE PCMAP: Thematic Mapping Software for the IBM Personal Computer, Version 2.3 PLACE TRANPLAN . US-ATLAS  相似文献   

Distribution of ionospheric O<Superscript>+</Superscript> ion in synchronous altitude region     

Jiankui?Shi?Email author  Zhenxing?Liu  Zhang?T.?L.  Jianshan?Guo  Manlian?Zhang  Sheping?Shang  Xigui?Luo 《中国科学D辑(英文版)》2003,46(10):986-993

Based on satellite observation data, using dynamics equation, the ionospheric O⁺ ion’s distribution in the synchronous altitude region for different geomagnetic activity indexK _p is studied by theoretical modeling and numerical analyzing, and semi-empirical models for the O⁺ ion’s density and flux versus longitude in the synchronous altitude region for differentK _p are given. The main results show that in the synchronous altitude region: (i) The O⁺ ion’s density and flux in day-side are larger than those in nightside. (ii) With longitude changing, the higher the geomagnetic activity indexK _p is, the higher the O⁺ ion’s density and flux, and their variation amplitude will be. The O⁺ ion’s density and flux whenK _{p ≥} 6 will be about ten times as great as that whenK _p = 0. (iii) WhenK _p = 0 orK _{p ≥} 6, the O⁺ ion’s density reaches maximum at longitudes 120° and 240° respectively, and minimum in the magnetotail. WhenK _p = 3−5, the O⁺ ion’s density gets to maximum at longitude 0°, and minimum in the magnetotail. However, the O⁺ ion’s flux reaches maximum at longitude 120° and 240° respectively, and minimum in the magnetotail for anyK _p value.  相似文献   

利用WIN—SURFER软件绘制物化探图件   总被引：10，自引：4，他引：6  

田黔宁 《物探化探计算技术》1998,20(4):366-369

本文主要介绍了如何在ＷＩＮ－ＳＵＲＦＥＲ环境下实现物化探图件中的经纬网绘制、标准图框绘制、曲线类型图绘制方法。  相似文献   

公转轴应力场星球说——地球、火星南南西应力场四组三维构造系     

孙兆元  孙娟 《地球科学进展》1999,14(3):218-228

介绍了对地球构造格局,运动方式及其动力源问题研究取得的新成果。它不同于流行已久的以地球自转轴旋转和以软流圈带动岩石圈漂移以及随机的地幔柱（流）为构造动力源的观点,而是与黄赤交角相关的沿公转轴方向的统一应力场,认为中国西部ＮＷＷ向压性,ＮＥＥ与ＮＮＷ是与黄赤交角相关的沿公转轴方向的统一应力场。认为中国西部ＮＷＷ向压性,ＮＥＥ与ＮＮＷ向两组共轭扭性及ＮＮＥ向张性带交接,为来自全球ＳＳＷ主压应力场形成的  相似文献   

中国大陆地区热流数据的分布及其初步分析          下载免费PDF全文

黄少鹏 《地震地质》1989,11(3):17

本文首次系统地收集整理了观测资料比较齐全、国内公开发表的热流数据167个,并对之进行了初步分析。这些数据的地理分布还很不均匀,热流值变化范围为25—245mWm-2,多种平均方法得到的结果表明,中国大陆区域代表性热流值范围为61—68mWm-2。作者所作的经纬度网格和条带统计还揭示,数据覆盖区内热流沿经、纬向的分布有明显的差异,纬向条带平均热流值看来具有波状起伏变化的规律。这一结果已经得到日本及其周围海域热流数据的初步印证,如果获得更广泛的证实,无疑具有深刻的地质和地球物理意义  相似文献