川西盆地雾和能见度的气候特征及其对飞行的影响   总被引：1，自引：0，他引：1  

李子良  傅刚  郝丽萍 《中国海洋大学学报(自然科学版)》2007,37(2):191-196

利用川西盆地广汉机场气象台1986年1月~1995年12月共10 a地面观测资料,对广汉机场低能见度的生消时间、持续时间和能见度的年季节变化及其日变化做了统计分析,研究广汉机场全年能见度的飞行气候特征,特别是低能见度气候特征对飞行的影响。结果表明,能见度日变化特征表现为:白天早、晚时段能见度较低,午后能见度达到最高。能见度的季节变化特征表现为:冬(12,1,2月)、春季(3,4,5月)能见度较低,而夏(6,7,8月)、秋季(9,10,11月)能见度较高。冬季能见度的变化主要受辐射雾影响,夏季能见度的变化主要受降水的影响,随着降水强度的变化而变化,低能见度时间短暂。各标准低能见度逐时频率的日变化特征在各季基本相似,低能见度高频率区均出现在早晨到上午,低频率区均出现在下午。  相似文献   

塔里木干旱区水稻田蒸发的实验研究     

王保栋 《干旱区地理》1992,15(4):54-59

根据中科院06—02—01研究计划任务,作者于1990年开始在阿克苏水平衡站进行观测实验,获得了宝贵的第一手资料,并应用EBBR法(能量平衡——包文比法)计算了稻田的蒸发量。通过分析评价表明,由于受“绿洲效应”的影响,结果明显偏大,不符合物理规律,因此该法在干旱区绿洲的应用尚需更多的探索,有待进一步完善。  相似文献   

改进的能量守恒方法及其在CHAMP重力场恢复中的应用(英文)   总被引：1，自引：0，他引：1  

XU Tianhe HE Kaifei Xi’an Research Institute of Surveying  Mapping  Middle Yanta Road  Xi’an  China. 《地球空间信息科学学报》2008,11(3):168-173

An efficient method for gravity field determination from CHAMP orbits and accelerometer data is referred to as the energy balance approach. A new CHAMP gravity field recovery strategy based on the improved energy balance approach IS developed in this paper. The method simultaneously solves the spherical harmonic coefficients, daily Integration constant, scale and bias parameters. Two 60 degree and order gravitational potential models, XISM-CHAMPO1S from the classical energy balance approach, and XISM-CHAMPO2S from the improved energy balance, are determined using about one year＇s worth of CHAMP kinematic orbits from TUM and accelerometer data from GFZ. Comparisons among XISM-CHAMPO1S, XISM-CHAMPO2S, EIGEN-CGO3C, EIGEN-CHAMPO3S, EIGEN2, ENIGNIS and EGM96 are made. The results show that the XISM-CHAMPO2S model is more accurate than EGM96, EIGENIS, EIGEN2 and XISM-CHAMPO1S at the same degree and order, and has almost the same accuracy as EIGEN-CHAMPO3S.  相似文献   

波流共存场中多向随机波浪传播变形数学模型   总被引：1，自引：0，他引：1       下载免费PDF全文

郑金海  Hajime Mase 《水科学进展》2008,19(1):78-83

基于波作用量守恒方程建立了波流共存场中多向随机波浪传播变形数学模型,模型中考虑了波浪绕射的影响和水流引起的波浪弥散多普勒效应,应用包含水流和地形影响的激破波模式计算波浪破碎的能量耗散,采用一阶上迎风有限差分格式离散控制方程。分别计算了有无近岸流情况下单向和多向随机波浪的波高分布,考虑水流影响的数值计算结果与物理模型实验数据吻合良好,比较分析表明,所建立的数学模型能够复演由于离岸流引起的波高增大,可用于波流共存场多向随机波浪传播变形的模拟和预报。  相似文献   

利用参考重力场模型基于能量法确定GRACE加速度计校准参数   总被引：1，自引：0，他引：1  

徐新禹  李建成  王正涛  邹贤才 《武汉大学学报(信息科学版)》2008,33(1):72-75

利用多个参考重力场模型分别对GRACE一个月的实测加速度计观测数据进行检校.数值计算结果的比较分析表明了利用参考重力场模型确定加速度计校准参数是有效的.  相似文献   

评价生物气生成量、生成期的元素平衡法及其应用   总被引：2，自引：0，他引：2  

卢双舫  刘绍军  申家年  薛海涛  徐庆霞  胡慧婷  王民 《地学前缘》2008,15(2):195-199

生物气的生成期对其成藏有至关重要的制约作用,但目前国内外尚缺少可信、有效方法来对此进行评价。针对这一难题,考虑到无论生物气的生成机理如何,都是一个有机元素之间的物质平衡过程,文章探索并建立了评价生物气生成量的元素平衡法,并利用松辽盆地大量的实际分析数据,对这一评价方法(模型)进行了标定和应用。结果表明,松辽盆地生物气的生成可能主要发生在800m以浅的埋深条件下;区内源岩生物气的生成量约为285.0×1012m3;生物气的主要生成期在嫩江组沉积末期之前。  相似文献   

Time-dependent stress change during failure of rocks     

V.T. Belikov  A.F. Shestakov 《Russian Geology and Geophysics》2008,49(5):350-356

The energy balance of a solid subject to fracture has been explored using heat and mass transfer equations with regard to the volumetric and superficial components. In the suggested model, brittle fracture of a cracked solid considered as a heterogeneous two-phase medium is described by an equation analogous to the Griffith’s criterion for propagation of a single crack. The derived equation is used, together with estimates of relative change in specific interface area, to study the respective change of free strain energy and pressure in rocks associated with failure.  相似文献   

Energy balance of simple elastodynamic sources     

Václav Vavryčuk 《Pure and Applied Geophysics》1994,143(4):563-586

Complete relations are derived for energy and energy flux of elastic waves generated by an isotropic and double-couple source in a perfectly elastic, homogeneous, isotropic, and unbounded medium. In the energy balance of elastodynamic sources near-field waves play an essential role, transforming static energy into wave energy, andvice versa. For explosive and dislocation sources, the sources surface radiates a positive wave energy that is partially distributed to the medium transforming into static energy. For implosive and antidislocation sources, the source surface generates elastic waves, but it does not necessarily imply that it also radiates a positive wave energy. The energy transported by waves can originate in gradual transformation of the static-to-wave energy during propagation of waves through a stressed medium.On leave from Geophysical Institute, Czech Academy of Sciences, Boní II/1401, 41 31, Praha 4 Czech Republic  相似文献   

Dynamics of Mars-orbiting dust: Effects of light pressure and planetary oblateness     

A. V. Krivov  L. L. Sokolov  V. V. Dikarev 《Celestial Mechanics and Dynamical Astronomy》1995,63(3-4):313-339

This paper deals with dynamics of impact ejecta from Phobos and Deimos initially on near-circular equatorial orbits around Mars. For particles emitted in a wide size regime of 1 micron and greater, and taking into account the typical particle lifetimes to be less than 100 years, the motion is governed by two perturbing forces: solar radiation pressure and influence of Mars' oblateness. The equations of motion of particles in Lagrangian non-singular elements are deduced and solved, both analytically and numerically, for different-sized ejecta. We state that the coupled effect of both forces above is essential so that on no account can the oblateness of Mars are be neglected. The dynamics of grains prove to be quite different for the ejecta of Phobos and Deimos. For Deimos, the qualitative results are relatively simple and imply oscillations of eccentricity and long-term variations of orbital inclination, with amplitudes and periods both depending on grain size. For Phobos, the dynamics are shown to be much more complicated, and we discuss it in detail. We have found an intriguous peculiar behavior of debris near 300 µm in size. Another finding is that almost all the Phobos ejecta with radii less than 30 µm (against the values of 5 to 20 µm adopted earlier by many authors) should be rapidly lost by collisions with martian surface. The results of the paper may be the base for constructing an improved model of dust belts that presumably exist around Mars.  相似文献   

A new treatment of the albedo radiation pressure in the case of a uniform albedo and of a spherical satellite     

Nicole Borderies  Pierre-yves Longaretti 《Celestial Mechanics and Dynamical Astronomy》1990,49(1):69-98

The purpose of this paper is to present a model for the radiation pressure acceleration of a spherical satellite, due to the radiation reflected by a planet with a uniform albedo. A particular choice of variables allows one to reduce the surface integrals over the lit portion of the planet visible to the satellite to one-dimensional integrals. Exact analytical expressions are found for the integrals corresponding to the case where the spacecraft does not "see" the terminator. The other integrals can be computed either numerically, or analytically in an approximate form. The results are compared with those of Lochry (1966). The model is applied to Magellan, a spacecraft orbiting Venus.  相似文献