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在大气臭氧垂直分布的研究中,逆轉方法B在最近几年有着比較广泛的应用。不久前我們曾証明,方法B的解是不唯一的,李鈞等同志对我們的工作提了一些意見,我們觉得这很好。 相似文献
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本文结合CR-InSAR、PS-InSAR技术,将CR、PS点联合构网,采用LAMBDA方法进行相位解缠,研究西秦岭北缘断裂带中断的微小形变,结果得出断裂带表现出左旋走滑运动特征,断裂带南盘平均形变速率为2.3mm·a~(-1),北盘平均形变速率为-1.5mm·a~(-1),南北两盘平均形变速率差异为3.8mm·a~(-1),与其他学者GPS、地质测年研究成果相近.对研究区内的角反射器(CR点)安装、影像特征分析及形变解算进行了较为详细的论述,并对比分析了CR、PS点联合构网和PS点单独构网解算结果,得出对地质环境复杂的断裂带做永久散射体形变研究时,CR、PS点联合构网解算结果好、研究结果可靠.说明CR、PS点联合构网中,CR点由于其自身的高稳定特性,对整个解算网络起到了很好的整体控制作用,保证了解算结果正确. 相似文献
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研究了基于纤维模型的CFT框架柱滞回性能模拟的建模方法,建立了基于不同材料本构模型的CFT框架柱数值模型,并探讨了材料本构关系、纤维截面网格划分、积分点数量等因素对模拟精度的影响。以试验为依据,运用Opensees软件,通过计算结果与试验结果的对比,分析了影响滞回模型计算精度的主要因素。结果表明,受约束混凝土本构关系的下降段,钢材本构关系的强化段,是影响滞回模型准确性的主要因素,而网格划分和积分点数量的影响则主要体现在程序运行速率方面。研究将为基于纤维模型法的CFT框架柱滞回性能模拟分析提供理论依据。 相似文献
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本文詳細地介紹了武汉采用的交点相关法和十点相关法的理論基础和具体計算方法,并与Philtips和spcncer的相关法（PS法）及Yerg的六点相关法进行了比較。正如理論上所預期到的,武汉的实驗表明:交点法提供的参量最多,也最精确可靠,但計算量与PS法的差不多;十点法提供的参量与交点法的一样多,精确性不此PS法的低,然而計算量比PS法的少得多,与六点法的差不多。文中还討論了利用时移图上曲直线,以进一步提高十点法的精确性,以及在相关分析中采用結构函数和后效函数,以进一步簡化計算的可能性。本文还初步討論了各种相关分析法的誤差間題;并提出了相关函数值在时空上的預报方法,以及根据相关函数的預报值与实測值的对此等,判别在記录分析中有无反常現象,和甄別所求出的参量值是否可疑的方法。最后还特別指出了电离层混乱运动变化速度出現虛数值的可能性,并介紹了消除这种虛数值的方法。 相似文献
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本文利用相对論带电粒子的两个寝渐不变量,討論了磁暴主相期間外輻射带中心結构的变化。作者认为磁暴主相是由“磁暴带”环电流所产生。“磁暴带”假設位于外輻射带中心之外,它是太阳等离子体穿入磁层后形成的。本文对初始能量W=20Kev和W=1Mev的电子分別进行了計算。 結果表明,在磁暴主相期間电子向外漂移,其赤道投擲角減小,但镜点离地面距离增高。因此,主相时所观測到的极光,并不是由于地磁場的平緩下降使小投擲角电子注入大气层而形成的。此外,計数率降低的主要原因是由于力管截面膨胀造成的粒子密度減小以及电子減速,而电子減速与投擲角有关,由此决定了电子通量沿磁力线分布的变化。以上結果与探险者6号（Explorer Ⅵ）的观測一致。 相似文献
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在线数值模拟方法是一种基于模型更新的混合试验方法,其是不完整边界条件混合试验的通用解决方案。在该方法中：结构反应由结构整体数值模型计算得到,边界条件自然得以满足;物理子结构的恢复力不再参与运动方程的求解,而是用于估计数值模型的本构参数,提高了数值模型的可靠性。论文提出多本构模型参数同步更新的在线数值模拟方法,以提高多种本构模型参数不确定性同时存在时在线数值模拟方法的精度,并以Levenberg-Marquardt算法为参数估计方法,实现了采用恢复力对钢筋和混凝土材料本构模型参数的同步估计。研究表明：以恢复力来估计材料本构模型参数是可行的,且Levenberg-Marquardt算法具有较高的收敛速度和计算精度;在线数值模拟方法有效地提高了混合试验的模拟精度。 相似文献
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不排水抗剪强度与初始超固结比OCR的关系可以由三轴压缩状态下的不排水抗剪强度公式表示。首先根据该公式由强度试验数据计算土体各点OCR与其深度的关系式;然后将该关系式引入到UH模型有限元程序中;最后应用UH模型的有限元程序分别对考虑OCR随深度变化和OCR为1的不排水地基进行了数值分析,并对两种情况下的载荷-沉降曲线、随时间变化的地基表面沉降、随时间变化的结点剪应变、体应变和孔压曲线作了比较。分析可知:采用OCR随深度变化的UH模型的有限元程序能够合理考虑地基土体实际的超固结比,在非均质不排水地基的有限元分析中是有必要的。 相似文献
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本文探討了Gotz逆轉效应中,单色天頂散射光强I3112（?）的有效散射高度hE的上升过程。首先从理論上証明:hE并非沿高度連續的上升,而是跳跃上升的。然后用实际观測数据的計算,証实了理論結果。由此并指出,由于hE的跳跃,那么在应用逆轉效应,建立測定大气臭氧垂直分布方法时,如果将大气分层較多,那么可能在臭氧层中下部所得的結果,是不唯一的。基于上述結果,进一步研究了方法B,发現目前国际上通用的,由Ramanathan与Davo所給出的逆轉方法B的解是不唯的。这些解之間有着亘大的差异。因此以該方法計算出的各层臭氧含量,并不能肯定大气臭氧的垂直分布情况。 相似文献
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Summary The accuracy of the electrochemical ozone sonde, type OSR, has been estimated by analysing tandem ozone soundings of the balloon-borne electrochemical ozone sonde OSR at the Lindenberg Observatory from May to November 1982. A negative bias, though not significant, has been observed above about 28 km for soundings having high single correction factors. Random errors are at their minimum just above the level of the maximum of ozone partial pressure, and reach their maximum in the troposphere. Except at heights above about 28 km the random error of ozone sondes is a factor 2 to 3 times less than the error of the short Umkehr method. Provided that soundings with too high correction factors are neglected, the ozone sonde OSR has an accuracy comparable to that of other Brewer type sondes.The maximum amount of information on the vertical ozone distribution can be drawn from sonde measurements in the lower stratosphere. A study is underway to improve the sensitivity of the sonde OSR and thus to further enhance its reliability. 相似文献
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H. U. Dütsch 《Pure and Applied Geophysics》1978,116(2-3):511-529
All available data of the vertical ozone distribution measured with chemical sondes have been assembled and combined with one year's results from the BUV satellite to obtain the best possible information on the vertical ozone distribution averaged over longitude as a function of season (month by month). For the southern hemisphere Umkehr data have been used as a guideline in the necessary smoothing procedure. Especially in the northern hemisphere considerable adaptation to the observed latitudinal mean of the total amount was needed because most sounding stations, are situated in upper air trough positions.The results are presented as vertical distributions, as meridional cross sections of partial pressure and of mixing ratio and as partial pressure isolines as a function of latitude and season at different levels. The interaction between photochemical processes and transport resonsible for the observed distribution is briefly discussed. 相似文献
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The observed relationship between atmospheric vorticity variations and solar magnetic sector boundary passages is examined for a possible connection via ionization changes affecting ozone distributions. A superposed epoch analysis was performed on Umkehr distributions for 18 years from Arosa, Switzerland, with use of more than 500 solar sector boundary passages as keyday zero. No significant responses are observed in any Umkehr level or in total observed ozone amounts. Further analyses on shorter records for Belsk, Poland, and Hohenpeissenberg, West Germany, corroborate these results. Another analysis for Arosa with about 100 type IV solar flares as keyday zero also shows no definitive trend. It is concluded that ozone distribution changes cannot be the primary causative mechanism for vorticity variations.Journal Paper No. J-8838 of the Iowa Agriculture and Home Economics Experiment Station, Ames, Iowa. Project No. 1852. 相似文献
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J. K. Angell 《Pure and Applied Geophysics》1980,118(1):378-386
Examined are temperature and ozone variations in the Northern Hemisphere stratosphere during the period 1958–77, as estimated from radiosondes rocketsondes, ozonesondes, and Umkehr measurements. The temperature variation in the low tropical stratosphere is a combination of the variation associated with the quasi-biennial oscillation, and a variation nearly out of phase with the pronounced 3-yearly temperature oscillation (Southern Oscillation) present in the tropical troposphere since 1963. Based on radiosonde and rocketsonde data, the quasibiennial temperature oscillation can be traced as high as the stratopause, the phase varying with both height and latitude. However, the rocketsonde-derived temperature decrease of several degrees Celsius in the 25–55 km layer of the Western Hemisphere between 1969 (sunspot maximum) and 1976 (sunspot minimum) is not apparent in high-level radiosonde data, so that caution is advised with respect to a possible solar-terrestrial relation.There has been a strong quasi-biennial oscillation in ozone in the 8–16 km layer of the north polar region, with ozone minimum near the time of quasi-biennial west wind maximum at a height of 20 km in the tropics. A quasi-biennial oscillation in ozone (of similar phase) is also apparent from both ozonesonde data and Umkehr measurements in 8–16 and 16–24 km layers of north temperate latitudes, but not higher up. Both measurement techniques also suggest a slight overall ozone decrease in the same layers between 1969 and 1976, but no overall ozone change in the 24–32 km layer. Umkehr measurements indicate a significant 6–8% increase in ozone amount in all stratospheric layers between 1964 and 1970, and in 1977 the ozone amount in the 32–46 km layer was still 4% above average despite the predicted depletion due to fluorocarbon emissions. The decrease in ozone in the 32–46 km, layer of mid latitudes following the volcanic eruptions of Agung and Fuego is believed to be mostly fictitious and due to the bias introduced into the Umkehr technique by stratospheric aerosols of volcanic origin. Above-average water vapor amounts in the low stratosphere at Washington, DC, appear closely related to warm tropospheric temperatures in the tropics, presumably reflecting variations in strength of the Hadley circulation. 相似文献
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《Journal of Atmospheric and Solar》2003,65(11-13):1235-1243
The aim of the present paper is to study the solar response in the vertical structure of ozone and temperature over the Indian tropical region and a search for any mutual relationship between their solar coefficients on a decadal scale in the lower stratosphere. For the purpose, the data obtained by ozonesonde and Umkehr methods for the lower stratospheric ozone and that of the total ozone amount from Dobson spectrophotometer during the period 1979–2001 have been analyzed. These data are analyzed using the multi-functional regression model, which takes into account most of the known natural and anthropogenic signals. The NCEP- and MSU-satellite data for the temperature over this region have been used. Results indicate an in-phase correlation of around 0.5 between ozone and solar flux (F10.7) in the vertical structure over the equatorial station, Trivandrum (8.3°N) but no significant correlation over Pune (18.3°N). The solar components of ozone and temperature indicate an in-phase but poor correlation in the lower stratospheric altitudes over both stations. However, when total ozone content data is analyzed, it indicates a very high correlation (⩾0.9) between the solar components of ozone and temperature. The solar trend in the vertical distribution of ozone is found to be of the order of 5–25% per 100 units of F10.7 solar flux for Trivandrum but it is relatively smaller (1.6–15.2%) over Pune. The solar dependence of temperature is found to be quite significant for the entire Indian tropical region with not much latitudinal variation. 相似文献
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利用地面遥感O_3垂直分布的逆转方法〈C〉测量出的北京上空O_3剖面资料,对雨云7号卫星的SBUV系统测量的同地区的O_3垂直分布数据进行了订正.对订正后的长达8年(1979—1986年)的完整的SBUV资料进行了较为仔细的分析,得出了这一时期内的O_3垂直分布长期演变呈下降趋势.并在上层O_3含量的季节变化特征和周期振荡等方面,有新的发现,得出一些有意义的结果. 相似文献