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1.
运用随机函数理论将甘东南至陕甘宁交界地区的地震活动能量场看作时间和空间的随机函数,用自然正交函数展开方法,系统研究主要典型能量场的时间权重系数变化曲线以及典型能量场的空间等值线图。结果发现,目标曲线较大幅度的升、降变化预示了可能发生中强地震的时间段,而等值线图的高值变化对应了可能发生中强地震的区域。  相似文献   

2.
云南地区地震活动能量场的时空分布特征   总被引:3,自引:1,他引:3  
罗国富  杨明芝 《中国地震》2005,21(3):332-340
本文运用随机函数理论,将云南地区地震活动能量场看作时间和空间的随机函数,用自然正交函数展开方法,研究地震活动区内主要典型能量场的时间权重系数变化曲线以及该典型能量场的空间等值线图。研究发现,目标曲线较大幅度的升、降变化预示了可能发生中强地震的时间段,而目标等值线图的疏密变化揭示了可能发生中强地震的区域。  相似文献   

3.
运用随机函数理论,将宁夏及邻区地震活动能量场看作时间和空间的随机函数,用自然正交函数展开方法,系统研究宁夏及邻区主要典型能量场的时间权重系数变化曲线以及典型能量场的空间等值线图。结果发现,目标曲线较大幅度的升、降变化预示了可能发生中强地震的时间段,而等值线图的高值变化(危险区)对应了可能发生中强地震的区域。  相似文献   

4.
运用随机函数理论将地震释放能量作为地震活动场的基本要素,采用自然正交函数展开方法系统研究了2013年岷县漳县6.6级地震前震中区域地震活动能量场的时空特征。结果表明:地震前能量场的前4个主要特征值对应的典型能量场时间因子出现明显上升变化,可能是中短期时间异常特征;而主要典型场的空间等值线形成局部能量高值异常危险区,可能是中短期空间异常特征。最后分析不同时间段研究区域均值能量场空间变化图像,显示出岷县漳县6.6级地震前震中确实存在长期的能量场高值危险区背景,短期的能量场均值异常显著变化;宁夏南部及邻区也存在长期的能量场高值危险区背景,只是短期的能量场均值异常不明显,未来几年或稍长时间也存在发生强震的可能。  相似文献   

5.
采用随机能量场的概念,将地震活动能量场看作时间和空间的随机函数场,用自然正交函数展开的分析方法,研究江苏及邻区自1970年1月至2007年12月的中小地震(2.1≤M_L≤4.5)能量场变化特征,以及主要典型能量场的时间"权重"系数的变化特征.结果显示:前7个典型场的展开精度为0.9244.研究区内不同构造块体的地震活动能量场强度存在明显差异,其中下扬子块体的苏中、苏南地区及南黄海海域的地震背景能量值高于其他地区;从典型场的分布来看,该区域对研究区能量场的影响也最为显著.前6个主要典型场的时间"权重"系数随时间的变化幅度与研究区大部分中强震之间在时间上存在很强的相关性.  相似文献   

6.
宁夏及邻近地区地震活动能量场的统计分析   总被引:6,自引:0,他引:6       下载免费PDF全文
杨明芝  赵卫明 《地震学报》2004,26(5):516-522
应用随机函数理论,将区域地震活动能量看作是空间和时间的随机函数,采用自然正交函数展开的分析方法,对宁夏及邻近地区小地震活动场的特征进行了研究.重点分析了场的主要部分,即前几个典型场的时间权重系数的时间变化,发现它们在中强地震发生前数值有较大幅度的升、降变化,显示出了与区域及其周围中强地震相关的变化特性.从宁夏地区的震例看,地震能量随机场的自然正交函数展开方法是一种值得探索的地震分析预测方法.   相似文献   

7.
汶川8.0级地震前地震活动能量场中短期异常   总被引:6,自引:0,他引:6  
罗国富  杨明芝  马禾青  许晓庆 《地震》2011,31(3):135-142
本文应用随机函数理论,将地震释放能量作为地震活动场的基本要素,采用自然正交函数(或称经验正交函数)展开方法,讨论了2008年汶川8.0级地震前区域地震活动能量场的中短期时空异常.结果表明,汶川8.0级地震前震源周围区域能量场的几个主要特征值对应的特征向量(典型场)的时间权重因子出现了明显中长期异常变化,这可能是汶川地震...  相似文献   

8.
运用随机函数理论,系统研究2013年芦山7.0级地震前区域地震活动能量场的时空特征。结果表明,四川芦山7.0级地震前能量场的前2个主要特征值对应的典型能量场时间因子出现明显上升变化,可能是该次地震的中短期时间异常特征;而主要典型场的空间等值线形成局部能量高值异常危险区,该区域可能是芦山7.0级地震的中短期空间异常特征。  相似文献   

9.
许多学者认为2008年汶川8级地震可能对龙门山断裂带及其周围不同断裂带上后续发生的6级以上地震有一定的影响.本文以地震应变场作为地震活动的变量,通过自然正交函数展开方法,研究2008年以来龙门山断裂带周围5次6级以上地震前的地震应变场,提取出震前应变场时空异常的变化.结果表明:(1)2008年汶川8.0级地震前和2013年芦山7.0级地震前地震应变场时间因子分别出现明显的中短期异常和短临异常;而2013年岷县漳县6.6级地震前、2014年康定6.3级地震前和2017年九寨沟7.0级地震前地震应变场时间因子中短期异常不明显,分析其原因主要是受到2008年汶川8.0级地震应变场时间因子最大幅度异常的影响.(2)研究应变场时间因子对应的区域空间等值线变化,发现2009年以后地震应变场空间等值线高值异常区以及异常区周围发生的强震,均可能受到2008年汶川8.0级地震应变场的影响.(3)最后分析1970年以来龙门山断裂带周围地震应变的空间演化过程,总结强震应变变化特征的发震模式,从地震应变演变角度探讨强震之间的相互影响,以及断裂带所在块体间的相互牵制和调整作用.  相似文献   

10.
中国大陆6级以上强震前的地震应变场研究   总被引:1,自引:0,他引:1       下载免费PDF全文
以地震应变场作为地震活动的变量,通过自然正交函数展开方法,计算了中国大陆6级以上强震前的地震应变场,提取出震前时间因子的异常变化.计算结果分析发现大地震前时间因子在平稳背景上会出现突跳上升或突跳下降变化,且震前地震应变场前4个典型场中至少有3个典型场会出现异常变化,具有多分量显示异常的特点,而异常出现的最早时间大约在震前3年,并且一些地震前出现短临的时间因子异常变化特征.通过震例研究表明用地震应变场分析地震活动异常,提取的时间因子异常结果比应用地震能量场更具有独特的优越性,并讨论了应变场与能量场的差异.  相似文献   

11.
The determination of the coefficient of viscosity of eruptive products gives useful elements to the knowledge of possible variations of composition and physical conditions of the magmas.  相似文献   

12.
13.
Geomagnetism and Aeronomy - The magnetic evolution of the active region of the Sun at the level of the photosphere has been studied. Magnetic synoptic maps of the 2007 Kitt Peak Observatory were...  相似文献   

14.
15.
Until recently, the existing data prevented the geophysicists from accurately dating the Bysy-Yuryakh stratum, which outcrops in the middle reach of the Kotuy River, constraining the time of its formation to a wide interval from the end of the Late Cambrian to the beginning of the Silurian. The obtained paleomagnetic data unambiguously correlate the Bysy-Yuryakh stratum to the Nyaian regional stage and constrain its formation, at least a considerable part of it, by the Tremadocian. This result perfectly agrees with the data on the Bysy-Yuryakh conodonts studied in this work and yields a spectacular example of the successful application of paleomagnetic studies in solving important tasks of stratigraphy and, correspondingly, petroleum geology. Within the Bysy-Yuryakh stratum, we revealed a large normal-polarity interval corresponding to the long (>1 Ma) period when the geomagnetic reversals were absent. This result, in combination with the data for the Tremadocian and Middle–Upper Cambrian sequences of the other regions, indicates that (1) the rate of occurrence of the geomagnetic reversals on the eve of the Ordovician Moyero superchron of reversed polarity was at most one reversal per Ma; (2) the superchron does not switch on instantaneously but is preceded by a certain gradual change in the operation conditions of the dynamo mechanism which, inter alia, manifests itself by the reduction of the frequency of geomagnetic reversals with the approach of the superchron. This finding supports the views according to which a process preparing the establishment of the superchrons takes place at the core–mantle boundary.  相似文献   

16.
Summary A simple model is proposed suitable for studying the effect of the ground layer of the atmosphere, polluted by aerosol, on the albedo. This model is founded on solving the equation of transfer of radiative energy. The numerical results are discussed, particular attention being paid to the analysis of errors due to neglecting the multiple reflection of solar radiation on the aerosol particles. A method which would also include the multiple reflection is proposed, and the conditions under which the presence of the aerosol is responsible for an increase or decrease of the solar radiation balance on the Earth's surface, are analysed.  相似文献   

17.
Summary The results of two different methods of the determination of the non-linearity of the gravimeter scale are compared; the economy is discussed as well.  相似文献   

18.
Atmospheric temperature and humidity fields as well as information on other meteorological parameters are nowadays retrieved from radiance measurements recorded by operational meteorological satellites. Up to now, the inversion procedures used only take into account crude information on the topography of the Earth’s surface. However, the applied radiative transfer codes have to consider the Earth’s surface as the lower boundary of the atmospheric model and, therefore, need a more precise mean elevation and a classification of the roughness of the Earth’s surface. The influence of the topography of the Earth surface on retrieved temperature profiles is studied by using a physico-statistical inversion method. An objective analysis is made of the more precise mean elevation and derivation of roughness parameters using a new high-resolution digital elevation model (DEM) with a resolution of 500 m×500 m. By means of a geomorphological process and a newly developed topography rejection test, areas with a high surface roughness are localized and singled out. The influence of topography on the retrieved temperature profiles is illustrated by case studies. Changes are found predominantly in areas with a high variation of topography. Using the new high-resolution DEM and the topography rejection test, the geographical position of the calculated temperature profiles tends to be shifted towards areas with a small vertical variation of topography. The mean elevation determined by the new elevation model better characterizes the area observed. Hence, the temperature profiles can be calculated down to lower atmospheric levels. Furthermore, a guess profile better describing the atmospheric situation is selected by the more precise elevation. In addition, the temperature profiles obtained near the coast are improved considerably by the more precise determination of the surface property ‘sea’ and ‘land,’ respectively. Integration of an independent physical information such as topography leads, on average, to a slight improvement of the results of the physico-statistical inversion procedure. In some cases, however, significant improvements have been achieved regarding the desired accuracy of temperature profiles of the order of 1 K. In future, the spatial resolution of new high-resolution sounding instrumentation on the next generation of operational meteorological satellites will be increased. To exploit the resolving power of this new instrumentation, the different variation of the topography of the Earth surface, especially in regions with a high variation of topography, can be taken into account more precisely by using a high-resolution DEM.  相似文献   

19.
Резюме Дается вывод формул для вычислений длины хорды, длины и азимутов нормаляных сечений и длины геодезической линии эллипсоида. Применяются тригонометрические функции данных величин и постоянные принятого ргфгргнц-эллипсоида, что является целесообразным при использовании вычислителQjных машин, особенно автоматов. Рабочие формулы рекомендуются в форме (8–11).

Dedicated to Professor František Fiala on His 85th Birthday

Address: Veveři 95, Brno.  相似文献   

20.
Summary The maintenance of the axisymmetric component of the flow in the atmosphere is investigated by means of a steady-state, quasi-geostrophic formulation of the meteorological equations. It is shown that the meridional variations in the time-averaged axisymmetric variables can be expressed as the sum of three contributions, one being due to the eddy heat transport, another to the eddy momentum transport, and a third to the convective-radiative equilibrium temperature which enters the problem through the specification of a Newtonian form of diabatic heating. The contributions by the large scale eddies are evaluated through the use of observed values for the eddy heat and momentum transports.The contributions from each of the three forcing mechanisms to the temperature and zonal wind fields are invstigated individually and found to be of about equal importance. The sum of the three contributions are also presented for the temperature, the zonal wind, the stream function associated with the mean meridional circulation and the corresponding vertical motion. Although the results fail to reproduce the main observed features of the lower stratosphere, they are found to be in good agreement with observations in the middle latitude troposphere. At any pressure level, for example, the computed mean zonal wind has a jet-like profile and the axis of the jet is found to slope to the south with height, as observed in the atmosphere.Based in part on a thesis submitted by the first author as partial fulfillment of the requirements for the Ph.D. degree at the University of Michigan. — Publication No. 194 from the Department of Meteorology and Oceanography, The University of Michigan.  相似文献   

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