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1.
The heights of the daytime convective boundary layer (CBL), computed by a one-dimensional model for a bare soil surface at a semi-arid station,Anand, during the dry and hot summer month of May 1997, are presented. As input, the model requires surface heat flux, friction velocity and air temperature as functions of time. Temperature data at the one-metre level from a tower and sonic anemometer data at 9.5 m collected during the period 13–17 May 1997 in the Land Surface Processes Experiment (LASPEX-97) are used to compute hourly values of surface heat flux, friction velocity and Obukhov length following the operational method suggested by Holtslag and Van Ulden [J. Climate Appl. Meteorol. 22,517–529 (1983)]. The model has been tested with different values for the potential temperature gradient ( ) above the inversion. The model-estimated CBL heights comparefavourably with observed heights obtained from radiosonde ascents.  相似文献   
2.
秘金钟  李毓麟  张鹏 《测绘科学》2002,27(2):10-12,45
应用“中国地壳运动观测网络”1998年到 2 0 0 0年的多期 GPS联测数据 ,得到“网络工程”基准站和基本站各点在 ITRF97框架下的速度场 ,以及相对于 NNR- NUEARL1A模型的中国大陆板内运动速度场和相对于某一单站 (如 CHAN站 )的速度场 ,并对速度场信息的可靠性进行了初步分析。  相似文献   
3.
For at least 30 years now it has been well known that the Dst index can be modelled using the solar wind as input. Since then, many attempts have been made to improve the predictability of Dst using different approaches. These attempts are useful, for instance, to understand which features of the solar wind–magnetosphere interactions are most important in producing magnetospheric activity and how the Dst index would improve the space weather forecast. The Dst index is by far the most reliable and simple indication that a magnetic storm is in progress. In this work, the effect of using more than four magnetic stations and shorter time intervals than the hourly averages used in Sugiura's procedures is evaluated. The discussion is based on the results presented by Burton in 1975 and Feldstein in 1984 considering 4 or 12 magnetic stations and time averages of 2.5 min for a magnetic disturbed period that occurred from February 7–28, 1967, including two geomagnetic storms. The analysis has shown that the global representation of a magnetic storm by the standard Dst (Sugiura) is well preserved either using 4, 6, 12 magnetic stations or using 1 h, 2.5 min 1 min averages. A brief review of the current understanding of Dst has been included to support the discussions. The analysis performed has shown that a more refined Dst index (time and number of stations>4) would be useful to investigate the intrinsic processes and the different current systems involved in the ring current development during magnetic storms; the standard Dst, as it is conceived, is quite adequate to monitor geomagnetic storms and identify their overall features; concerning the magnetic stations normally considered, the inclusion of higher magnetic latitude stations (>35) may underestimate the observed Dst.  相似文献   
4.
5.
介绍利用Access97编制科技论文登记数据库的具体过程及使用方法。通过该数据库,可以及时将发表的科技论文入库。当论文全部入库后,可以方便地进行查询及统计,从而得出有效的数据,大大提高了工作效率。  相似文献   
6.
~~Global tectonics and the plate motion obtained from the ITRF97 station velocity vectors@马宗晋 @任金卫 @张进~~  相似文献   
7.
We hypothesize that the spatial and temporal variation in large-scale soil moisture patterns can be described by a small number of spatial structures that are related to soil texture, land use, and topography. To test this hypothesis, an empirical orthogonal function (EOF) analysis is conducted using data from the 1997 Southern Great Plains field campaign. When considering the spatial soil moisture anomalies, one spatial structure (EOF) is identified that explains 61% of the variance, and three such structures explain 87% of the variance. The primary EOF is most highly correlated with the percent sand in the soil among the regional characteristics considered, but the correlation with percent clay is largest if only dry days are analyzed. When considering the temporal anomalies, one EOF explains 50% of the variance. This EOF is still most closely related to the percent sand, but the percent clay is unimportant. Characteristics related to land use and topography are less correlated with the spatial and temporal variation of soil moisture in the range of scales considered.  相似文献   
8.
Astrometric and photometric observations of major planets, their satellites and asteroids have been made with the 26-in. refractor of the Pulkovo observatory during the period from 1995 to 2006. The CCD (ST6) and photographic observations were carried out. Accurate relative position of satellites of Jupiter and Saturn have been derived. The positions of Saturn have been calculated using the theoretically predicted coordinates of satellites relative to the planet without measurements of the photographic images of the planet. Also the observations of Hale-Bopp comet and Mercury transit have been made. The 26-in. refractor has been included into the international campaign PHEMU-2003: photometric CCD observations of mutual occultations and eclipses of Galilean satellites. The light curves of the events have been obtained and parameters of the events have been determined.  相似文献   
9.
在随着2000国家大地坐标系在全国不断推广与应用,将ITRF2000框架下的坐标转换到CGCS2000框架时,需先转换到ITRF1997框架下。本文采用布尔沙-沃尔夫模型对基于不同基准的两框架之间进行坐标转换,设计了七参数求解程序,并通过实例分析验证其准确性和可靠性。  相似文献   
10.
ITRF97下空间对地观测站速度矢量显示的全球构造运动   总被引:3,自引:2,他引:3  
利用ITRF97的站速度矢量研究现代地壳运动特征,发现ITRF97站速度矢量与NUVEL-1A板块运动模型有很好的一致性. 它们共同显示,北半球以北大西洋为轴向北东、北西向裂开,欧亚大陆向北东、东、南东运动; 北美大陆向北西、西、南西运动, 但南半球板块运动状态截然不同, 南美、非洲、印-澳三板块各自的本体运动几乎全部指向北东-北北东, 三者之间以南大西洋脊和印度洋脊为界, 而且运动矢量逐次加大, 呈现南半球整体运动与洋脊张裂运动的叠加所造成的“落后式”拉张关系, 北半球和南半球之间速度矢量场的差异十分明显, 显示其间运动场不协调带, 此带内地质调查早已确定存在一组斜列式断续延伸的剪切破裂带. 沿此南/北半球之间的运动不协调带及其内部的大断裂带自1999年8月至2001年1月连续发生8次M≥7.8地震, 而环太平洋俯冲带内地震活动则明显降低, 充分显示了南/北半球之间的运动不协调带在全球板块运动中所显示的全球尺度的独立地位. 验算结果初步揭示了南/北半球之间的相对错动关系.  相似文献   
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