中国大陆水平地壳运动的数学模型

在获得中国区域1000个实测GPS台站速度场的基础上,利用多面函数法、滑动欧拉矢量法和滑动弹塑性模型法建立了中国大陆水平地壳运动模型,统计表明3种方法外部符合精度2～4mm/a,模型互差精度约为3mm/a。     

一类多物种生态模型的稳定性

应用李雅普诺夫直接法研究了一类多物种生态模型的稳定性，给出了系统的局部和全局稳定性的充分条件。     

地壳相对活动区的灰色划分

本文根据灰色系统中的聚类原理,提出了有关复测网区内地壳活动区的灰色划分方法,即根据动态平差得到的观测值速率和关联度这两个灰类指标,对观测值按不同的灰类进行灰色聚类,从而划分地壳的相对活动区。文中给出了重力网重复观测值的灰色关联度、聚类权以及灰类白化函数的计算方法,并用一个复测重力网资料进行了计算,结果表明:用该方法所划出的相对活动区与实际情况比较符合。     

土地利用分类及其影响因素研究

土地利用分类是研究土地利用的最基础工作，它直接影响着土地利用的科研与实践，本文在全面研究土地利用分类理论与方法的基础上，比较且说明了当前国内外土地利用分类的优劣。并提出多层统一标准的系统分类设想。     

A THEORETICAL DISCUSSION ON TYPES AND MEASUREMENT OF SUSTAINABLE DEVELOPMENT

１ＩＮＴＲＯＤＵＣＴＩＯＮＴｈｅｃｏｒｅｏｆｇｅｏｇｒａｐｈｉｃａｌｓｔｕｄｉｅｓｔｈｅａｒｅａｌｓｙｓｔｅｍｏｆｍａｎｌａｎｄｒｅｌａｔｉｏｎｓｈｉｐＷＵ１９９１ｉｓｔｈｅｓｔａｒｔｉｎｇｐｏｉｎｔｏｆｓｔｕｄｙｉｎｇｒｅｇｉｏｎａｌｓｕｓｔａｉｎａｂｌｅｄｅｖｅｌｏｐｍｅｎｔ．Ｆｒｏｍｔｈｅｐｏｉｎｔｏｆｓｕｓｔａｉｎａｂｌｅｄｅｖｅｌｏｐｍｅｎｔｔｈｅｃｏｏｒｄｉ-ｎａｔｉｏｎｏｆｍａｎｌａｎｄｒｅｌａｔｉｏｎｓｈｉｐｉｓｄｅｖｅｌｏｐｍｅｎｔｓｕｓｔａｉｎ-ａｂｉｌｉｔｙ．…     

GPS水准的有限元法与多面函数法的加权综合模型

应用有限元法与多面函数法的加权综合模型改进拟合模型在逼近高程异常曲面时的拟合效果。由大地高求出准确的正常高，通常应用有限元法或多面函数法等单一拟合模型来拟合高程异常曲面。GPS水准的单一模型在逼近高程异常曲面时其拟合效果往往不稳定。通过对实测数据的计算分析可发现：有限元法与多面函数法的加权综合模型的逼近结果比单一模型的逼近结果有了一定的提高。由此可见综合模型对于局部地区解决GPS高程转化为正常高是有使用价值的。     

Stellar contents of two young open clusters: NGC 663 and 654

UBVRI CCD photometry in a wide field around two young open clusters, NGC 663 and 654, has been carried out. Hα and polarimetric observations for the cluster NGC 654 have also been obtained. We use the photometric data to construct colour–colour and colour–magnitude diagrams, from which we can investigate the reddening, age, mass and evolutionary states of the stellar contents of the these clusters. The reddening across the cluster regions is found to be variable. There is evidence for anomalous reddening law in both clusters; however, more infrared and polarimetric data are needed to conclude about the reddening law. Both clusters are situated at about a distance of 2.4 kpc. Star formation in both clusters is found to be a continuous process. In the case of NGC 663, star formation seems to have taken place sequentially, in the sense that formation of low-mass stars precedes the formation of most massive stars. Whereas, in the case of NGC 654, formation of low-mass stars did not cease after the formation of most massive stars in the cluster.