一种简单方便的防拷贝程度设计方法：识别计算机的C语言程序…

本主要讨论一种特殊的Ｃ语言程序设计方法，这种程序能有效地对自身的关键模块加密，能运行是地完成动态解密。     

苏联经济区方案定量研究的经验

通常,经济区划的任务包括以下几个主要阶段:1) 确定作为基础区的地域;2)按照基础区选择区划指标系统及其定量评价;3) 选择区域系统模式;4) 阐明课题建立算法,直接把基础区进行分类计算;5)解释已获得的结果,选出最好的区划方案和有关进一步改善工作方法的结论等等。基础区的范围视所要解决的任务性质而定。     

上一轮实施的基本评估和对新一轮的建议 龙泉市土地利用总体规划

土地利用总体规划是在一定区域内,根据国家社会经济可持续发展的要求和当地自然、经济、社会条件,对土地的开发、利用、治理、保护在空间上、时间上所作的总体安排和布局,是国家实行土地用途管制的基础。县、乡级土地利用总体规划属实施性规划,其主要任务是按照上级土地利用总体规划的指标和布局要求,划分土地利用区,明确各土地利用区的土地主要用途和区内土地使用条件,为单位和个人合理使用土地,进行土地开发、整理提供依据,为政府审批农     

景观单元评价方法

本文通过对瓜达卢皮山国家公圆的分区和评价,提出了一种对土地系统和景观单元进行划分的方法。划分土地系统和景观单元,以许多相关因素作为基础。给一些小的区域下定义,然后再将这些小区域合并成大区域。     

利用射电源位置残差解算章动系数的改正

章动序列的不准确引起春分点和黄赤交角的变化，直接影响到射电源的赤经、赤纬。利用IRIS网五天一组的VLBI观测资料，我们解算了定组观测的13颗射电源的赤经、赤纬，从射电源的位置残差解算出黄经章动和交角章动的改正，并估算了章动周年项（365.3天）和半年项（182.6天）的系数改正及自由核章动的振幅。     

Magnetic Field Strengths and Structures from Radio Observations of Solar Active Regions

Radio observations of some active regions (ARs) obtained with the Nobeyama radioheliograph at λ=1.76cm are used for estimating the magnetic field strength in the upper chromosphere, based on thermal bremsstrahlung. The results are compared with the magnetic field strength in the photosphere from observations with the Solar Magnetic Field Telescope (SMFT) at Huairou Solar Observing Station of Beijing Astronomical Observatory. The difference in the magnetic field strength between the two layers seems reasonable. The solar radio maps of active regions obtained with the Nobeyama radioheliograph, both in total intensity (I-map) and in circular polarizations (V-map), are compared with the optical magnetograms obtained with the SMFT. The comparison between the radio map in circular polarization and the longitudinal photospheric magnetogram of a plage region suggest that the radio map in circular polarization is a kind of magnetogram of the upper chromosphere. The comparison of the radio map in total intensity with the photospheric vector magnetogram of an AR shows that the radio map in total intensity gives indications of magnetic loops in the corona, thus we have a method of defining the coronal magnetic structure from the radio I-maps at λ=1.76 cm. Analysing the I-maps, we identified three components: (a) a compact bright source; (b) a narrow elongated structure connecting two main magnetic islands of opposite polarities (observed in both the optical and radio magnetograms); (c) a wide, diffuse, weak component that corresponds to a wide structure in the solar active region which shows in most cases an S or a reversed S contour, which is probably due to the differential rotation of the Sun. The last two components suggest coronal loops on different spatial scales above the neutral line of the longitudinal photospheric magnetic field.     

黄河口水下底坡微地貌及其成因探讨

高分辨率的回声测深、旁侧声纳及浅地层剖面记录首次直观地揭示了黄河口水下底坡上发育有大量形态不同的微地貌类型。据其形态特征和规模的差异,将它们划分为平滑海底、凹坑与洼地、冲沟、残留岗丘及扰动复合海底等五种类型。这些微地貌分布在不同水深条件下的不同水下三角洲单元上,并存在着相互联系和相互转化。黄河口海域特殊的沉积环境和复杂的动力条件是导致水下底坡微地貌形成发育的主要机制。