基于网络加权Voronoi图分析的南京市商业中心辐射域研究

道路网络在城市社会和经济活动中发挥重要作用.它是联系商业中心与需求间的桥梁.道路系统的更新与变化必然会对它们的关联产生影响Voronoi图足划分势力空间的有效工具,基于道路网络分析构建的加权Voronoi图可以模拟城市商业中心功能辐射的实际情形.本文给出了基于道路网络分析的Voronoi图和加权Voronoi图构建方法.通过对各种Voronoi图的比较分析,认为基于网络路径时间分析构建的加权Voronoi面域图在商业中心辐射域模拟中最为有效.将空间相互作用和断裂点理论与网络加权Voronoi面域图相结合.模拟不同交通条件下南京市商业中心辐射域空间格局及其需求覆盖变化,并提取了辐射域的覆盖面积、覆盖人口、最远辐射路径距离和平均辐射路径距离等信息.对商业中心的地铁邻近度与其辐射域的扩张面积进行相关分析.采用域邻接矩阵描述空间划分平衡与不平衡之间的相互转变过程,可分析道路系统变更后商业中心之间空间竞争的变化趋势.分析结果表明商业中心的地铁邻近度与辐射域的扩张具有较大的相关性,快速轨道交通在商业中心空间竞争中发挥关键作用.     

γ射线噪Blazar天体中尘埃的作用

利用具有多波段谱指数及流量观测资料的５９ 个Ｂｌａｚａｒ 天体作为样本,我们研究了各波段流量之间,谱指数之间的可能的相关性。新的可能的限制已从理论上进行了深入地讨论。结果暗示：（１） 同步自康普顿机制是Ｂｌａｚａｒ 天体γ射线辐射的主要机制。（２） 相对论电子与吸收积盘热光子的逆康普顿散射是Ｂｌａｚａｒ 天体γ射线产生的另一个重要机制。（３）ＢＬＬａｃ 天体不是“纯非热辐射”的天体,它们也具有强的热辐射。     

基于DEM的黄河流域天文辐射空间分布

Based on the developed distributed model for calculating astronomical solar radiation (ASR), monthly ASR with a resolution of 1 km× 1 km for the rugged terrains of Yellow River Basin was calculated, with DEM data as the general characterization of terrain. This model gives an all-sided consideration on factors that influence the ASR. Results suggest that (1) Annual ASR has a progressive decrease trend from south to north; (2) the magnitude order of seasonal ASR is: summer＞spring＞autumn＞winter; (3) topographical factors have robust effect on the spatial distribution of ASR, particularly in winter when a lower sun elevation angle exists; (4) the ASR of slopes with a sunny exposure is generally 2 or 3 times that of slopes with a shading exposure and the extreme difference of ASR for different terrains is over 10 times in January; (5) the spatial differences of ASR are relatively small in summer when a higher sun elevation angle exists and the extremedifference of ASR for different terrains is only 16% in July; and (6) the sequence of topographical influence strength is: winter＞autumn＞spring＞summer.     

Anisotropic Beam Model for the Spectral Observations of Radio Burst Fine Structures on 1998 April 15

A fine structure consisting of three almost equidistant frequency bands was observed in the high frequency part of a solar burst on 1998 April 15 by the spectrometer of Beijing Astronomical Observatory in the range 2.6-3.8GHz. A model for this event based on beam-anisotropic instability in the solar corona is presented. Longitudinal plasma waves are excited at cyclotron resonance and then transformed into radio emission at their second harmonic.The model is in accordance with the observations if we suppose a magnetic field strength in the region of emission generation of about 200G.     

Back reaction and Hawking radiation from a Vaidya black hole

Using Damour-Ruffini’s and Hamilton-Jacobi’s methods, Hawking radiation from a Vaidya black hole is investigated. Due to non-stationary black holes, the event horizon r _H and the entropy S are all related to both the mass m(υ) and . When the back-reaction of particles’s energy to space-time is considered, we get the emission probability. It is found that the result is different from that of the stationary Schwarzschild black hole, because is the function of mass m(υ).      

古尔班通古特沙漠的辐射热量交换分析

位于新疆准噶尔盆地的古尔班通古特沙漠是我国第二大沙漠。根据古尔班通古特沙漠的自然条件,对不同下垫面区域的太阳短波辐射和大气长波辐射热量进行了测量。结果表明:在晴天状况下,流动沙丘和固定沙丘的热量交换差异主要是由地表状况、沙层性质和气温等因素决定的。流动沙丘区反射率与长波辐射大于固定沙丘区,并且日、季变化明显。长波最大辐射值出现在午后,近似于太阳总辐射,最小值出现在日出前;沙层热通量随着深度的增加而增大,而辐射热量传输则随其深度的增加而减小,无论是流动沙层还是固定沙层,其热通量的零界面深度却基本一致(9月份),均在30~35cm之间。根据上述结果,本文还讨论了沙漠区在热量交换过程中,辐射热量差异引起的沙漠小气候效应和沙漠对区域气候的反馈作用。