dMe耀星的X射线的辐射

From Einstein Observatory, we know most nearby dM flare stars have X-ray emissions. X-ray flare energy of dM stars is far larger than that of large flares of sun. The corona temperature of dM stars is higher than that of sun. The X-ray flare time scales are several minutes to hours. Star corona heating model for X-ray flares is loop model, which provide a mechanism to convert magnetic energy to heat energy in star corona.Within identification of ROSAT X-ray sources, we found that X-ray source: RX1102.0 4347 corresponds to WX UMa, a dM5e flare star, which is in a nearby visual binary: Gliese 412A B. The binary is very near to earth, 5.38pc, and has high proper motion, 4".54/ year. The binary is also an Einstein X-ray source: 1 E1103.0 4346.In March 27, 1993, we observed WX UMa by CCD BVRI photometry at BAO 2.16m telescope. Magnitudes of the star are: V = 14.56, B-V = 1.95, V-R = 0.97, R-I = 2.06, which are similar to previous observations.From the ROSAT X-ray survey data in November 7-17, 1990, average X     

安徽滁州市旅游资源开发利用研究

分析滁州市旅游资源的特点以及开发利用条件，并对滁州市旅游资源开发利用总体规划与措施提出一些基本设想     

大陆岩石圈对扩张机制的响应——辽蒙地质走廊中—新生代火山活动的时空分布

选择以辽西为中心,近东西向延伸800km的辽蒙地质走廊为研究区,通过年代学研究,确认130Ma以来的中、新生代火山活动对称分布的时空格局具有“中间老、两侧新”的特点,而且随着时间的推移,软流圈来源的岩浆向东西两侧侧向流动,岩浆来源不断加深。在此基础上提出“软流圈底辟体上涌和水平侧向流动”的模式。     

海底隧道体系地震反应分析方法

本文研究海底隧道体系在深部一个底面处给定的地震动作用下的反应分析方法。研究中计及了海水的影响,采用了有限元模型和时域解法。其中,根据作者的先期研究结果,给出了考虑海水影响的质量矩阵的形成方法根据岩-土叠合一类体系的阻尼分布特点,以及不再适宜用经典阻尼矩阵描述体系相应特性的考虑,经过物理分析,给出了与问题的物理图式符合较好的阻尼矩阵的形成方法;最后对一实例进行了数值计算和结果分析,说明了有关的几个问题。     

剪切运动在区域构造演化中的作用与意义：兼论开,合,剪的关系

本文从区域构造角度论述了剪切运动的普遍性和重要性,讨论了开、合、剪三种运动的辩证关系.剪切运动在区域构造演化中扮演着重要角色:转换断层协调大洋板块的扩张与俯冲;走滑断裂协调大陆盆地形成、造山带演化和地体运移;韧性剪切协调深部构造变形,并将地表构造和深部构造结合起来.开、合、剪处于同一运动系统中,其中开合是一对主要矛盾,剪切是桥梁与纽带;开、合往往导致突变与质变,剪切经常表现为渐变与量变.开、合、剪的辩证关系体现其运动的整体性、层次性、旋回性、互补性、共生性和互为因果等特征.