台湾集集大地震断层非均匀滑动分布的反演

利用台湾1999集集大地震前后GPS测量获得的地表位移数据,反演断层面上的非均匀滑动分布.反演中采用二次样条函数作为滑动分布的基函数,通过引入阿卡克贝叶斯准则,获得了反演问题的惟一解.反演得到的地表位移与实测位移的差在几个厘米,较好地解释了观测到的GPS位移.另一方面,用反演结果计算得到的地表形变场同INSAR得到的地表实测位移场较相近.     

利用任意时刻AVHRR资料近似估计区域地表温度日较差的试验

根据表征土壤温度日变化的土温方程一阶近似解，提出一种利用一日中任意时刻NOAA－AVHRR图像数据估计地表温度日较差的简易推算方法。该方法尤其可用于反演土壤含水量的计算，当图像数据的时次与热惯量法所要求的最高、最低温度时次配不准的情况下，近似地估计地表温度日较差，进而计算地表热惯量及相应的土壤含水量。用实例验证了该方法的可行性，为进一步推广应用奠定基础。     

论地质作用中元素间的相关性及制约因素

本文把地质作用中元素间的相关性划分为曲线相关、准线性相关和线性相关三种类型;并在建立反映岩浆、沉积作用过程中元素间相关关系的数学模型及其它工作的基础上,详细讨论分配系数、源区成分和作用过程等方面对地质作用中元素间相关关系的制约作用。进而获得批式熔融、结晶分异、岩浆混合、化学沉积、碎屑沉积等过程中元素间呈线性和(?)线性关系的一般特征和应用前景。最后还给出La/Ce相关性的应用实例。     

康古尔塔格硅灰石矿床地质特征与成矿条件分析

作者首次在该区找到了硅灰石矿。在专题研究基础上，分析了区域地层、构造、岩浆活动和硅灰石矿床地质特征等，提出该硅灰石矿主要产于康古尔断裂带内的花岗岩与碳酸盐地层接触带，属矽卡岩型硅灰石矿。对区内花岗岩、碳酸盐地层、矽卡岩、大地构造等硅灰石成矿条件作了分析，初步提出了该矿主要应用领域为建筑陶瓷工业。     

A Flare-Triggered Heating of a Quiescent Filament

Using data obtained with the 20-cm H full-disk telescope at Big Bear Solar Observatory and Fexii 195 Å EIT on SOHO, we analyze a sudden disappearance event of a quiescent filament in detail. The filament was located along the common boundary of the active regions NOAA 9672 (S19 E13) and NOAA 9673 (N03 E18). The filament disappeared during a time interval between 17:59 UT and 19:47 UT on 22 October 2001 immediately after the onset of a major flare, which occurred in the active region NOAA 9672. At about 23:23 UT of the same day, the filament began to reappear in H and, after about 15 hours, the filament recovered to its steady state with its size being slightly smaller than that before its disappearance. This filament disappearance event belongs to the thermal type of sudden filament disappearances, which is caused by an input of additional heat. The heating mechanism that leads to sudden thermal disappearances of quiescent filaments is still not well understood. This simple event, due to the explicit cause and effect relationship between the flare and the disappearance of the filament, shows us that the flare triggered some kind of heating mechanism which continued several hours. The heat may come from the flare via heat conduction from its ribbon or from the excitation of dissipating Alfvén waves. However, from the data analysis, we conclude that the flare triggered an in-situ heating, which is likely caused by magnetic reconnection.     

在97.8GHz处测量地球大气的不透明度

用研制的全自动辐射计在97．8GHz上测量南京市内大气的不透明度以及这种不透明度随时间的变化．辐射计记录大气在不同天顶高度的辐射温度,由此测出天顶方向的大气不透明度。在56小时的测量时间内,取得了1400多组数据,拟合得到了在观测时段内天顶方向的大气不透明度在0．2至0．7之间,典型值为0．4,表明测试地点的大气条件允许进行3mm波段的射电天文观测．由于在工作频段内大气不透明度的主要来源是对流层水汽的吸收,测量的不透明度可用来直接反映大气内水汽的含量,并实时校准大气吸收．