A solar flare in the Fe I 5324 line on 24 June, 1993     

Lin Yuanzhang  Zhang Hongqi  Zhang Wenjian 《Solar physics》1996,168(1):135-143

A solar flare with both H and Fe i 5324 emissions was observed in AR 7529 (S13, E65) on 24 June, 1993 at the Bejing Astronomical Observatory. Our calculations show that the Fe i 5324 emission region of the flare was located in the low photosphere at a height of about 180 km above ₅₀₀₀ = 1, which is lower than many previous studies of white-light flares. To study a Fe i 5324 flare, which represents a kind of extreme case in solar flares, would be useful for clarifying some arguments in the researches of white-light flares as well as for understanding the mechanism of solar flares.The synthetic analyses from vairous features of the flare lead to the following possible exciting mechanism of the Fe i 5324 flare: owing to the flow of energetic electrons from the corona and probably also the thermal conduction downward into the lower atmosphere, a condensation with a temperature higher than that below it was formed near the transition region. Then the low photosphere was heated through backwarming. The Fe i 5324 flare occurred as an indicator of the excitation in the low photosphere.  相似文献   

Configuration of the chromospheric magnetic field in a unipolar sunspot region     

Hongqi Zhang 《Solar physics》1994,154(2):207-214

A set of H chromospheric magnetograms at various wavelengths near the line center, chromospheric Dopplergrams, and photospheric vector magnetograms of a unipolar sunspot region near the solar limb were obtained with the vector video magnetograph at the Huairou Solar Observing Station. The superpenumbral chromospheric magnetic field is almost parallel to the surface at the outside of the sunspot penumbra, where the magnetic lines of force are mainly concentrated in the superpenumbral filaments. In the gaps between the filaments the chromospheric horizontal field is weak.  相似文献   

Universal birefringent filter with a new double passband mode     

Jingshan Wang  Guoxiang Ai  Guofeng Song  Bin Zhang  Xiangming Ye  Yingping Nie  Tzihong Chiveh  Weanshun Tsay  Huanshin Li 《Solar physics》1995,161(2):229-239

This article describes the universal birefringent filter (UBF) which will be mounted at Taiwan. The UBF permits observations of solar images, vector magnetic fields and/or line-of-sight velocity fields in any Fraunhofer line in the wavelength region from 4000 to 7000 with half width from 0.05 to 0.14 . We have tested it at ten Fraunhofer lines under a spectral telescope in Huairou Station of Beijing Astronomical Observatory and obtained the passband profiles. The principles of magnetic field and velocity field measurement with the UBF are also described.  相似文献   

Increasing critical sensitivity of the Load/Unload Response Ratio before large earthquakes with identified stress accumulation pattern   总被引：2，自引：0，他引：2  

Huai-zhong Yu  Zheng-kang Shen  Yong-ge Wan  Qing-yong Zhu  Xiang-chu Yin   《Tectonophysics》2006,428(1-4):87-94

The Load/Unload Response Ratio (LURR) method is proposed for short-to-intermediate-term earthquake prediction [Yin, X.C., Chen, X.Z., Song, Z.P., Yin, C., 1995. A New Approach to Earthquake Prediction — The Load/Unload Response Ratio (LURR) Theory, Pure Appl. Geophys., 145, 701–715]. This method is based on measuring the ratio between Benioff strains released during the time periods of loading and unloading, corresponding to the Coulomb Failure Stress change induced by Earth tides on optimally oriented faults. According to the method, the LURR time series usually climb to an anomalously high peak prior to occurrence of a large earthquake. Previous studies have indicated that the size of critical seismogenic region selected for LURR measurements has great influence on the evaluation of LURR. In this study, we replace the circular region usually adopted in LURR practice with an area within which the tectonic stress change would mostly affect the Coulomb stress on a potential seismogenic fault of a future event. The Coulomb stress change before a hypothetical earthquake is calculated based on a simple back-slip dislocation model of the event. This new algorithm, by combining the LURR method with our choice of identified area with increased Coulomb stress, is devised to improve the sensitivity of LURR to measure criticality of stress accumulation before a large earthquake. Retrospective tests of this algorithm on four large earthquakes occurred in California over the last two decades show remarkable enhancement of the LURR precursory anomalies. For some strong events of lesser magnitudes occurred in the same neighborhoods and during the same time periods, significant anomalies are found if circular areas are used, and are not found if increased Coulomb stress areas are used for LURR data selection. The unique feature of this algorithm may provide stronger constraints on forecasts of the size and location of future large events.  相似文献   

ZnS柱撑高岭石-蒙脱石混层矿物纳米复合材料的制备及其光降解伊红-B的研究     

杨浩文李金洪  赵文婷苗世顶 《岩石矿物学杂志》2005,24(6):578-582

以硫尿和乙酸锌为前驱物,通过离子交换和溶液热反应的方法在有机高岭石蒙脱石混层矿物(高蒙混层矿物)层间原位合成了ZnS纳米粒子,得到ZnS柱撑高岭石蒙脱石混层矿物纳米复合材料。X射线粉末衍射分析(XRD)表明高蒙混层矿物的d001从原来的0.98nm被柱撑到1.95nm,表明层间被插入了直径小于1nm的ZnS纳米颗粒。扫描电镜(SEM)观察发现,原高蒙混层矿物的有序片层结构部分被破坏,在被剥离的片层上面均匀覆盖了ZnS颗粒聚集体,粒径在25nm左右。透射电镜(TEM)显示,ZnS颗粒聚集体是由3～5nm的颗粒堆积而成,夹杂在被剥离的高蒙混层矿物层中。选区电子衍射(SAED)和能量散射谱(EDS)测定表明形成的ZnS属于六方晶系,结晶度较低。光降解伊红_B(eosion_B)实验表明该纳米复合物具有极高的反应活性,紫外可见吸收光谱(UV_Vis)跟踪反应历程,表明降解过程中没有其他中间产物生成,20min之内降解率达到99.1%。本方法制备的ZnS柱撑高蒙混层矿物纳米复合材料与前人制备的ZnS纳米粒子相比具有更高的催化活性,方法更简单,原料较便宜,可重复利用。  相似文献   

一种基于InSAR相干系数的SAR阴影提取方法   总被引：1，自引：0，他引：1  

王健  向茂生  李绍恩 《武汉大学学报(信息科学版)》2005,30(12):1063-1066

给出了一种新的阴影提取方法,根据阴影区域在InSAR相干系数图上的特性,利用Sigma滤波和最优阈值分割算法实现阴影的自动提取。实验结果表明,本方法是一种高效的阴影提取方法。  相似文献   

CT图像存档与管理解决方案     

赵伟东  阮昌京 《CT理论与应用研究》2002,11(1):13-16

本文针对数字影像设备（如CT、MRI等）日益突出的图像存储和管理问题，进行深入的分析和研究。鉴于不同厂家和时期设备配置不同，提出了4种切实可行的解决方案：胶片扫描，视频采集，光盘或MOD输入，DICOM接口连接，完全解决了图像长期大量存储的问题。同时具有网络联机查询，图文报告，电子病历管理，激光相机接口等丰富的增值功能，是数字化医院的理想选择。  相似文献   

非规则测区三维地震偏移的边界吸收层法   总被引：7，自引：0，他引：7       下载免费PDF全文

王玉学  张关泉  周瑞芬 《地球物理学报》2002,45(5):700-706

对不规则测区的地震资料直接进行三维偏移不仅可减少计算量,而且可提高偏移剖面的质量. 本文在单程波方程中增加了一项简单的阻尼因子,其作用如同在实际不规则测区的外部有一个薄吸收层. 因为波穿越这个薄层时,波场值迅速衰减,所以偏移时把吸收层外边界处的波场值取为零所产生的反射非常微弱. 又因为不规则测区零边界条件偏移程序极易编制,所以就可以实现对不规则测区的地震资料直接进行三维偏移. 通过对实际地震资料的处理,说明了该方法的有效性.  相似文献   

用于地震调查的航空红外遥感实时传输系统研究     

乔成斌  李茂堂  张瑞青 《地震地磁观测与研究》2002,23(3):15-19

该系统提供了航空红外遥感资料的袢时采集和传输，为及时开展地震野外调查工作提供了一个有力的手段。该系统由红外传感器系统、机载站图像和数据实时处理系统、机载站通信系统、转发站通信系统、地面站接收系统、地面站图像和数据实时处理系统组成。  相似文献   

环电流区中性原子观测特性模拟研究   总被引：2，自引：1，他引：2       下载免费PDF全文

沈超  刘振兴 《地球物理学报》2003,46(1):1-1

为了给双星计划中性原子(ENA)探测仪的研制提供可靠 的理论依据，并为未来中性原子探测数据的分析及研究做好准备，针对双星轨道初步模拟计 算了双星ENA探测仪对磁暴时中性原子的观测特性. 建立了磁暴主相期间环电流离子分布的 一 个近似理论模式，并模拟计算了极轨卫星在极区上空、赤道面以及其他位置上对不同强度磁 暴主相期间环电流区ENA空间角分布及能谱的观测结果. 研究表明，存在环电流区方向和南 北极区环电流粒子沉降带两个中性原子强度极大区域；磁暴越强烈，注入区高度越低，环电 流区观测到的ENA通量越高；处于有利位置的ENA探测器可分辨注入区内边界或注入前沿；EN A探测器能够分辨环电流带离子分布的不均匀性；由于离子交换截面的差异，H，O，He 3种E NA的能谱分布不同；在10～80keV能谱范围内通量较强，易于观测；环电流区H，O两种ENA 通 量较强，有利于观测；而环电流区He ENA通量很弱，不易于观测. 模拟计算研究表明，双星 极轨卫星能够对环电流区ENA进行有效探测；低纬轨道上的ENA探测器也能够对环电流区ENA 进行一些观测；ENA探测器的研制应重视低、中能量范围ENA的探测.  相似文献