Three Super Active Regions in the Descending Phase of Solar Cycle 23   总被引：2，自引：0，他引：2  

Hong-Qi Zhang  Xing-Ming Bao  Yin Zhang  Ji-Hong Liu  Shu-Dong Bao  Yuan-Yong Deng  Wei Li  Jie Chen  Jin-Ping Dun  Jiang-Tao Su  Juan Guo  Xiao-Fan Wang  Ke-Liang Hu  Gang-Hua Lin  Dong-Guang WangNational Astronomical Observatories  Chinese Academy of Sciences  Beijing   《中国天文和天体物理学报》2003,3(6):491-494

We analyze the magnetic configurations of three super active regions, NOAA 10484, 10486 and 10488, observed by the Huairou Multi-Channel Solar Telescope (MCST) from 2003 October 18 to November 4. Many energetic phenomena, such as flares (including a X-28 flare) and coronal mass ejections (CMEs), occurred during this period. We think that strong shear and fast emergence of magnetic flux are the main causes of these events. The question is also of great interest why these dramatic eruptions occurred so close together in the descending phase of the solar cycle.  相似文献   

Multi-cloud model (MCM) method and its applications to the study on asymmetric spectral profiles   总被引：1，自引：0，他引：1  

Xiao-Ma Gu  Jun Lin  Ke-Jun Li  Jing-Ping Dun 《Astrophysics and Space Science》1996,240(2):263-271

A method of multi-cloud model (MCM) is proposed in this paper in order to research asymmetric profiles of spectral line formed by solar discrete active objects aligned along the line-of-sight difection. Based on the MCM method, under the conditions of certain assumptions and approximations, the line-of-sight velocityV and three other physical parameter approximation values, (i.e. Doppler width _D , source functionS and optical depth at line center ₀) within different clouds may be derived simultaneously by fitting both profiles theoretical and observational. An application example of the method withm=3 shows that MCM method is suitable to measure the velocity fields of multi-object at the same time from their non-Gaussian profiles of complex. TheV and _D derived from the method are reliable,S and ₀ are approximation. An influence of the variations of initial values in the parameter on the solution is given as well.  相似文献   

青藏高原隆升与环境效应   总被引：17，自引：1，他引：17  

黎敦朋  肖爱芳  李新林  周小康 《陕西地质》2004,22(1):1-10

通过对青藏高原北缘库木库里盆地新生代沉积建造、孢粉、阶地热年龄、沉积响应的调查研究，得出青藏高原新生代的渐新世、上新世和更新世一全新世形成的三套磨拉石建造代表青藏高原最强烈的三次隆升作用；自渐新世以来到上新世晚期高原隆升幅度达1500～2000m，更新世、全新世高原隆升了约2500m，46．4Ka．Bp至今高原隆升了约44m；青藏高原的隆升速率由渐新世开始有愈来愈强烈的趋势，预示青藏高原的隆升是一个多阶段、不等速和非均变的复杂过程；根据库木库里盆地沉积演化揭示青藏高原的隆升经历了早中渐新世早期隆升期、晚渐新世——早中新世早期稳定剥蚀夷平期、早中新世中晚期小幅隆升期、中中新世较稳定剥蚀夷平期、晚中新世振荡隆升期、上新世快速隆升期、更新世一全新世强烈隆升期共七个隆升阶段；并探讨了高原隆升引起的气候干燥、生物灭绝、荒漠化等多种环境效应。  相似文献   

Editorial     

Natascha Klocker  Olivia Dun 《The Australian geographer》2016,47(4):373-376

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海面大气和海洋条件变化引起的太阳辐照度高频变化分析     

赵进平  王维波  矫玉田 《中国海洋大学学报(自然科学版)》2010,40(4)

海洋光学考察时需要同步测量大气中的下行太阳辐照度,其测量采样频率比常规大气辐射观测高300倍,可记录到达海面太阳辐射的高频变化。利用2007年在白令海考察的数据,详细研究了辐照度高频变化的特征与原因,得出影响辐照度记录的主要因素有云层、海雾和海浪。结果表明,这3种因素的影响有明显的差别,使作者有可能在不确切知道现场情况的条件下,由数据本身判断辐照度变化的原因,并获取有关的参数。云层引起的辐照度变化具有低频率、大振幅的特征。海雾引起的辐照度变化最为复杂,变化幅度大,变化周期复杂,从几秒到上百秒,与云层效应相区别。晴空条件下,海浪调制的反射信号通过空气中的水汽散射影响辐照度计测量数值,形成周期短、振幅小的稳定振动信号,与云和雾的效应有明显区别。文中提供了云、雾和浪对辐照度影响的定性特征和定量分析结果,对理解海面辐照度记录,并正确处理数据有指导意义。  相似文献   

清代移民屯田对新疆地名的影响   总被引：1，自引：1，他引：1  

董琳 《干旱区地理》1993,16(4):63-68

本文从移民地名、屯田地名、方位地名、方言地名等方面，论述了清代移民屯田对新疆的地名的影响。  相似文献   

Fuzzy random vibration of multi-degree-of-freedom hysteretic systems subjected to earthquakes     

Guang-Yuan Wang  Jin-Ping Ou 《地震工程与结构动力学》1987,15(5):539-548

Earthquake excitation not only has evident randomness but also has strong fuzziness owing to the uncertainties in the definition of earthquake intensity and site soil classification. In this paper, the seismic ground motion is simulated as a stationary filtered white noise with fuzzy parameters, an analytical procedure is proposed to analyse the fuzzy random vibration of multi-degree-of-freedom (MDOF) hysteretic systems, and the covariance matrix of the fuzzy random responses is derived by the equivalent linearization technique. Finally, some numerical results for a two-storey shear hysteretic frame are presented to demonstrate the validity and effectiveness of the procedure proposed.  相似文献   

新疆库木库里盆地铜矿地质特征及找矿前景   总被引：3，自引：1，他引：3  

肖爱芳  黎敦朋  李新林  周小康  杜少喜 《陕西地质》2002,20(2):50-58

新疆库木库里盆地砂砾岩型铜矿带位于东昆仑成矿带西段东昆中断裂北侧新生代陆相盆地中 ,与西部且末县嘎其哥洛德和克孜勒小型砂砾岩型铜矿组成近2 0 0km长的大型砂砾岩型铜矿化带。铜矿化赋存于石马沟组上段 (E3 S1)砂岩中。围岩中铜含量一般低于地壳丰度值 ,南部火箭山地区发现有斑岩型铜矿化、昆中结合带也发现规模巨大的铜矿化带 ,它们可能是本区铜矿化的矿源层。铜矿化呈透镜状、似层状 ,剖面上已发现三层铜矿化 ,其中上部铜矿化较好。地表氧化矿石矿物组合简单 ;矿石构造为条带状、浸染状、团块状 ,填隙结构。铜矿化受湖泊三角洲相、三角洲前缘亚相的近岸砂坝、远岸砂坝的砂体控制。  相似文献   

1989年8月17日耀斑后环系速度场分析     

顾啸马  郭金平 《紫金山天文台台刊》1999,18(2):128-130

本文给出了１９８９ 年８ 月１７ 日耀斑后环的观测视向速度场,在环内物质在太阳重力、磁场梯度和大气压力梯度联合作用下沿环腿螺旋上升和环内物质密度由环腿向环顶和环足线性递增的假设下,理论上计算了该环系的视向速度场,理论计算和观测结果基本相符,似乎为耀斑物质由色球蒸发作上升运动的观点提供了间接的例证  相似文献   

The X10 Flare on 29 October 2003: Was It Triggered by Magnetic Reconnection between Counter-Helical Fluxes?     

Yu Liu  Hiroki Kurokawa  Chang Liu  David H. Brooks  Jingping Dun  Takako T. Ishii  Hongqi Zhang 《Solar physics》2007,240(2):253-262

Vector magnetograms taken at Huairou Solar Observing Station (HSOS) and Mees Solar Observatory (MSO) reveal that the super active region (AR) NOAA 10486 was a complex region containing current helicity flux of opposite signs. The main positive sunspots were dominated by negative helicity fields, while positive helicity patches persisted both inside and around the main positive sunspots. Based on a comparison of two days of deduced current helicity density, pronounced changes associated with the occurrence of an X10 flare that peaked at 20:49 UT on 29 October 2003 were noticed. The average current helicity density (negative) of the main sunspots decreased significantly by about 50%. Accordingly, the helicity densities of counter-helical patches (positive) were also found to decay by the same proportion or more. In addition, two hard X-ray (HXR) “footpoints” were observed by the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) during the flare in the 50 – 100 keV energy range. The cores of these two HXR footpoints were adjacent to the positions of two patches with positive current helicity that disappeared after the flare. This strongly suggested that the X10 flare on 29 October 2003 resulted from reconnection between magnetic flux tubes having opposite current helicity. Finally, the global decrease of current helicity in AR 10486 by ∼50% can be understood as the helicity launched away by the halo coronal mass ejection (CME) associated with the X10 flare. Electronic Supplementary Material The online version of this article () contains supplementary material, which is available to authorized users.  相似文献