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排序方式: 共有138条查询结果,搜索用时 265 毫秒
1.
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
2.
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
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
3.
青藏高原隆升与环境效应 总被引:17,自引:1,他引:17
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
4.
5.
Grey relational analysis on the relation between marine environmental factors and oxidation-reduction potential 总被引:2,自引:0,他引:2
The effects of marine environmental factors-temperature(T),dissolved oxygen(DO),salinity(S) and pH-on the oxidation-reduction potential(ORP) of natural seawater were studied in laboratory.The results show an indistinct relationship between these four factors and the ORP,but they did impact the ORP.Common mathematical methods were not applicable for describing the relationship.Therefore,a grey relational analysis(GRA) method was developed.The degrees of correlation were calculated according to GRA and the va... 相似文献
6.
清代移民屯田对新疆地名的影响 总被引:1,自引:1,他引:1
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
7.
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
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
8.
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
9.
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
10.
通过中伊双方合作交流,详细考察了伊朗的地震台网。伊朗现建有4类台网:地震遥测台网、国家地震台网、强震台网及水库诱发地震台网。这些台网中高性能宽频带地震仪数量不足,使得地震定位精度不高;且4类台网分属不同机构,在一定程度上限制了伊朗的地震监测能力。 相似文献