Evolution of relative helicity in active regions     

Ma  Zhenguo 《Solar physics》2002,211(1-2):189-198

The evolution dH _R/dt of relative helicity H _R provides a gauge-invariant measure of the helicity flow across the open surface S _o of an active region. With the incompressible approximation, reformulation of the evolution reveals that it is determined not only by the widely used cross-helicity h _mvp=A _pv contributed by the vector potential A _p of a reference potential field B _p, where v is the fluid velocity, but by another cross-helicity h _mvo=A _ov contributed by the vector potential A _o of the open field B _o in the region as well. Only under two conditions, (1) A _p=A (A is the transverse component of A _o), (2) v _z=0 (v _z is the longitudinal component of v) or A _z=0 (A _z is the longitudinal component of A _o), can h _mvo be merged into h _mvp to give the pioneering dH _R/dt equation shown in Equation (4) of Berger (1984). Results show that h _mvo originates from vh _o (h _o=A _oB _o is the helicity density of the open field) and should also be considered in dealing with the development of relative helicity in active regions. Finally, the equation to calculate dH _R/dt in active regions is synthesized and presented.  相似文献   

A comparison between photospheric and chromospheric quiet-Sun magnetograms     

Zhang  Mei  Zhang  Hongqi 《Solar physics》2000,194(1):19-28

Photospheric (Fei 5324.19 Å line) and chromospheric (H line) magnetic fields in quiet-Sun regions have been observed in the solar disk center by using the vector video magnetograph at Huairou Solar Observing Station of Beijing Astronomical Observatory. Observational results show that the quiet-Sun magnetic elements in the solar photosphere and chromosphere present similar magnetic structures. Photospheric and chromospheric magnetograms show corresponding time variations. This suggests that the magnetic fields in quiet-Sun regions present different 3-D magnetic configurations compared to those in solar active regions.  相似文献   

The Generating Region of Bidirectional Electron Beams in the Corona   总被引：1，自引：0，他引：1  

Xie  R.X.  Fu  Q.J.  Wang  M.  Liu  Y.Y. 《Solar physics》2000,197(2):375-385

Metric and decimetric type III bursts and microwave spike emissions with negative and positive frequency drift rates which were observed with radio spectrometers at Yunnan and Beijing Observatories are presented. The frequencies and heights at which the bidirectional electron beams originated are estimated. Three events reveal a separatrix frequency (at 250, 1300, and 2900 MHz) between normal- and reverse-drifting radio bursts, indicating a compact acceleration source where electron beams are injected in both upward and downward directions. These cases may indicate that the changeover frequencies of bidirectional electron beams are within a large band from 250 to 2900 MHz and the frequency bands of separatrices are in very small (4 to 100 MHz) and different bands. These type III bursts appear to be a plasma emission phenomenon from a beam of electrons which seem to have widely separated acceleration regions from the high to the low corona. These cases suggest that current sheets that separate open and closed magnetic fluxes in the low corona, and oppositely directed open field lines in the high corona are possible sites for bidirectional electron acceleration. The regions of magnetic topology from closed to open magnetic field structures should be very large (from about 20000 to 107000 km above the photosphere).  相似文献   

Type III burst pair     

Ning  Zongjun  Fu  Qijun  Lu  Quankang 《Solar physics》2000,194(1):137-145

We present a special solar radio burst detected on 5 January 1994 using the multi-channel (50) spectrometer (1.0–2.0 GHz) of the Beijing Astronomical Observatory (BAO). Sadly, the whole event could not be recorded since it had a broader bandwidth than the limit range of the instrument. The important part was obtained, however. The event is composed of a normal drift type III burst on the lower frequency side and a reverse drift type III burst appearing almost simultaneously on the high side. We call the burst type III a burst pair. It is a typical characteristic of two type III bursts that they are morphologically symmetric about some frequency from 1.64 GHz to 1.78 GHz on the dynamic spectra records, which indicates that there are two different electron beams from the same acceleration region travelling simultaneously in opposite directions (upward and downward). A magnetic reconnection mode is a nice interpretation of type III burst pair since the plasma beta 0.01 is much less than 1 and the beams have velocity of about 1.07×10⁸ cm s^–1 after leaving the reconnection region if we assume that the ambient magnetic field strength is about 100 G.  相似文献   

湖南省桃源县李家冲金矿主要控矿因素及找矿方向   总被引：1，自引：0，他引：1  

尤泽峰  李丰收  杨兵  甘先平 《矿产与地质》2006,20(4):374-378

李家冲金矿是近年来实施矿产资源补偿费项目时确定的具有一定找矿远景的金矿床。矿区地处扬子准地台江南地轴南缘的雪峰弧形构造隆起带的中段，距著名的大型沃溪金（锑钨）矿床南东约18km。金矿成矿主要受元古界板溪群马底驿组合矿层位及断裂构造双重因素控制，地层提供了矿源层，构造提供了矿化进一步富集的动力条件，使矿质得以活化、迁移并在有利成矿空间定位形成金矿体。在对矿床的地质特征和主要控矿因素分析的基础上，对进一步寻找金矿体的勘查方向进行了探讨，认为区内以郭家冲断裂为主的NE向断裂带是今后找金工作的重点，具体部位是近EW向层滑断裂破碎带与NE向断裂的交汇部位，并圈定出叶家坳一电厂、茶子山、文明等三处具体的勘查靶位，可作为矿区进一步工作部署的参考依据。  相似文献   

东天山大地构造演化的成矿示踪   总被引：54，自引：7，他引：54       下载免费PDF全文

王京彬王玉往  何志军 《中国地质》2006,33(3):461-469

矿床是大地构造演化的重要指示标志,矿床特征和时空分布格局为重建东天山地区大地构造演化提供了新的制约。研究表明,夹于吐哈地块和中天山地块之间的东天山古生代造山带,在空间上可分为吐哈盆地南缘铜矿带(北带)、康古尔金矿带(中带)和阿齐山—雅满苏铁(铜)-银多金属矿带(南带)3个不同的构造-地层(岩浆)-成矿带。在时间上东天山造山带具有明显的三阶段演化性:(1)吐哈盆地南缘奥陶—泥盆纪为活动大陆边缘,形成了包括VMS型铜锌矿床和斑岩型铜矿床在内的古陆缘成矿系统;晚泥盆世末—早石炭世初古洋壳向北俯冲关闭,中天山地块增生拼贴到吐哈地块(属哈萨克斯坦—准噶尔板块组成部分)南缘。(2)早石炭世(维宪期)沿康古尔缝合带再次拉张,形成石炭纪裂陷槽火山-沉积岩系及相应的层控成矿系统(VMS型铜锌矿床、火山岩型铁(铜)矿床、自然铜矿床),裂陷槽封闭过程中发育了夕卡岩型银多金属矿床。(3)早二叠世形成与幔源岩浆底侵作用有关、跨构造单元发育的铜镍硫化物成矿系统和与剪切活动有关的金矿床。依据上述认识,对东天山地区的矿产勘查提出了新建议。  相似文献   

东疆雅西371-西北坡铜金矿化带下石炭统火山岩地球化学特征与成矿背景   总被引：4，自引：2，他引：4  

方维萱  高珍权  贾润幸  黄转盈刘正桃李丰收徐国端 《岩石学报》2006,22(1):215-224

新疆东天山雅西371-西北坡铜金化带中下石炭统火山岩属钙碱性系列。流纹岩类中SiO2（73．96％～78．01％）和Al2O3（11．3％～14．63％）含量高，含Na2O为2．04％～4．15％，K2O为2．74％～3．74％，（Na2O＋K2O）为5．34％～7．03％；流纹岩类属过铝质、中钾-高钾火山岩系列。微量和稀土元素分析结果显示：流纹岩类具有Ti、Nb、P和Ta明显负异常、Sr中等负异常，LREE明显富集，La／Nb值为0．4～2．3，La／Th值0．4—1，Th／Ta值高（6～36．5），具有明显δEu（0．17-0．29）负异常，地球化学特征表明流纹岩类可能形成在活动大陆边缘上的陆缘岛弧构造背景中。本区（含矿）酸性火山岩特征对于寻找与长英质火山岩有关的金属硫化物矿床十分有利，因此认为本区具有较大找矿前景。  相似文献   

东天山卡拉塔格钠质火山岩岩石学、地球化学及成因   总被引：10，自引：10，他引：10  

唐俊华  顾连兴郑远川方同辉张遵忠高军辉王福田汪传胜张光辉 《岩石学报》2006,22(5):1150-1166

东天山卡拉塔格早泥盆世卡拉塔格组火山岩主要岩性为海相富钠质的安山岩、流纹岩和英安岩，夹少量的钠质玄武安山岩和钠质玄武岩以及正常系列的玄武安山岩。钠质火山岩的特征是：Na2O=1．69～6．38％，Na2O／K，O〉1，多在2～100间：无论是斑晶还是基质，斜长石均为富钠长石；酸性岩石斑晶主要是钠长石和石英，中基性岩石斑晶主要是钠长石（少量更长石）：酸性岩以斑状结构、霏细结构、球粒结构为主，而中基性岩以交织结构、玻晶交织结构为主。各类岩石全岩化学分析计算结果均含标准矿物Q、Hy、Hm，一部分含Di或C，在TAS图上全都投于亚碱性区；∑REE=25、96-96．11ppm，LaN／YbN=1．68-5．32，Eu／E^＊=0．46-1．25，LaN／SmN=1．01-2．95；强不相容元素适度富集，Nb和Ta强烈亏损，部分样品Cs、Rb、K、Zr和Hf适度亏损。这些特征表明，该区钠质火山岩的原始岩浆可能来自富钠俯冲洋壳熔体与地幔楔岩石反应的产物部分熔融。这样的岩浆形成机制与前人有关卡拉塔格是早泥盆世岛弧的认识相一致。  相似文献   

2004年12月26日印尼地震海啸与全球低温   总被引：6，自引：4，他引：6       下载免费PDF全文

杨冬红  杨学祥  刘财 《地球物理学进展》2006,21(3):1023-1027

气候潮汐循环说和海震调温说，阐明了冷气候、强潮汐和强震相互对应的物理机制，对2000年地球进入拉马德雷冷位相后的气候预测有重大科学意义.中国连续18年暖冬的终结是2000年地球进入拉马德雷冷位相和印尼发生地震海啸的合理结果.规律表明，在拉马德雷冷位相时期，全球强震、低温、飓风伴随拉尼娜、全球性流感伴随厄尔尼诺将越来越强烈.在20世纪50~70年代，强沙尘暴年与流感爆发年一一对应，沙尘暴可能传播禽流感。  相似文献   

A new method for spatio-temporal prediction of rainfall-induced landslide   总被引：2，自引：0，他引：2  

DING Jixin  YANG Zhifa  SHANG Yanjun  ZHOU Shenghua  YIN Juntao 《中国科学D辑(英文版)》2006,49(4):421-430

1 Introduction The landslides influences on the human society have become an environment difficult problem not able to be neglected, and according to the priority of harms, harms of landslides are only smaller than those from earthquakes in all sorts of natural hazards[1]. Landslide is part of rock mass, soil mass or their compound mass slides downward along a certain slid- ing surface under the actions of inner and external dy- namics, and it is one severe instability phenomenon of rock and s…  相似文献