Formation of Transient Coronal Holes during the Eruption of a Quiescent Filament and its Overlying Sigmoid     

Li-Heng Yang  Yun-Chun Jiang  Dong-Bai Ren 《中国天文和天体物理学报》2008,8(3):329-336

By using Hα, He I 10830, EUV and soft X-ray (SXR) data, we examined a filament eruption that occurred on a quiet-sun region near the center of the solar disk on 2006 January 12, which disturbed a sigmoid overlying the filament channel observed by the GOES-12 SXR Imager (SXI), and led to the eruption of the sigmoid. The event was associated with a partial halo coronal mass ejection (CME) observed by the Large Angle and Spectrometric Coronagraphs (LASCO) on board the Solar and Heliospheric Observatory (SOHO), and resulted in the formation of two flare-like ribbons, post-eruption coronal loops, and two transient coronal holes (TCHs), but there were no significantly recorded GOES or Hα flares corresponding to the eruption. The two TCHs were dominated by opposite magnetic polarities and were located on the two ends of the eruptive sigmoid. They showed similar locations and shapes in He Ⅰ 10830, EUV and SXR observations. During the early eruption phase, brightenings first appeared on the locations of the two subsequent TCHs, which could be clearly identified on He Ⅰ 10830, EUV and SXR images. This eruption could be explained by the magnetic flux rope model, and the two TCHs were likely to be the feet of the flux rope.  相似文献   

Relationship between pulse width and energy in GRB 060124: from X-ray to γ-ray bands     

Fu-Wen Zhang  Yi-Ping Qin   《New Astronomy》2008,13(7):485-490

GRB 060124 is the first event that both prompt and afterglow emission were observed simultaneously by the three Swift instruments. Its main peak also triggered Konus-Wind and HETE-II. Therefore, investigation on both the temporal and spectral properties of the prompt emission can be extended to X-ray bands. We perform a detailed analysis on the two well identified pulses of this burst, and find that the pulses are narrower at higher energies, and both X-rays and γ-rays follow the same w–E relation for an individual pulse. However, there is no a universal power-law index of the w–E relation among pulses. We find also that the rise-to-decay ratio r/d seems not to evolve with E and the r/d values are well consistent with that observed in typical GRBs. The broadband spectral energy distribution also suggests that the X-rays are consistent with the spectral behavior of the γ-rays. These results indicate that the X-ray emission tracks the γ-ray emission and the emissions in the two energy bands are likely to be originated from the same physical mechanism.  相似文献   

顾及大气角动量的Prophet-VAR日长变化预报方法     

钱炜  岳建平  单丽杰  韩宸宇 《大地测量与地球动力学》2022,42(3):264-268

针对日长变化参数序列中蕴含的复杂非线性特征会严重影响其预报精度的问题,同时为探讨引入大气角动量序列是否有助于提升预报精度,提出一种Prophet拟合外推联合向量自回归(vector autoregression,VAR)残差补偿的组合模型用于日长预报.选用2008～2020年的日长变化参数序列进行实验,同时设计不顾及大...  相似文献   

粤东塘唇石英脉型钨(锡)矿床地质特征、成矿时代及其找矿意义          下载免费PDF全文

卢友月  付建明  张国培  郑宗皓  李楠  程顺波  秦拯纬  马丽艳 《地球科学》2019,44(2):387-398

塘唇钨(锡)矿是近年来新发现的一个具有大型规模找矿潜力的石英脉型矿床.矿床产于粤东龙窝花岗闪长岩岩体西部外接触带,赋矿地层为下侏罗统金鸡组碎屑岩,该层位是南岭及邻区石英脉型钨锡矿的最新赋矿地层.在详细的野外地质调查基础上,对矿床含钨石英脉中的白云母进行⁴⁰Ar-³⁹Ar测年,获得白云母⁴⁰Ar-³⁹Ar坪年龄为150±1 Ma,等时线年龄为149±2 Ma(MSWD=1.20),它们在误差范围内一致,为南岭地区燕山早期大规模成岩成矿作用高峰期的产物.塘唇钨(锡)矿的发现,不仅拓宽了石英脉型钨锡矿的找矿视野,还有助于完善石英脉型钨锡矿成矿规律和成矿模式,对区域下一步找矿具有重要指导意义.  相似文献   

沙漠微生物矿化覆膜及其稳定性的现场试验研究   总被引：2，自引：0，他引：2  

李驰  王硕  王燕星  高瑜  斯日古楞 《岩土力学》2019,40(4):1291-1298

将微生物诱导矿化技术应用于原位沙漠覆膜的形成,使得流动沙丘经结皮固定而成为半固定、固定沙丘,从根本上阻断沙尘暴的源头。在内蒙古乌兰布和沙漠腹地选择两个微生物矿化试验区域（TP1和TP3）,分别用于两种不同矿化菌种诱导生成碳酸钙覆膜。研究沙漠微生物矿化覆膜的现场试验方法及工艺,对原位矿化覆膜的强度及其在沙漠环境中的长期稳定性进行跟踪检测。采用沙漠土中自行提取的葡萄球菌和传统的巴氏芽孢杆菌两种不同的微生物矿化菌种,通过现场贯入试验检测7、14、28、60、210 d后矿化覆膜沿深度发展的贯入阻力,并将覆膜厚度为2 cm处的平均贯入阻力换算成覆膜层强度,总结覆膜强度随时间的发展变化规律。现场观测结果显示,不同微生物菌种诱导生成的矿化覆膜均在试验的第4天开始形成,到第7天覆膜层具有稳定的强度和厚度,现场检测覆膜的平均厚度为2.0～2.5 cm,经自源葡萄球菌诱导生成的矿化覆膜（TP1）的强度是巴氏芽孢杆菌诱导生成的矿化覆膜（TP3）强度的1.05倍。当经历冬春交替后覆膜层强度都有不同程度的降低,明显地TP3较TP1区域表面剥落更为严重,第210天检测TP3的平均厚度为0.7～1.0 cm,覆膜强度较第7天时降低19%,覆膜内碳酸钙含量较第7天检测时降低15%～30%。而TP1在第210天时的强度较第7天时强度降低仅2%。因此,微生物诱导矿化技术可以应用于沙漠原位覆膜的形成,且沙漠自源葡萄球菌经诱导生成的矿化覆膜层具有更好的强度表现和稳定性。  相似文献   

西藏泥盆纪海相红层的分布与时代   总被引：1，自引：0，他引：1  

林宝玉  李明  武振杰 《地质学报》2019,93(10):2383-2402

在作者及前人对西藏地区泥盆纪地层学、古生物学等资料研究的基础上,作者对该区泥盆纪海相红层进行了初步的系统整理。共识别出6层(套)海相红层,它们是:早泥盆世扎西岗组海相红层(洛赫柯夫阶—布拉格阶)(XDRB1)和春节桥组上部海相红层(埃姆斯阶)(XDRB2),中泥盆世海通组海相红层(艾费尔阶)(XDRB3)和丁宗隆组底部海相红层(吉维阶)(XDRB4),晚泥盆世查果罗玛组(下部)海相红层(弗拉斯阶)(XDRB5)和羌格组顶部海相红层(法门阶)(XDRB6)。所有海相红层均形成于近岸或浅水碳酸盐岩台地环境,因此,属于浅水-半深水陆棚红层,此外,还讨论了中国南方泥盆纪海相红层的分布及全球法门期海相红层广布事件。  相似文献   

新疆东天山小白石头钨(钼)矿辉钼矿Re-Os同位素年龄及成矿时代   总被引：1，自引：0，他引：1  

李宁  杨富全  李超  张志欣  杨成栋 《岩矿测试》2019,38(1):112-122

小白石头钨(钼)矿床位于新疆东天山造山带中的中天山地块南缘,该矿床是一个由黑云母花岗岩和花岗闪长岩侵入中元古界卡瓦布拉格群形成的矽卡岩型钨(钼)矿床。辉钼矿作为其主要的矿石矿物之一,呈不同产出状态分布于花岗闪长岩、黑云母花岗岩、矽卡岩和石英脉中。目前,对于小白石头钨(钼)矿成矿时代尚有争议,特别是与花岗闪长岩有关的辉钼矿化形成时代缺乏精确的限定。本文选取与花岗闪长岩有关的不同产状辉钼矿进行Re-Os同位素定年,获得Re-Os加权平均模式年龄为245. 0±1. 7Ma,Re-Os等时线年龄为245. 5±4. 3Ma。准确的Re-Os同位素定年限定小白石头钨(钼)矿床的成矿年龄和花岗闪长岩的侵位年龄为245Ma左右,为矿床模型建立和找矿方向确定提供了关键依据,同时也为东天山区域成矿规律总结提供了重要的年代学证据,并指出新疆东天山—甘肃北山地区存在一条找矿潜力巨大的三叠纪钨钼成矿带。  相似文献   

河北洞子沟银铜多金属矿床地质特征及成因分析          下载免费PDF全文

王银川 《地质找矿论丛》2019,34(2):163-170

洞子沟银铜多金属矿床产于华北克拉通北缘长城系常州沟组地层中,受地层控制明显。通过对该矿床地质特征及矿石的稀土元素地球化学特征、矿物流体包裹体特征、硫氢氧同位素组成及U-Pb同位素年代研究表明:成矿物质来源于幔源;矿床形成于古元古代晚期华北克拉通吕梁运动后的伸展裂解过程中,在断陷盆地接受沉积的同时,有沿同生断裂上升的幔源热液、银铜金铅锌等成矿物质组分与常州沟组陆源碎屑一同沉积,形成洞子沟银铜多金属沉积层控型矿床。  相似文献   

扬子地台西南缘朱家坝辉绿岩地球化学特征及其地质意义     

杨斌  金灿海  郭阳  王子正  董国臣 《矿物岩石》2019,39(1):43-51

近年来在扬子西缘大量的早—中元古代岩浆岩证据显示扬子地台内形成的断陷盆地及早中元古代岩浆岩与全球性的Columbia超大陆裂解事件有着密不可分的联系。这种联系主要表现在区内早中元古代的岩浆岩地球化学特征上。为了探讨武定裂陷槽朱家坝辉绿岩的地球化学特征及其意义,以12块朱家坝辉绿岩的地球化学分析数据为基础,在分析了其主微量和稀土元素的特征之后发现朱家坝辉绿岩w(SiO_2)为44.16%～48.08%,w(K_2O+Na_2O)为3.54%～4.26%,在化学成分上属于钙碱性岩石;其稀土元素的总量为183.1×10^-6～206.91×10^-6,LREE/HREE=1.44～1.96,表明在其形成过程中发生了明显的地壳混然或者是岩浆分异作用,其化学成分基本可以反映出岩浆源区的化学组成特征。基于此,对朱家坝辉绿岩进行了源区性质、构造环境和可能的成因机制探讨,认为朱家坝辉绿岩形成于拉张环境之中,很有可能是在昆阳裂谷形成初期形成,其岩浆来源于较富集的地幔源区,形成过程中几乎没有地壳物质参与。  相似文献   

Atmospheric Reactive Nitrogen Cycle and Stable Nitrogen Isotope Processes: Progresses and Perspectives   总被引：1，自引：1，他引：0  

Tao Zhou  Zhuang Jiang  Lei Geng 《地球科学进展》2019,34(9):922-935

Oxidized reactive nitrogen in the atmosphere mainly consists of nitrogen oxides (NO _X =NO+NO₂, NO₃) and nitric acid. The atmospheric cycling of NO _X influences the formation of ozone and hydroxyl radicals that are important for atmospheric oxidation capacity. Nitric acid, the final product of NO _X oxidation, not only is an important component of particulate pollutants, but also has a direct impact on the ecosystem through dry and wet deposition. The stable nitrogen isotope (δ¹⁵N) shows the potential to study reactive nitrogen cycle, and to trace the emission, transport and deposition of reactive nitrogen from local to global scales. Here, we reviewed previous studies using δ¹⁵N to investigate NO _X emission and atmospheric reactive nitrogen cycle, and discuss the uncertainties of δ¹⁵N signatures of different NO _X sources from two aspects: NO _X generation mechanism and NO _X collection methods. We also discussed the nitrogen isotope fractionation and the consequences during the conversions of NO _y molecules. We ended up with discussions on the possibility of using δ¹⁵N to trace NO _X emissions. Although there are still large uncertainties in quantifying and tracing NO _X emissions using nitrogen stable isotopes, such isotope tool is efficient enough to trace reactive nitrogen cycles in the atmosphere. On the basis of this, we proposed that we can combine atmospheric chemistry transmission models with isotope tracers to improve our understanding of regional and global atmospheric reactive nitrogen cycle regarding the fluxes of different emission sources, their atmospheric transformation, etc.  相似文献