云南雨季开始期演变特征分析   总被引：10，自引：0，他引：10  

陶云  郑建萌  万云霞  刘瑜 《气候与环境研究》2006,11(2):229-235

应用EOF分析方法、小波分析方法及云南16个地州代表站1961～2002年共42年逐日降水量资料,对云南雨季开始期的空间分布、时间演变及多尺度周期变化等特征进行了诊断研究.结果表明:1)云南雨季开始期的空间分布,第一主要特征是全省雨季开始期一致偏早(晚);第二主要特征为云南滇中及以东、以南地区与云南西部雨季开始期反向变化的空间异常分布型态;2)云南雨季开始期存在明显的40年左右长周期、28年左右的年代际周期和8年左右的年际周期.从小波方差看,云南雨季开始期的变化以40年和28年左右的变化周期的振动最强,变化最显著,而年际变化相对较弱;3)云南雨季开始偏早期与偏晚期5月份500 hPa高度距平场有着明显区别;4)印度季风与南海季风对云南雨季开始爆发也起着积极的作用.  相似文献   

贵州雪峰至加里东旋回构造演化与区域成矿规律          下载免费PDF全文

陶平  陈建书  白培荣 《贵州地质》2023,40(4):344-352, 361

以《中国矿产地质志·贵州卷》研究项目为依托,在前人研究基础上,进行了贵州雪峰至加里东构造旋回构造演化及区域成矿规律的系统研究。认为在该构造旋回,随着构造动力从离散(裂解)向汇聚(造山)发展,盆地类型从陆内裂陷(谷)盆地转化为被动大陆边缘盆地,再转化为板内结合带压陷盆地,从而形成了各时期特有的地质建造及多种矿产,尤其是贵州最有特色的锰、磷、重晶石等沉积矿产。这些矿产在各种地质建造及其地质体中呈现出有序分布规律。在此基础上,建立并论述了与沉积作用、浅成中-低温热液作用、岩浆作用有关的矿床成矿系列各一个及亚系列数个,并建立了贵州与南华纪至中寒武纪早期主要矿产的区域成矿模式。这些成果进一步揭示了贵州该旋回中的区域成矿规律。  相似文献   

Observational Study of a Peculiar Solar Limb Event Occurred on 11 January 2002     

Hui Li  Jianqi You 《Solar physics》2009,258(1):89-104

On 11 January 2002, using the Multi-channel Infrared Solar Spectrograph (MISS) at the Purple Mountain Observatory (PMO), we obtained Hα, Ca ii 8542 Å and He i 10?830 Å spectra and slit-jaw Hα images of a peculiar solar limb event. A close resemblance of its intensity to that of a small flare and the GOES X-ray flux indicates that it was an active prominence. However, its morphological evolution and velocity variation were different from general typical active prominences, such as limb flares, post-flare loops, surges and sprays. It started with the ejection of material from the flare site. In the early phase, the ejecta was as bright as a limb flare and kept rising until reaching the height of (8????10)×10⁴ km at an almost constant velocity of 91.7 km? s ^?1 with its lower part always connected to the solar surface. EUV images in 195 Å show similar structure as in the Hα line, indicating the coexistence of plasmas with temperatures differing by more than two orders of magnitude. Later some material started to fall back to another bright area on the solar surface. The falling material did not show the collimated structure of surges or the arc structure of flaring arches. A red-shift velocity of more than 200 km? s ^?1 was detected in a bright point close to the outer edge of the closed loop system formed later, which dispersed in a few minutes and became a part of the newly formed large loop. The ejected material did not leave the sun, indicating that the magnetic reconnection was not sufficient to remove the overlying field lines during the process. The spectral line profiles showed large widths and variable velocities, and therefore the line-pair method is not applicable to this event for the estimation of physical parameters.  相似文献   

利用窄线宽激光测量锶原子束速率分布     

赵亚楠  吴慧  常宏  张首刚 《时间频率学报》2009,32(1):1-5

利用多普勒频移效应,通过线宽2MHz窄线宽激光与锶原子束在大角度作用下的荧光信号分析,测量了锶原子束速率分布。比较和分析表明,理论结果与实验结果符合较好。  相似文献   

Flare-induced signals in polarization measurements during the X2.6 flare on 2005 January 15     

Meng Zhao  Jing-Xiu Wang  Sarah Matthews  Ming-De Ding  Hui Zhao  Chun-Lan Jin 《中国天文和天体物理学报》2009,9(7)

Flare-induced signals in polarization measurements which were manifested as apparent polarity reversal in magnetograms have been reported since 1981. We are motivated to further quantify the phenomenon by asking two questions: can we distinguish the flare-induced signals from real magnetic changes during flares, and what we can learn about flare energy release from the flare-induced signals? We select the X2.6 flare that occurred on 2005 January 15, for further study. The flare took place in NOAA active re-gion (AR) 10720 at approximately the central meridian, which makes the interpretation of the vector magnetograms less ambiguous. We have identified that flare-induced signals during this flare appeared in six zones. The zones are located within an average distance of 5 Mm from their weight center to the main magnetic neutral line, have an average size of (0.6±0.4)×1017 cm2, duration of 13±4 min, and flux density change of 181±125 G in the area of reversed polarity. The following new facts have been revealed by this study: (1) the flare-induced signal is also seen in the transverse magnetograms but with smaller magnitude, e.g., about 50 G; (2) the flare-induced signal mainly manifests itself as apparent polarity reversal, but the signal starts and ends as a weakening of flux density; (3) The flare-induced signals appear in phase with the peaks of hard X-ray emission as observed by the Ramaty High Energy Solar Spectroscopic lmager (RHESSI), and mostly trace the position of RHESSI hard X-ray footpoint sources. (4) in four zones, it takes place cotemporally with real magnetic changes which persist after the flare. Only for the other two zones does the flux density recover to the pre-flare level immediately after the flare.The physical implications of the flare-induced signal are discussed in view of its relevance to the non-thermal electron precipitation and primary energy release in the flare.  相似文献   

基于Oracle多分辨率遥感影像数据库的设计     

陶治宇  马东洋  徐青  解志刚 《测绘科学技术学报》2005,22(1):65-68

简要介绍了Oracle提供的Oracle Spatial和Oracle interMedia 两个选件的特性,详细阐述了基于对象-关系模型的多分辨率遥感影像数据的组织和管理,并设计和建立了多分辨率遥感影像数据库的原型,采用了地形瓦片和影像金字塔的快速索引结构.实验表明该设计正确有效,能够平稳快速地实现多分辨率遥感影像的快调度显示.  相似文献   

Pressure dependence of viscosity of rhyolitic melts     

Hejiu Hui  Youxue Zhang  Piero Del Gaudio  Harald Behrens 《Geochimica et cosmochimica acta》2009,73(12):3680-3693

Viscosity of silicate melts is a critical property for understanding volcanic and igneous processes in the Earth. We investigate the pressure effect on the viscosity of rhyolitic melts using two methods: indirect viscosity inference from hydrous species reaction in melts using a piston cylinder at pressures up to 2.8 GPa and direct viscosity measurement by parallel-plate creep viscometer in an internally-heated pressure vessel at pressures up to 0.4 GPa. Comparison of viscosities of a rhyolitic melt with 0.8 wt% water at 0.4 GPa shows that both methods give consistent results. In the indirect method, viscosities of hydrous rhyolitic melts were inferred based on the kinetics of hydrous species reaction in the melt upon cooling (i.e., the equivalence of rheologically defined glass transition temperature and chemically defined apparent equilibrium temperature). The cooling experiments were carried out in a piston-cylinder apparatus using hydrous rhyolitic samples with 0.8-4 wt% water. Cooling rates of the kinetic experiments varied from 0.1 K/s to 100 K/s; hence the range of viscosity inferred from this method covers 3 orders of magnitude. The data from this method show that viscosity increases with increasing pressure from 1 GPa to 3 GPa for hydrous rhyolitic melts with water content ?0.8 wt% in the high viscosity range. We also measured viscosity of rhyolitic melt with 0.13 wt% water using the parallel-plate viscometer at pressures 0.2 and 0.4 GPa in an internally-heated pressure vessel. The data show that viscosity of rhyolitic melt with 0.13 wt% water decreases with increasing pressure. Combining our new data with literature data, we develop a viscosity model of rhyolitic melts as a function of temperature, pressure and water content.  相似文献   

Distinguishing gases derived from oil cracking and kerogen maturation: Insights from laboratory pyrolysis experiments     

Guo Liguo  Xiao Xianming  Tian Hui  Song Zhiguang 《Organic Geochemistry》2009,40(10):1074-1084

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内蒙古苏尼特左旗乌兰德勒钼铜多金属矿床辉钼矿铼-锇同位素定年及其地质特征   总被引：14，自引：0，他引：14  

陶继雄  王弢  陈郑辉  罗忠泽  许立权  郝先义  崔来旺 《岩矿测试》2009,28(3):249-253

中蒙边境内蒙古苏尼特左旗乌兰德勒钼铜多金属矿床是内蒙古二连—东乌旗成矿带上近几年国土资源地质大调查工作过程中新发现的一个规模较大的矿床,包括赋存于上部细粒石英闪长岩、中粗粒花岗闪长岩中细脉浸染状矿体和赋存于隐伏的细粒二长花岗岩中的浸染状矿体,属典型的斑岩型钼矿床。文章通过采集WZK1钻孔211.2～214m细脉浸染状矿石的辉钼矿纯样,获得辉钼矿的等时线年龄为(134.1±3.3)Ma,并对比了矿区细粒二长花岗岩的锆石SHRIMP年龄(131.4±1.6)Ma,两者基本一致,表明矿床的形成主要与隐伏的燕山期细粒二长花岗岩有着密切关系。测定的辉钼矿铼-锇同位素年龄能够精确代表该矿床的成矿时间,表明在乌兰德勒区域找矿工作中,需要密切关注燕山期构造-岩浆活动的相关成矿作用。  相似文献   

超声提取-固相萃取小柱净化-气相色谱法测定土壤中14种有机氯农药   总被引：7，自引：7，他引：0  

刘文长  陶文靖  程丽娅  余兴  田旻  黄勤  李胜生 《岩矿测试》2009,28(6):541-544

对土壤中14种有机氯农药的超声提取技术和磺化、固相萃取小柱两种净化方法进行系统研究。结果表明,超声提取节省提取时间,提高分析效率;磺化法和固相萃取小柱法都有净化作用,但磺化法使样品中的艾氏剂、狄氏剂和异狄氏剂全部损失;固相萃取小柱净化当丙酮-正己烷淋洗液体积比为1∶9、淋洗液收集8 mL时回收率>90%,干扰最小。方法检出限为0.63~2.59μg/kg,精密度(RSD,n=7)为1.17%~14.66%,基体加标平均回收率为82.78%~106.94%。方法用于生态地球化学调查评价批量土壤样品的实际分析,检测结果满足评价工作需要。  相似文献