腾冲明光老波厂铅锌矿围岩蚀变及找矿标志

矿体产于白垩纪马头窝单元（K1^7M^λπ）石英斑岩与石炭系上统空树河组三段二层（C2k^3-3）地层的石英砂岩、长石石英砂岩接触带上,或上述两类岩石的破碎带中,矿体与围岩界线常呈波状起伏,呈突变或渐变接触。矿区围岩蚀变明显,有进一步找矿的前景。     

Height of Tracers and the Correction of the Measured Solar Synodic Rotation Rate: Demonstration of the Method

Two large stable solar filaments were used as test tracers to determine the apparent synodic rotation rate as a function of the central meridian distance for several filaments' segments at different heights. An analytic fitting procedure was applied to determine simultaneously the real synodic rotation rate and the height of the traced filament segments. The determined heights were compared with the values obtained from the widths of filament contours on the solar disk and with the values obtained by direct measurements at the solar limb. Furthermore, the obtained rotation rates and heights of the filaments' segments close to the filaments' pivot points were compared with the values obtained using two successive central meridian passages. Finally, sources and scales of errors were investigated and possible implications on the previous studies of the solar differential rotation were considered.     

The wet-dry changes in recent 40 years in taklimakan area

IINTRODUCTIONAlongwiththePetroleumexploitationofTarimBasin,consideringaboutwaterresources,peoplepaidmuchattentiontothestudyofthemodernclimatechangeinTaklimakanarea.SomePeoplehaddonemanalySeSwiththemeteorologicaldatainthearea(Yang,1992;Jietal.,1992;Zheng,1991;Xue,1989;Li,1989;Wenetal.,1988).BasedontheO~ionaldstaofprecipitationinrecent40years,thisPaperCarefullyanalyZedthewet-drychangeinrecentseveraldeCadesinTaklilnakanareaanditsneighdringareas(thenorthernXinjiang,QinghaiandGansuPro…     

基于BERT的金矿地质实体关系抽取模型研究

金矿实体关系的智能识别是提高金矿文献分析挖掘和知识提取的重要方法和途径.此次研究针对目前金矿实体关系抽取涉及到的核心问题,如金矿实体关系复杂、 人工标注信息少等特点,提出了基于BERT(Bidirectional Encoder Representations from Transformer)的远程监督关系抽取模型....     

不同去趋势方法对格尔木地区胡杨宽度年表的气候意义影响分析

基于2014年采自柴达木盆地南缘格尔木地区的胡杨树轮样本,采用三种不同去趋势方法(样条函数法、负指数拟合和区域曲线去趋势方法)建立树轮标准化序列,结合格尔木气象站气候资料,分析不同去趋势方法下胡杨径向生长对气候的响应。研究表明,利用区域去趋势方法建立的树轮年表包含有较多的气候环境信息,胡杨树轮年表与逐月气候因子相关表明,树轮年表对降水响应不显著,与生长季的平均气温和平均最高气温有较好的相关性,最高相关系数达0.411(p0.01),格尔木胡杨树轮的区域去趋势年表与组合相关的6—10月平均最高气温相关性最好,生长季的平均最高气温对胡杨径向生长有一定的限制作用并具有树木生理学意义。用区域曲线去趋势方法得出的格尔木胡杨树轮年表对气候的响应最好。     

Environmental aspect of radon potential in terra rossa and eutric cambisol in Slovenia

Terra rossa and eutric cambisol soils were surveyed in Slovenia. At both sites, 6–13 boreholes were drilled in a regular 24 m × 24 m square grid. Soil samples from various depths were taken for gamma spectrometric analysis, and radon in soil gas was measured at a depth of 80 cm using an AlphaGuard instrument. The following ranges of activity concentration (Bq kg⁻¹) were obtained for ²³⁸U, ²²⁶Ra, ²²⁸Ra, ⁴⁰K and ¹³⁷Cs: in terra rossa, 64–74, 70–84, 45–49, 293–345, 20–30 and, in eutric cambisol, 55–80, 132–147, 50–57, 473–529, 106–272. Radon activity concentrations in both soils ranged from about 100 kBq m⁻³ to 370 kBq m⁻³.     

The Jurassic Prehodavci Formation of the Julian Alps: easternmost outcrops of Rosso Ammonitico in the Southern Alps (NW Slovenia)

The Julian Alps are located in NW Slovenia and structurally belong to the Julian Nappe where the Southern Alps intersect with the Dinarides. In the Jurassic, the area was a part of the southern Tethyan continental margin and experienced extensional faulting and differential subsidence during rifting of the future margin. The Mesozoic succession in the Julian Alps is characterized by a thick pile of Upper Triassic to Lower Jurassic platform limestones of the Julian Carbonate Platform, unconformably overlain by Bajocian to Tithonian strongly condensed limestones of the Prehodavci Formation of the Julian High. The Prehodavci Formation is up to 15 m thick, consists of Rosso Ammonitico type limestone and is subdivided into three members. The Lower Member consists of a condensed red, well-bedded bioclastic limestone with Fe–Mn nodules, passing into light-grey, faintly nodular limestone. The Middle Member occurs discontinuously and consists of thin-bedded micritic limestone. The Upper Member unconformably overlies the Lower or Middle Members. It is represented by red nodular limestone, and by red-marly limestone with abundant Saccocoma sp. The Prehodavci Formation unconformably overlies the Upper Triassic to Lower Jurassic platform limestone of the Julian Carbonate Platform; the contact is marked by a very irregular unconformity. It is overlain by the upper Tithonian pelagic Biancone (Maiolica) limestone. The sedimentary evolution of the Julian High is similar to that of Trento Plateau in the west and records: (1) emergence and karstification of part of the Julian Carbonate Platform in the Pliensbachian, or alternatively drowning of the platform and development of the surface by sea-floor dissolution; (2) accelerated subsidence and drowning in the Bajocian, and onset of the condensed pelagic sedimentation (Prehodavci Formation) on the Julian High; (3) beginning of sedimentation of the Biancone limestone in the late Tithonian.     

Kinematics of Interacting ICMEs and Related Forbush Decrease: Case Study

We study heliospheric propagation and some space weather aspects of three Earth-directed interplanetary coronal mass ejections (ICMEs), successively launched from the active region AR 11158 in the period 13?–?15 February 2011. From the analysis of the ICME kinematics, morphological evolution, and in situ observations, we infer that the three ICMEs interacted on their way to Earth, arriving together at 1 AU as a single interplanetary disturbance. Detailed analysis of the in situ data reveals complex internal structure of the disturbance, where signatures of the three initially independent ICMEs could be recognized. The analysis also reveals compression and heating of the middle ICME, as well as ongoing magnetic reconnection between the leading and the middle ICME. We present evidence showing that the propagation of these two, initially slower ICMEs, was boosted by the fastest, third ICME. Finally, we employ the ground-based cosmic ray observations, to show that this complex disturbance produced a single cosmic ray event, i.e., a simple Forbush decrease (FD). The results presented provide a better understanding of the ICME interactions and reveal effects that should be taken into account in forecasting of the arrival of such compound structures.     

Validity of the Relations Between the Synodic and Sidereal Rotation Velocities of the Sun

Existing methods for conversion between synodic and sidereal rotation velocities of the Sun are tested for validity using state-of-the-art ephemeris data. We found that some of them agree well with ephemeris calculations while others show a discrepancy of almost 0.01^° day^?1. This discrepancy is attributed to a missing factor and a new corrected relation is given.