大气和极移的高频变化比较

采用从1988－1999年的现代技术测定的高精度极移序列EOP（IERS97C04）推导出激发函数χ^m）和美国国家环境预测中心和美国国家大气研究中心（CNEP／NCAR）提供的大气角动量激发函数χp和χib^p，使用几种数据分析方法，分析了大气对极移高频振荡（12－42cpy)激发贡献，复数小波变换和功率谱分析表明，χ^m和χ^p序列在高频段内呈现比较强的谱峰，它们具有相似的谱特征，比较而言，χib^p在这个频率段内比χ^p要弱些，χ^m和χ^p之间的相关系数分别为0．75（逆向）和0．6（顺向），两个序列之间的平方相关谱的估计值分别在0．5－0．9之间（负频）和0．4－0．6（正频），相位谱表明χ^p(AAM)超前x^m一天左右，这些大气是极移高频变化的主要激发源，特别是在逆向运动上具有更大的贡献，由于它们之间位相差和振幅变化的不稳定性，说明可能存在AAM以外的其他激发源，这个问题有待进一步深入研究。χ     

A Statistical Study of Transequatorial Loops

We identify 356 transequatorial loops (TLs) from the data set of Yohkoh Soft X-Ray Telescope (SXT) in the period of solar cycles 22 and 23. The classification of the TLs can be made on two bases. One is according to the magnetic polarities of the footpoints of TLs, and the other is according to the number of TLs in the same region. Based on the first criterion, TLs fall into two categories: PTLs in which the magnetic polarities of the footpoints are the same as the preceding polarities and FTLs in which the footpoint polarities are the same as the following polarities of active regions, respectively. It is found that PTLs have a preference; about 66% of the TLs are PTLs, and this preference of PTLs is independent of the solar cycle. The percentage of FTLs is about 34%. Based on the second criterion, TLs are also divided into two categories: the number of TLs in a region is either single (STLs) or multiple (MTLs). In addition, we find that the number of TLs, PTLs, and FTLs have good correlations with solar cycle indices. By comparing the number of TLs and the number of active regions in each year, we obtain the ratio between them. The separation of footpoints and their yearly variations are calculated, and we find that our result is consistent with spörer's law.     

Formation of the CME Leading Edge Observed in the 2003 February 18 Event

This work investigates a typical coronal mass ejection (CME) observed on 2003 February 18, by various space and ground instruments, in white light, Ha, EUV and X-ray. The Ha and EUV images indicate that the CME started with the eruption of a long filament located near the solar northwest limb. The white light coronal images show that the CME initiated with the rarefaction of a region above the solar limb and followed by the formation of a bright arcade at the boundary of the rarefying region at height 0.46 R(?) above the solar surface. The rarefying process synchronized with the slow rising phase of the eruptive filament, and the CME leading edge was observed to form as the latter started to accelerate. The lower part of the filament brightened in Ha as the filament rose to a certain height and parts of the filament was visible in the GOES X-ray images during the rise. These brightenings imply that the filament may be heated by the magnetic reconnection below the filament in the early stage of the eruption. We suggest that a possible mechanism which leads to the formation of the CME leading edge and cavity is the magnetic reconnection which takes place below the filament after the filament has reached a certain height.     

关于CAS FGOALS-f3-L模式中青藏高原地表温度偏差的归因分析

中国科学院全球海洋-大气-陆地耦合模式(FGOALS-f3-L)参加了耦合模式比较计划的第六阶段(CMIP6)试验,但是其对关键气候敏感地区青藏高原的地表温度的再现能力还不清楚.这项研究用再分析资料CFSR评估了FGOALS-f3-L模式对青藏高原地表温度的再现能力.结果表明,FGOALS-f3-L可以合理模拟整个高原上年平均地表温度的空间分布,但低估了整个高原上年平均地表温度.模拟的地表温度在整个高原上冬春季表现为冷偏差,夏秋季表现为暖偏差.基于地表能量平衡方程的进一步定量分析表明,地表反照率反馈(SAF)项极大地贡献了高原西部年平均,冬春季平均地表温度的冷偏差,而对高原东部是暖偏差贡献.与SAF项相比,地表感热项对地表温度偏差的贡献几乎相反,这大大抵消了SAF项引起的偏差.云辐射强迫项对高原东部的年平均和季节平均弱冷偏差有很大贡献.与高估的水蒸气含量有关的长波辐射项造成了夏秋季整个高原上大部分的暖偏差.该研究表明,提高FGOALS-f3-L中的陆面和云过程对降低高原上地表温度偏差至关重要.     

华为P30手机GPS/BDS/GLONASS/Galileo观测值随机模型优化及定位性能分析

针对P30智能手机采用GPS/BDS/GLONASS/Galileo等多系统定位时的随机模型进行研究,重点对使用多系统手机观测值定位时的伪距噪声进行评估,并分析不同随机模型对手机伪距单点定位精度的影响。结果表明,华为P30智能手机不同系统卫星伪距噪声差异较大,GPS、BDS、GLONASS、Galileo的伪距噪声中误差分别为5.30 m、2.75 m、7.92 m和1.07 m。采用信噪比+系统间加权的随机模型时手机终端的定位性能最优,相比于传统高度角模型,该随机模型在E、N、U方向上的伪距单点定位精度分别提升了36.12%、25.79%、31.30%。     

Geophysical Well-Log Evaluation in the Era of Unconventional Hydrocarbon Resources: A Review on Current Status and Prospects

Surveys in Geophysics - Geophysical well-log evaluation in the era of unconventional hydrocarbon resources (mainly tight oil and gas, shale oil and gas) is complicated and challenging. This review...     

GLONASS频间码偏差特性分析及其在宽巷模糊度固定中的应用

受接收机类型、固件版本和天线的影响,GLONASS IFCB变化规律复杂且难以有效改正,导致GLONASS HMW组合包含系统性偏差,无法用于GLONASS宽巷模糊度固定。本文提出一种基于GLONASS HMW组合观测值残差的站间IFCB估计方法,并对站间IFCB变化特性进行分析。结果表明,站间IFCB长期稳定,少数相同类型硬件（包括接收机类型、固件版本和天线）站间IFCB可达0.5 m。为削弱伪距多路径效应对站间IFCB估值的影响,基于一个轨道重复周期的观测数据求得一组站间IFCB对实时观测值进行补偿,实现HMW组合平滑序列直接用于GLONASS宽巷模糊度实时固定。进行站间IFCB补偿后,基线宽巷模糊度固定正确率均在98%以上。     

Genesis of the Ore-related Granite Porphyry and Molybdenite Re-Os Age of Laomiaogou Porphyry-skarn Mo Deposit,Western Henan Province: Implications for Regional MineralizationEI北大核心CSCD

The newly discovered Laomiaogou porphyry-skarn Mo deposit is located south of the Machaoying fault in western Henan province. The ore-body is hosted in the contact between the Laomiaogou granite porphyry dyke and the Duguan Formation. LA-ICP-MS U-Pb analyses for zircons from the granite porphyry yield a weighted mean 206Pb/238U age of 152.1±0.6 Ma, and seven molybdenite separates yield a weighted mean age of 151.9±0.9 Ma and isochron age of 151.6±5.1 Ma. Thus, the granite porphyry dyke and Mo mineralization are contemporaneous. The ore-related granite porphyry dyke is a peraluminous I-type granite with high contents of SiO2 and K2O. The rocks are strongly depleted in P, Nb, Ta and Ti, indicative of intensive fractionation of apatite and Fe-Ti oxides, and characterized by low whole-rock εNd(t) (-20.6 to -17.6) and zircon εHf(t) values (-26.9 to -22.6). The old tDM2(Nd) ages (2.37 to 2.61 Ga) and zircon tDM2(Hf) ages (2.62 to 2.88 Ga) suggest that the granite porphyry was likely derived from an ancient crustal source. Considering the tectonic evolution and geochemical characteristics of the granite as well as other Mesozoic granites in the southern margin of the North China Craton, we suggest that the Laomiaogou granite porphyry dyke and Mo were most likely derived from partial melting of the Taihua Group metamorphic rocks under extensional tectonic regime related to the subduction of the paleo-pacific plate. © 2018, Science Press. All right reserved.     

乌拉特中旗284东金矿区综合信息找矿模型

284东矿区位于内蒙古乌拉特中旗北部,区内自发现金矿化以来,一直为民间开采,地质勘查无较大突破。本文通过研究以往地质资料以及野外地质踏勘,发现284东矿区以往勘查中可能存在漏矿现象,进而对已施工钻孔进行样品补取、分析,证实炭质千糜岩层为含金层位,新探获矿体走向长500m,最大斜深500m,金矿床规模达到中型。含炭千糜岩层位严格受布尔罕特敖包逆断裂（F9断裂）控制,总体沿岩体和地层接触带分布,蚀变带分带特征明显;具有高极化率,低电阻率的特征;区内金、银、铜、镍、铅丰度高、分异性强,Au、As组合高背景区呈北东向带状展布,与主控矿断裂一致,推测与含矿热液沿裂隙迁移、富集有关。通过对地质、物探、化探特征的综合分析,建立了284东金矿区综合信息找矿模型,提出地质找矿主线,为后期找矿提供思路。