2022年《中国学术期刊影响因子年报》发布——《地球学报》复合影响因子2.578

<正>由《中国学术期刊(光盘版)》电子杂志社有限公司、中国科学文献计量评价研究中心和清华大学图书馆出版的《中国学术期刊影响因子年报(自然科学与工程技术)(2022年版)》(简称《年报》)已发布。根据《年报》的统计结果,在105种地质类期刊中,《地球学报》2022年影响力指数为377.707,排名第21,复合影响因子是2.578,分区为Q1(表1)。《年报》采用的统计分析方法体现了如下8个特点:     

分支河流体系河网形态演变规律——以格尔木河流扇为例

为了探索分支河流体系河网分布规律,为创建储层建模训练图像提供知识库信息。利用Google Earth、Global Mapper、91卫图助手等现代地理信息软件,系统测量了现代格尔木河流扇表面河道分叉特征,应用Horton定律和分形方法建立了河流扇的河网形态模型。结果表明：①格尔木河流扇从顶点到入湖段共识别出26级河道,882个节点和2162个河道段,泉线上、下的河道表现出不同的河网形态;②泉线上部共发育64个节点,每级河道数目增长是上一级河道的RB=1.8900倍,每级河道平均长度是下一级河道的RL=1.0095倍,即河网形态特征参数RB=1.8900和RL=1.0095;泉线下部共发育818个节点,每级河道数目增长是上一级河道的RB=1.0279倍,每级河道平均长度是下一级河道的RL=0.9899倍,即河网形态特征参数是RB=1.0279和RL=0.9899;③河网形态特征参数受坡度影响变化较大,坡度较大则河网形态特征参数较大,坡度较小则河网形态特征参数较小。河网形态特征参数定量表征促进了分支河流体系沉积学发展,为开展陆相盆地储层建模和砂体预测提供了新的知识库信息     

坝上草原相关花粉源范围与相对花粉产量估算

基于坝上草原地区30个采样点表土花粉分析和植被调查的研究结果显示,花粉组合以蒿属、藜科、禾本科、菊科和莎草科等草本植物为主,基本能够反映草原植被特征,但花粉百分比与其在植被中盖度差异明显.运用Extended R-Value(ERV)模型估算的坝上草原区相关花粉源范围大致为2100m,当风速大于3.5m/s时,基本稳定,受风速影响不大.估算的相对花粉产量结果显示,蒿属和藜科的相对花粉产量最高,为禾本科的20倍左右;其次为莎草科和菊科,为禾本科的7～9倍;百合科略高于禾本科;旋花科、豆科、唇形科及委陵菜属的相对花粉产量则明显低于禾本科.利用相对花粉产量对花粉与植被关系的校正结果表明:蒿属、藜科的校正效果明显,其相对花粉产量可以作为定量重建古植被的参考;莎草科、菊科、百合科和唇形科由于受植被和花粉数据梯度限制,其相对花粉产量能否用于植被与花粉关系的校正有待通过更多植被群落调查进一步证实;其他花粉类型由于在花粉组合中含量多低于5％,所以在校正花粉与植被关系时的作用不明显.     

Optical observations of the broad-lined type Ic supernova SN 2012ap

The optical observations of the type Ic supernova(SN Ic) SN 2012 ap in NGC 1729 are presented. A comparison with other SNe Ic indicates that SN 2012 ap is highly reddened(with E(B- V)host～0.8 mag) and may represent one of the most luminous SNe Ic ever observed, with an absolute V-band peak magnitude of ～-19.3±0.5 mag after extinction correction. The near-maximum-light spectrum shows wide spectral features that are typical of broad-lined SNe Ic. One interesting feature in the spectrum is the appearance of some narrow absorption features that can be attributed to the diffuse interstellar bands, consistent with the large reddening inferred from the photometric method. Based on the light curves and the spectral data, we estimate that SN 2012 ap produced a56 Ni mass of ～ 0.3 ± 0.1M in the explosion, with an ejecta mass of 2.4+0.7-0.7M and a kinetic energy of E5K= 1.1+0.4-0.4× 102 erg. The properties of its progenitor are also briefly discussed.     

X-ray afterglow of GRB 050712: multiple energy injections into the external shock

As indicated by observed X-ray flares,a great amount of energy can be intermittently released from the postburst central engine of gamma-ray bursts(GRBs).As a natural consequence,the GRB’s external shock could be repeatedly energized.With such a multiple energy injection model,we explore the unique X-ray afterglow light curve of GRB 050712,which exhibits four shallow decay plateaus.Together with three early X-ray flares,the central engine of GRB 050712 is believed to have released energy at least seven times after the burst.Furthermore,we find that the energies released during the four plateaus are all on the same order of magnitude,but the luminosity significantly decreased with time.These results may provide some interesting implications for the GRB central engine.     

Research on method of pressure grouting piling of driven tube

The pressure grouting pile of driven tube can improve the load bearing capacity of the single pile from the mechanism of pressure grouting pile of driven tube.On the basis of analyzing the mechanism,the authors designed the machines and tools of pressure grouting,determined the operating manufacture and technology parameter on the pressure grouting secondly.The result shows that the pressure grouting pile of driven tube not only changes the pile type but also reduce the length of the pile and its engineering cost,it enhances the load bearing capacity of single pile an the same time.     

The grain-size characteristics of Quaternary deposits at Xingshan near Siping in Jilin province, China

This research paper analyses the grain-size characteristics of the Quaternary deposits at Xingshan near Siping, Jilin province in China by employing graphic measures to study the grain size distribution and its mode of transport and deposition. The Quaternary deposits at Xingshan lie unconformable on Cretaceous rocks made of siltstone, mudstone and sandstone. The average grain size is between 8.06 to 8.55Ф （0. 002 6 0. 003 7 mm）. The Quaternary deposits at Xingshan mainly compose of very fine silt to clay. The compositions of the grade are clay 63 % and silt 37 %. The clay size components are weathered debris transported and deposited by flowing water from the SE highlands or hills to the low lying NW Xingshan plains whereas the silty components accumulated by aoelian process. The Quaternary deposits at Xingshan accumulated in the middle and late Pleistocene interglacial periods from （459.12 - 39.03 ） ka to （88.92 - 7.56 ） ka. The standard deviation ranged from 0.96 to 1.36%, indicating that the sediments are moderately to poorly sorted, Coefficient of skewness ranged from 0.16 - 0.31 with an average skewness of 0. 218, （Positively skewed towards fine）. Kurtosis values （0.84- 1.05） from the grain size distribution and visual inspection of the frequency curves indicate platykurtic to mesokurtic curves and unimodal to bimodal grain-size distribution. The type of deposit formation is sand dune and the source is at a distal from its provenance.     

阿尔金造山带东段地质构造演化概论

阿尔金造山带曾是一个早古生代拗拉槽,其两侧地质体具有极为相似的地质构造特征。该区构造演化可以概括为:晚太古代至早元古代处于底侵造壳阶段,经吕梁旋回发生克拉通化,出现中元古代稳定型盖层沉积。加里东旋回中叶,经过短暂的拗拉、裂陷,分裂的塔柴板块又重新聚合。华力西旋回该区以剥蚀夷平作用为主,仅在山间断陷或山前凹陷的局部地段沉积有上泥盆统磨拉石建造。石炭纪发生短暂小规模海侵。侏罗纪全区进入陆相发育阶段。区内岩浆活动频繁,燕山旋回为最高潮。在喜山旋回,随着印度板块与欧亚板块的碰撞,该区也被卷入青藏高原总体的巨大演变之中。早期由边缘断陷转化为大型断陷盆地,至上新世湖水淹没了大部地区;晚期,随着阿尔金迅速崛起,塔里木—柴达木板块再度分裂,南盘抬升,北盘下降。文章最后探讨了阿尔金左行斜滑地震断裂带的控震作用。     

东昆仑三维重力异常解释方法研究

小波变换是一种广泛应用的信号处理技术,它具有良好的时—频局部化特性。本文探讨了小波变换在分解重力异常中的应用。同时,利用计算机对重力资料的三维定量解释,进行了初步试算。通过东昆仑地区实际资料处理,认为这二种方法在重力资料处理解释中,具有快速、简捷的特点。