Can we constrain the evolution of HI bias using configuration entropy?     

Biswajit Das  Biswajit Pandey 《天文和天体物理学研究(英文版)》2021,(2)

We study the evolution of the configuration entropy of HI distribution in the post-reionization era assuming different time evolution of HI bias.We describe time evolution of linear bias of HI distribution using a simple form b(a)=b₀aⁿ with different index n.The derivative of the configuration entropy rate is known to exhibit a peak at the scale factor corresponding to theΛ-matter equality in the unbiasedΛCDM model.We show that in theΛCDM model with time-dependent linear bias,the peak shifts to smaller scale factors for negative values of n.This is related to the fact that the growth of structures in the HI density field can significantly slow down even before the onset ofΛdomination in the presence of a strong time evolution of the HI bias.We find that the shift is linearly related to the index n.We obtain the best fit relation between these two parameters and propose that identifying the location of this peak from observations would allow us to constrain the time evolution of HI bias within the framework of theΛCDM model.  相似文献   

GRB 130310A: very high peak energy and thermal emission     

Song-Mei Qin  Lu-Yao Jiang  Xiang-Gao Wang 《天文和天体物理学研究(英文版)》2021,(3):215-226

The special GRB 130310 A was observed by Fermi Gamma-Ray Burst Monitor and Large Area Telescope,with T90~2.4 s.With a combination of a Band function and a blackbody(BB)function,the time-resolved spectral analysis of GRB 130310 A confirmed that there is a sub-dominate thermal component in the early period(e.g.,slice T0+[4.03-4.14]s)spectrum with BB temperature(kT)being~7~5 keV,which can be interpreted as photosphere emission.The precursor of GRB 130310 A can be fitted well with a BB component with kT~45 keV,which is higher than that of the main burst.It suggests that the radiation of GRB 130310 A is in transition from thermal to non-thermal.Such a transition is an indication of the change in jet composition from a fireball to a Poynting-flux-dominated jet.A very high peak energy is obtained in the first time bin,with the peak energy E_p of the Band component for Band+BB and Band model being~8.5~5.2 MeV and~11.1~7.4 MeV,respectively.Afterwards,the E_p drops to~1 MeV.The E_p evolution patterns with respect to the pulses in the GRB 130310 A light curves show a hard-to-soft evolution.The interpretation of the high peak energy E_p within the photosphere and internal shock model is difficult.It also suggests that at least for some bursts,the Band component must invoke a non-thermal origin in the optically thin region of a GRB outflow.Assuming the redshift is z~0.1~8,the radius of the jet base r₀~10⁹ cm to allow(1+σ₁₅)>1 in line with the calculation results of the magnetization parameter at~1015 cm(σ₁₅).However,the value of(1+σ₁₅)is■1 in the zone z around 3 for r₀~10⁹ cm,suggesting the non-excluded possibility that the origin is from ICMART with a low value.The photosphere-internal shock seems capable of interpreting the high peak energy,which requires electron Lorentz factorγe~60 andεe~0.06.  相似文献   

Guide for contributors     

《世界地质(英文版)》2020,(1):I0002-I0002

The journal of Global Geology(English Edition)is sponsored by the International Center of Geoscience Research and Education in Northeast Asia,Jilin University of China(ISSN 1673-9736,CN22-1371/P).The former name of the journal was the Journal of International Geoscientific Research in Northeast Asia.  相似文献   

微量沉降背景下地面沉降GPS测量最佳观测时段研究     

熊福文 《上海国土资源》2020,41(1)

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Effect of Shale Reservoir Characteristics on Shale Oil Movability in the Lower Third Member of the Shahejie Formation,Zhanhua Sag     

NING Chuanxiang  MA Zhongliang  JIANG Zhenxue  SU Siyuan  LI Tingwei  ZHENG Lunju  WANG Guozhen  LI Fengxun 《《地质学报》英文版》2020,94(2):352-363

To reveal the effect of shale reservoir characteristics on the movability of shale oil and its action mechanism in the lower third member of the Shahejie Formation(Es3l), samples with different features were selected and analyzed using N2 adsorption, high-pressure mercury injection capillary pressure(MICP), nuclear magnetic resonance(NMR), high-speed centrifugation, and displacement image techniques. The results show that shale pore structure characteristics control shale oil movability directly. Movable oil saturation has a positive relationship with pore volume for radius > 2 μm, as larger pores often have higher movable oil saturation, indicating that movable oil is present in relatively larger pores. The main reasons for this are as follows. The relatively smaller pores often have oil-wetting properties because of organic matter, which has an unfavorable effect on the flow of oil, while the relatively larger pores are often wetted by water, which is helpful to shale oil movability. The rich surface provided by the relatively smaller pores is beneficial to the adsorption of immovable oil. Meanwhile, the relatively larger pores create significant pore volume for movable oil. Moreover, the larger pores often have good pore connectivity. Pores and fractures are interconnected to form a complex fracture network, which provides a good permeability channel for shale oil flow. The smaller pores are mostly distributed separately;thus, they are not conducive to the flow of shale oil. The mineral composition and fabric macroscopically affect the movability of shale oil. Calcite plays an active role in shale oil movability by increasing the brittleness of shale and is more likely to form micro-cracks under the same stress background. Clay does not utilize shale oil flow because of its large specific surface area and its block effect. The bedding structure increases the large-scale storage space and improves the connectivity of pores at different scales, which is conducive to the movability of shale oil.  相似文献   

黄河站低热层中性风对极光亚暴的响应     

覃明辉  张燕革  艾勇 《极地研究》2019,31(2)

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浙西邵家山埃迪卡拉纪地层的碳同位素特征及其地层对比意义     

《地层学杂志》2020,(2)

埃迪卡拉纪普遍缺乏有效的同位素年龄和生物地层资料,碳同位素(δ~(13)C_(carb))常用来作为其内部地层划分与对比的标准。目前,关于埃迪卡拉纪扬子地台δ~(13)C_(carb)地层的研究多集中在中上扬子区,扬子地台东缘下扬子区的研究则较少。本文详细分析了扬子地台下扬子区邵家山剖面地层序列和δ~(13)C_(carb)特征,发现邵家山剖面以碳酸盐岩为主,为该时期典型的浅水相沉积;δ~(13)C_(carb)值分布范围为–2.6‰～5.7‰,均值为0.9‰±0.3‰。剖面的下部、中下部、中上部以及上部的δ~(13)C_(carb)负漂移幅度分别为1.6‰、4.1‰、7.6‰和3.2‰,可分别对应峡东地区的EN1/CANCE、EN2/BAINCE、EN3/DOUNCE和EN4/BACE。对比分析扬子地台典型的8个浅水相剖面发现:盖帽白云岩广泛发育EN1/CANCE,δ~(13)C_(carb)分布在–6‰～0‰之间;EN3/DOUNCE在各剖面均有发育,漂移幅度均大于4‰,最大可达15.6‰; EN2/BAINCE仅在峡东地区的剖面发育,漂移幅度可达8.2‰; EN4/BACE在大多数剖面发育,漂移幅度为1.2‰～8.7‰。其中, EN4/BACE可作为广泛采用的埃迪卡拉系—寒武系界线的划分依据,而EN1/CANCE和EN3/DOUNCE可作为扬子地台埃迪卡拉系内部地层划分对比的重要标志。  相似文献   

扎格罗斯前陆盆地晚中新世快速剥露证据——来自磷灰石(U- Th)/He的约束     

李佳纬  孙继敏  吕丽星  张志亮  田晟辰  曹萌萌  李有生  苏柏 《地质学报》2020,94(12):3674-3688

伊朗扎格罗斯造山带是世界上最年轻的造山带之一，前人对其构造演化历史的研究尚存争议。前陆盆地蕴藏着丰富的造山带热史信息，为研究造山带的隆升和剥露历史提供了重要途径。本研究选取位于扎格罗斯前陆盆地前缘中部的Kuh- E Bedush向斜和Kuh- E Murdeh向斜翼部出露的第三纪陆相红层(Agha Jari组)为研究对象，共采集11个粗砂岩样品进行磷灰石(U- Th)/He测试分析。11个样品共得到38个单颗粒年龄，年龄区间为0. 8~79. 9Ma。大部分样品的单颗粒年龄比较分散，表明这些样品没有发生完全热重置。相反，位于Murdeh向斜剖面最底部的样品，(U- Th)/He年龄小于其对应的地层年龄，并且集中分布在8. 3~6. 8Ma，表明该样品发生了完全重置并记录了最后一次剥露事件的时间。因此，我们认为扎格罗斯前陆盆地于晚中新世~7. 5 Ma经历了一期快速剥露事件。此外，我们发现未重置的(U- Th)/He年龄大致分布在四个时间段：晚白垩纪—早古新世、早—中始新世、渐新世、早—中中新世。根据所得热年龄并结合前人研究设定了三种不同的热史，正演模拟结果与实际样品拟合较好，由此推断出前陆中部Agha Jari陆相红层沉积物可能来自于：①晚白垩世以来以蛇绿岩套为主的仰冲体持续剥露；②萨南达季- 锡尔詹变质带(SSZ)渐新世和中新世逐渐加速的剥露；③渐新世末堆积在仰冲体之上的同造山期砾岩，在中新世的大规模逆冲作用下重新剥露。  相似文献   

大西洋鲑在封闭循环水养殖模式下的生长和性腺发育研究   总被引：1，自引：0，他引：1  

徐世宏  王彦丰  刘清华  刘鹰  王顺奎  徐滢轩  李军 《海洋科学》2019,43(11):97-102

本研究探讨了在封闭循环水养殖模式下大西洋鲑(Salmosalar)的生长发育模式,对封闭循环水系统养殖的大西洋鲑重要生长数量性状进行生物学测量,并跟踪性腺发育状况。本研究自2012年1月通过封闭循环水系统进行大西洋鲑养殖,经过周年养殖,体质量平均达到1194.42g,体长平均达到417.00 mm,体高平均达到100.58 mm,体宽平均达到53.52 mm,少数个体在养殖10个月后性腺发育较快,性腺质量达到9.76 g,性腺指数达到1.31%。本研究的研究结果为建立大西洋鲑标准化循环水养殖系统积累资料。  相似文献   

海底观测网发展现状及趋势研究     

陈建冬  张达  王潇  潘筱屹  王策男  张自丽  葛辉良 《海洋技术学报》2019,38(6):95-103

文中详细研究了当前世界上最典型的海底观测网的建设发展规模、形式、设备类型以及我国海底观测网的发展现状,并对国内外海底观测网的发展趋势进行总结。对日本、加拿大、美国及欧洲的海底观测网进行了设备级研究,对我国台湾地区、东海、南海的海底观测网现状进行了研究,并讨论了国外先进观测网对我国的海底观测网建设的借鉴意义。文中总结出海底观测网发展的整体趋势为:单节点网络加速验证新型设备及传感器的水下能力;区域尺度网络用于加速多学科发展并提升灾害预警能力;而浮标平台网络作为补充,铺设在远海区域以降低阶段建设成本。  相似文献