东准造山带原泥盆系的形成时代及源区：碎屑锆石U-Pb年代学证据

新疆东准地区晚古生代地层出露广泛,其沉积时限的精确限定对理解中亚造山带的增生和拼贴过程、确立该地区构造框架及油气开发具有深远意义。然而,目前的研究主要集中于岩浆岩方面,对于晚古生代地层时代及其空间展布的研究则相对缺乏,特别是石炭系和泥盆系沉积地层标定较为模糊。为此,本文选取了3个原泥盆系砂岩进行了细致的野外剖面测制、岩石学观测和碎屑锆石U-Pb年代学分析。研究显示：原泥盆纪砂岩的最年轻碎屑锆石年龄为346～312 Ma,碎屑锆石年龄谱图分为：380～310 Ma（晚泥盆世-早石炭世,71.8%）、445～385 Ma（志留纪-早-中泥盆世,11.7%）、480～450 Ma（奥陶纪,3.9%）、540～485 Ma（寒武纪,4.5%）和前寒武纪年龄段（8.1%）,碎屑锆石年龄谱图区域上具有由南向北、由西向东呈简单化趋势且晚古生代年龄比重增加。结合该区岩浆岩年代学研究成果,将研究区原泥盆系沉积时代重新厘定到晚石炭系早-中期,认为东准地区的碰撞拼贴时间应发生于晚石炭世,并非是不同期次碰撞拼贴之产物。     

陆生植物氮同位素组成与气候环境变化研究进展

近年来,由于植物氮同位素组成(δ15N)记载了气候环境变化的信息,因而被广泛应用于全球变化研究中,成为古气候环境再造和了解现代气候环境变化信息的有力工具。然而,人们对气候环境引起的δ15N变化及其指示的气候环境意义并不完全清楚,这就有可能限制植物δ15N在古气候环境变化等领域研究中的应用。在概述植物氮同位素分馏和植物不同氮源的氮同位素分布的基础上,分析了温度、降水、大气CO2浓度和海拔高度等气候环境因子对陆生植物δ15N的影响以及它们的关系。指出了目前研究中存在的问题及其研究前景,认为在全球变化研究中利用植物氮同位素技术不仅可以重建古气候环境(如重建大气CO2浓度变化),揭示历史时期温度、降水的变化,而且还可以在一定的时间和空间上综合反映生态系统氮循环的特征。     

Recent Progresses in Comparative Planetology——Summary of the Session of Comparative Planetology at the 3rd Conference of Earth System Sciences

Comparative planetology is an interdisciplinary science between Earth sciences and astronomy. It studies physical, chemical and dynamical properties of planets and satellites and their surface characteristics, interior structures and chemistry, magnetic field, climate and possible existence of life. Although the study of comparative planetary science is at its infancy stage in China, it is very encouraging to see that 25 papers were received by the session, which is much more than what we expected. It indicates that more and more scientists are interested in this research field. These papers can be classified into three categories: solar planets, extra-solar planets, and moon explorations. Scientists from both China and oversea reported their recent results.     

Research Progress in Responses of Modern Terrestrial Plant Carbon Isotope Composition to Climate Change

Global climate change has been one of the most concerned environmental problems in the world since the 1980s. Since stable carbon composition (¹³C) in plant tissues can record abundant information on climate changes, it has been widely used as an important climate proxy in global change studies and becomes a powerful tool for obtaining paleoclimate information, understanding paleoenvironment reconstruction and modern climate change, and predicting future climate trends. However, a lot of potential uncertainties have always involved in the reconstruction of paleoclimate and paleoenvironment by carbon isotope of the past period sediment or fossils. Among them, the most dominant uncertainty is due to our poor understanding of the relations between carbon isotope ratios of plants and climatic factors and the climatic and environmental significance indicated by modern plant ¹³C. This may limit the application of plant ¹³C in the study of climatic and environmental changes. Based on the Summary of plant ¹³C fractionation and carbon isotope distribution of different photosynthetic plants, the effects of environmental factors, e.g., temperature, precipitation, atmospheric CO₂ concentration, and altitude on terrestrial plant ¹³C and their relationships were reviewed in this paper, and the response mechanism of plant ¹³C to climate changes were also analyzed. Furthermore, the current existing problems and the future prospects in carbon isotope study were discussed. It is pointed out that strengthening some studies such as the response of C₄ plants ¹³C to climate environmental parameters, the transformation relation of different scale plant ¹³C, intersection and permeation of related disciplines, and various proxies and scientific method, will undoubtedly make us have a more accurate understanding of the climate history and eventually broaden the development of the field during the process of global change study by plant carbon isotope techniques.     

Characteristics of the supernova remnant G351.7+0.8 and a distance argument against its association with PSR J1721−3532

New images of the supernova remnant (SNR) G351.7+0.8 are presented based on 21-cm H  i -line emission and continuum emission data from the Southern Galactic Plane Survey. SNR G351.7+0.8 has a flux density of 8.4 ± 0.7 Jy at 1420 MHz. Its spectral index is 0.52 ± 0.25 ( S = v ^−α) between 1420 and 843 MHz, typical of adiabatically expanding shell-like remnants. H  i observations show structures possibly associated with the SNR in the radial velocity range of −10 to −18 km s⁻¹, and suggest a distance of 13.2 kpc and a radius of 30.7 pc. The estimated Sedov age for G351.7+0.8 is less than  6.8×10⁴ yr  . A young radio pulsar PSR J1721−3532 lies close to SNR G351.7+0.8 on the sky. The new distance and age of G351.7+0.8 and recent proper motion measurements of the pulsar strongly argue against an association between SNR G351.7+0.8 and PSR J1721−3532. There is an unidentified, faint X-ray point source 1RXS J172055.3−353937 which is close to G351.7+0.8. This may be a neutron star potentially associated with G351.7+0.8.     

关中盆地潜水化学特征及其变化趋势

本文在阐明关中盆地环境水文地质条件的基础上,论述了关中盆地潜水化学特征及其成因,并着重对盆地潜水化学变化的几个主要问题,诸如常规组份的升高及水化学类型的改变、潜水硬度的升高、硝酸盐的富集及微量重金属元素的污染等进行了分析。讨论了上述问题的因果及今后工作意见。     

Deepwater Ventilation and Stratification in the Neogene South China Sea

Combined data of physical property, benthic foraminifera, and stable isotopes from ODP Sites 1148, 1146, and 1143 are used to discuss deep water evolution in the South China Sea (SCS) since the Early Miocene. The results indicate that 3 lithostratigraphic units, respectively corresponding to 21-17 Ma, 15-10 Ma, and 10-5 Ma with positive red parameter (a*) marking the red brown sediment color represent 3 periods of deep water ventilation. The first 2 periods show a closer link to contemporary production of the Antarctic Bottom Water (AABW) and Northern Component Water (NCW), indicating a free connection of deep waters between the SCS and the open ocean before 10 Ma. After 10 Ma, red parameter dropped but stayed higher than the modern value (a*=0), the CaCO3 percentage difference between Site 1148 from a lower deepwater setting and Site 1146 from an upper deepwater setting enlarged significantly, and benthic species which prefer oxygen-rich bottom conditions dramatically decreased. Coupled with a major negative excursion of benthic δ13C at ~10 Ma, these parameters may denote a weakening in the control of the SCS deep water by the open ocean. Probably they mark the birth of a local deep water due to shallow waterways or rise of sill depths during the course of sea basin closing from south to east by the west-moving Philippine Arc after the end of SCS seafloor spreading at 16-15 Ma. However, it took another 5 Ma before the dissolved oxygen approached close to the modern level. Although the oxygen level continued to stabilize, several Pacific Bottom Water (PBW) and Pacific Deep Water (PDW) marker species rapidly increased since ~6 Ma, followed by a dramatic escalation in planktonic fragmentation which indicates high dissolution especially after ~5 Ma. The period of 5-3 Ma saw the strongest stratified deepwater in the then SCS, as indicated by up to 40% CaCO3 difference between Sites 1148 and 1146. Apart from a strengthening PDW as a result of global cooling and ice cap buildup on northern high latitudes, a deepening sea basin due to stronger subduction eastward may also have triggered the influx of more corrosive waters from the deep western Pacific. Since 3 Ma, the evolution of the SCS deep water entered a modern phase, as characterized by relative stable 10% CaCO3 difference between the two sites and increase in infaunal benthic species which prefer a low oxygenated environment. Thesubsequent reduction of PBW and PDW marker species at about 1.2 Ma and 0.9 Ma and another significant negative excursion of benthic δ13C to a Neogene minimum at ~0.9 Ma together convey a clear message that the PBW largely disappeared and the PDW considerably weakened in the Mid-Pleistocene SCS. Therefore, the true modern mode SCS deep water started to form only during the "Mid-Pleistocene climatic transition" probably due to the rise of sill depths under the Bashi Strait.     

川东北元坝西部须家河组二段优质储层展布特征研究

川东北元坝地区须家河组二段致密砂岩气资源潜力巨大,但储量探明率低、测试效果差异大,主要原因之一是致密砂岩储层非均质性强、优质储层分布规律不清。本文充分利用测录井、岩心及相关分析化验等资料,在分砂组刻画沉积微相展布的基础上,开展了须二段沉积演化过程、储层特征及其分布研究。结果表明：（1）元坝西部须二段经历了辫状河三角洲-滨浅湖-辫状河三角洲演化过程,沉积控制了砂体规模、粒度和矿物成分的空间变化;（2）须二段砂岩类型多样,整体致密,为低孔、低渗储层;储层物性与砂岩粒度,长石、石英和方解石胶结物含量等因素密切相关,这些因素主要受沉积和后期成岩作用控制;（3）须二段发育块状中粒长石岩屑砂岩和交错层理中粒石英砂岩两类有利岩石相,前者自西北向东南逐渐减薄、呈条带状展布,后者呈不连续土豆状,主体分布于西南部地区。     

2022年四川泸定MS6.8地震前地震活动与地球物理观测异常回顾与讨论

2022年9月5日四川泸定M_S6.8地震发生在2022年度全国地震重点危险区内,且震前作了较好的短期预测。本文回顾了中期(年度)和短期阶段地震活动和地球物理观测异常。①2022年度危险区确定的核心依据有川滇藏交界4级地震空区、危险区附近M_L≥3.5地震空区、跨断层形变趋势异常和重力场异常等,其中,川滇藏交界4级地震空区被2022年1月2日云南宁蒗M_S5.5地震打破具有中短期预测意义。②短期阶段,川滇藏交界4级地震空区经历了“打破—增强—平静”的演化过程,与1973年四川炉霍M_S7.6地震前高度相似,这可能与其发震构造相同、震源机制解一致和深部孕震环境相似有关。此外,还存在川滇地区震群和多个余震区准同步活动、巴塘显著震群等异常。地球物理观测方面,在2022年6月1日芦山M_S6.1和6月10日马尔康M_S6.0地震后,四川前兆异常无明显减少,而在7—8月显著增多,这可以作为强震后短期仍有可能再次发生强震的判定依据。新增异常主要分布在以三岔口(鲜水河断裂带、安宁河断裂带和龙门山断裂带交汇区,呈“Y”字形分布)为中心的300km范围内,这是震前短期地点预测的主要依据之一。③6.8级地震前形变中短期大幅度异常突出,且异常点均位于远场(距离6.8级地震震中130～300km范围内)。除礼州测距外,其余异常点均位于M_L3.5地震空区外围。形变异常出现的时间与M_L3.5地震空区打破后空区内部及边缘地震活动显著增强大体一致。④泸定6.8级地震发生在三岔口地区,该区及附近2015—2021年连续多年被确定为全国地震重点危险区,但均未发生预测地震,由此表明当前有效的强震年度(中期)时间预测依据少。     

Dating of multi-period earthquake-triggered rockfalls: a method for revealing paleo-seismic events that occurred along the Yushu fault in the eastern Tibetan Plateau

Landslides - The quantitative study of earthquake-triggered rockfall debris along seismogenic fault zones has proven to be a valid approach for use in identifying paleo-earthquakes and faulting...