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综述了大气气溶胶颗粒物的特征、颗粒物的界面反应与矿物协同演化意义;重点介绍了大气颗粒物粒径分布和矿物成分,以及常见有毒有害气体的界面反应产物特征与关键化学过程;总结了矿物颗粒在大气气溶胶形成过程中汇聚、调控、催化的作用,以及颗粒物与大气中SO2、NOx的协同反应机制;分析了微纳米颗粒对二次有机气溶胶形成的影响,以及大气矿物相颗粒界面反应产物组合及协同演化作用.可为进一步研究大气颗粒物与大气中痕量污染气体反应形成二次气溶胶进而影响大气化学组成的过程提供指导,对深入探讨大气矿物颗粒表面特性在复合污染物中多介质反应的微界面化学过程,矿物尘-污染物气溶胶体系在雾-霾形成、转换、新生粒子和阻断行为的复合作用具有重要的环境学意义. 相似文献
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近年的实验室模拟和野外观测研究表明,酚类化合物的水相反应(aqueous-phase reaction)对环境二次有机气溶胶(secondary organic aerosol,SOA)的形成具有重要的贡献,因此探讨酚类化合物光化学过程中的演化特征有助于深化二次气溶胶形成的科学认识。本文以苯酚为研究对象,利用大气压喷雾电离(ESI)-飞行时间质谱(TOF-MS),对其在水相光化学反应下的产物分布特征进行了初步探讨。水相光照实验通过直接光解(无添加氧化剂)和光氧化反应(添加H_2O_2)两种情况进行。结果表明,两种方式进行的水相光化学反应均可能生成一系列的低聚物、羟基化化合物以及其他多官能团含氧产物。在m/z 150～400的区间内,添加H_2O_2的光氧化反应产物的分子式种类(150种)明显多于直接光解的形成产物(60种),但直接光解形成的高分子量产物(如低聚物等)离子丰度明显高于光氧化反应,直接光解的产物中可观察到四聚体化合物的生成;同时,水相光反应的产物在紫外-可见光波段内具有明显的光吸收增强特征。由此推断在大气中,以苯酚为代表的酚类化合物进入大气水相环境(云、雾水和气溶胶液态水)中发生的光化学过程对大气吸光性有机物或气溶胶的形成具有贡献作用。 相似文献
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大气气溶胶地球化学研究进展 总被引：1，自引：0，他引：1
大气气溶胶地球化学研究进展刘广深，洪业汤（中国科学院地球化学研究所，贵阳５５０００２）关键词大气，气溶胶，生物地球化学循环天然和人为的颗粒物发生过程使低层大气尤其是对流层，成为大气气溶胶的圈层。大气气溶胶在地球表面无时无处不在，对人类生活和自然过程有... 相似文献
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张文倩葛茂发佟胜睿贾晨辉李伟然张欣然 《矿物岩石地球化学通报》2020,(1):44-50
土壤是大气活性含氮化合物(N2O、NOx、HONO和NH3)的重要来源。这些含氮物种释放到大气中与一次污染物发生反应,对大气氧化性和污染物的生消起到重要作用。土壤释放这些大气活性含氮物种涉及生物、化学、物理等多个过程,这些过程的反应物和反应产物之间又存在复杂的相互作用。土壤的理化性质如土壤酸碱度、湿度、含水量等对这些含氮物种的释放量有重要影响。目前在量化上述活性含氮物种以及模拟评估土壤释放过程对空气质量的影响方面存在不足。本文概括了目前国际上有关土壤释放上述活性含氮物种的机制和影响因素的研究现状,指出未来的研究需要进一步完善土壤释放活性含氮物种的关键微观机理,揭示土壤释放过程对大气污染的影响机制,以期为提高空气质量提供科学指导。 相似文献
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《矿物岩石地球化学通报》2020,(1)
土壤是大气活性含氮化合物(N_2O、NO_x、HONO和NH_3)的重要来源。这些含氮物种释放到大气中与一次污染物发生反应,对大气氧化性和污染物的生消起到重要作用。土壤释放这些大气活性含氮物种涉及生物、化学、物理等多个过程,这些过程的反应物和反应产物之间又存在复杂的相互作用。土壤的理化性质如土壤酸碱度、湿度、含水量等对这些含氮物种的释放量有重要影响。目前在量化上述活性含氮物种以及模拟评估土壤释放过程对空气质量的影响方面存在不足。本文概括了目前国际上有关土壤释放上述活性含氮物种的机制和影响因素的研究现状,指出未来的研究需要进一步完善土壤释放活性含氮物种的关键微观机理,揭示土壤释放过程对大气污染的影响机制,以期为提高空气质量提供科学指导。 相似文献
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应用带能谱的电子扫描电镜(SEM-EDX)对拉萨市夏季正常天气下收集的大气自然沉降气溶胶样品进行分析,研究了拉萨市大气降尘矿物组成和各种物相形貌特征信息。拉萨市大气颗粒物含有硅酸盐颗粒、富钙颗粒、富铁颗粒、富碳颗粒(燃煤飞灰颗粒和燃油飞灰颗粒)和植物残体颗粒。根据颗粒物数量统计发现拉萨市大气颗粒物以硅酸盐颗粒为主,富钙颗粒和富铁颗粒次之,需要指出的是以燃油飞灰为主的富碳颗粒已占到一定比重,说明以燃油为主的机动车尾气对拉萨大气污染在加强。研究结果表明,大气降尘矿物成分及其形貌特征可以用作判定污染物来源的重要标志,拉萨大气中颗粒来源的多样性决定了治理措施也应综合进行。 相似文献
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《地球化学》2020,(3)
基于2017年1月4日至7日成都市一次重霾污染过程的系留汽艇探测的低层大气气象要素和大气颗粒物垂直探空加密观测资料,分析了大气边界层结构及气溶胶垂直分布。结果表明,此次重霾污染期间,大气边界层昼夜变化特征基本消失。稳定边界层结构出现25次,对流边界层结构仅出现3次,大气边界层结构趋于稳定,边界层高度普遍在700 m以下。霾污染发生、维持及消散阶段大气边界层气溶胶垂直结构具有明显差异。霾污染发生阶段,大气边界层气溶胶粗、细粒子主要集中在300m高度以下,近地面层大气气溶胶粒子累积触发霾污染事件;霾维持阶段,大气颗粒物粒子浓度数垂直方向趋于一致,大气边界层稳定结构中存在强的大气垂直混合作用;在霾消散阶段,较高处的气溶胶粒子浓度最先下降,且下降幅度最大,表明对流层自由大气作用对霾污染消散具有影响。大气边界层风速的增大加剧了大气传输扩散。温度与大气颗粒物浓度在近地层呈负相关关系,在100m高度以上呈正相关关系。大气边界层低层偏冷,高层偏暖的稳定大气热力层结减弱了大气污染物的垂直扩散。相对湿度的增加有利于气溶胶粒子的吸湿增长和液相化学反应,加剧了霾污染。 相似文献
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北京市春夏季大气气溶胶的单颗粒分析表征 总被引：9，自引：0，他引：9
采集了北京市2000年春夏季大气气溶胶样品5个，采用扫描电镜X射线能谱技术分析大气气溶胶单颗粒约2500个。研究结果表明，沙尘期间，矿物尘是最主要的颗粒物种类，非沙尘期间，北京市大气气溶胶中主要检出矿物尘和含硫颗粒物。夏季随着颗粒物污染的加重，含硫颗粒物的数目百分数增加。是北京市大气颗粒物污染的重要特征。重点讨论了Ca-S颗粒、K-S颗粒和Ca-K-S颗粒三类典型含硫颗粒物的化学组成和粒径分布特征。数目可观的Ca-K-S颗粒以及其他硫酸盐颗粒的生成与相对湿度和云量等气象条件相关，这些颗粒物可能是云中过程的产物。减少SO2排放，减少含硫颗粒物，对于控制北京市的大气颗粒物浓度水平具有重要意义。 相似文献
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兰州市大气总悬浮颗粒物中有机污染物分布特征及来源 总被引：7，自引：1，他引：7
对兰州市区、郊区大气颗粒物、汽车尾气及烟尘样品中的饱和烃和芳香烃进行了色谱－质谱检测，较为系统地对兰州市大气有机污染物来源做了定量、半定量研究。结果表明，兰州市大气有机污染物主要来源于人为因素，小部分为自然因素。人为污染源是复杂（包括工业生产、汽车尾气和燃煤等的排放）且严重的，应引起足够重视。 相似文献
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Lal D 《Geochimica et cosmochimica acta》1993,57(19):4627-4637
We present calculations of rates of production of several nuclides in the Martian atmosphere and in the regolith due to nuclear interactions of cosmic ray and radiogenic particles and consider their implications to the evolutionary history of Mars. Nuclides selected are those which, considering their chemical properties, may be useful as tracers for delineating the past histories of the Martian atmosphere and regolith. Calculations are presented for different assumed atmospheric pressures. The regolith production rates for the present thin Martian atmosphere (approximately 20 g cm-2) are expected to be fairly robust because they are based primarily on observed cosmogenic effects in the Moon, for which semiempirical estimates of nuclide production rates have been provided earlier by Reedy (1981). Uncertainties which arise in the calculations of nuclide production rates for an earlier hypothetical Martian atmosphere of approximately 300-500 g cm-2 thickness are discussed. Compared to cosmic ray production rates, the nucleogenic production rates are smaller by several orders of magnitude. However, the nucleogenic production extends to much deeper levels, whereas the cosmogenic production is essentially confined to the top 750-1000 g cm-2 depth. Important examples of nucleogenic production are discussed. Isotopes of neon and argon appear to be very promising for delineating relative magnitudes of a number of planetary processes related to the temporal changes in the thickness of the atmosphere, as well as their release from the regolith. However, quantification of the processes would require higher-precision isotopic data for the atmosphere and also direct measurements of isotopic ratios in the Martian regolith, along with supplementary information on changes in the isotopic compositions of hydrogen, carbon, and nitrogen, which are affected by a variety of mechanisms of escape of gases from the atmosphere. Cosmogenic effects are minimal in these cases. We show that although we can at present draw but limited inferences, the planet Mars presents a unique opportunity to use cosmogenic nuclides as tools to delineate the evolutionary history of the planet as a whole, as well as its regolith and the atmosphere. This arises because of two factors: minimal degassing of the planet, and a fairly intense chemical weathering history of the upper surface. Consequently, an appreciable fraction of some of the isotopes of volatile elements is contributed by nuclear reactions. 相似文献
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The study of minerals is often focused on their crystallographic properties, chemistry and economic importance, and so their breakdown, or 'weathering'. by physical, chemical and biological processes is less well understood. However, mineral weathering is of considerable environmental significance. The interaction of minerals with water and microbes, such as algae and bacteria, controls soil fertility, the transportation of pollutants through the ground, and ultimately the removal of CO2 from the atmosphere over geological timescales. Therefore, minerals are a key factor in moderating global climate change. This article introduces conventional and new techniques that are being used by geologists to investigate these processes. 相似文献
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Methane exchange between coal-bearing basins and the atmosphere: the Ruhr Basin and the Lower Rhine Embayment, Germany 总被引：1，自引：0，他引：1
Thomas Thielemann Andreas Lücke Gerhard H. Schleser Ralf Littke 《Organic Geochemistry》2000,31(12):121
A precise knowledge of methane exchange processes is required to fully understand the recent rise of atmospheric methane concentration. Three of these processes take place at the lithosphere/atmosphere boundary: bacterial consumption of methane and emission of bacterial or thermogenic methane. This study was initiated to quantify these processes on a regional scale in the Ruhr Basin and the Lower Rhine Embayment. Since these areas are subject to bituminous coal and lignite mining, natural and anthropogenically-induced methane exchange processes could be studied. The methane emission and consumption rates and their carbon isotope signal were measured at the lithosphere/atmosphere boundary using flux chambers. On most of the soils studied, methane consumption by bacteria was identified. Thermogenic methane was released only at some of the natural faults examined. In active and abandoned bituminous coal mining areas methane emissions were restricted to small areas, where high emission rates were measured. The carbon isotope composition of methane at natural faults and in mining subsidence troughs was typical of thermogenic methane (−45 to −32 ‰ δ13C). Methane exchange balancing revealed that natural methane emissions from these two basins represent no source of atmospheric importance. However, methane release by upcast mining shafts dominates the methane exchange processes and is by about two orders of magnitude greater than methane consumption by bacterial oxidation in the soils. 相似文献
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Tectono-metallogenic systems are geological systems that link geodynamic and tectonic processes with ore-forming processes. Fundamental geodynamic processes, including buoyancy-related processes, crustal/lithospheric thinning and crustal/lithospheric thickening, have occurred throughout Earth's history, but tectonic systems, which are driven by these processes, have evolved as Earth's interior has cooled. Tectonic systems are thought to have evolved from magma oceans in the Hadean through an unstable “stagnant-lid” regime in the earlier Archean into a proto-plate tectonic regime from the late Archean onwards. Modern-style plate tectonics is thought to have become dominant by the start of the Paleozoic. Mineral systems with general similarities to modern or geologically recent systems have been present episodically (or semi-continuously) through much of Earth's history, but most of Earth's present endowment of mineral wealth was formed during and after the Neoarchean, when proto- or modern-style plate tectonic systems became increasingly dominant and following major changes in the chemistry of the atmosphere and hydrosphere. Changes in the characteristics of some mineral systems, such as the volcanic-hosted massive sulphide (VHMS) system, reflect changes in tectonic style during the evolution towards the modern plate tectonic regime, but may also involve secular changes in the hydrosphere and atmosphere.Whereas tectono-metallogenic systems have evolved in general over Earth's history, specific tectono-metallogenic systems evolve over much shorter time frames. Most mineral deposits form in three general tectono-metallogenic systems: divergent systems, convergent systems, and intraplate systems. Although fundamental geodynamic processes have driven the evolution of these systems, their relative importance may change as the systems evolved. For example, buoyancy-driven (mantle convection/plumes) and crustal thinning are the dominant processes driving the early rift stage of divergent tectono-metallogenic systems, whereas buoyancy-driven processes (slab sinking) and crustal thickening are the most important processes during the subduction stage of convergent systems. Crustal thinning can also be an important process in the hinterland of subduction zones, producing back-arc basins that can host a number of mineral systems. As fundamental geodynamic processes act as drivers at some stage in virtually all tectonic systems, on their own these cannot be used to identify tectonic systems. Moreover, as mineral systems are ultimately the products of these same geodynamic drivers, individual mineral deposit types cannot be used to determine tectonic systems, although mineral deposit associations can, in some cases, be indicative of the tectono-metallogenic system.Ore deposits are the products of geological (mineral) systems that operate over a long time frame (hundreds of millions of years) and at scales up to the craton-scale. In essence, mineral systems increase the concentrations of commodities through geochemical and geophysical processes from bulk Earth levels to levels amenable to economic mining. Mineral system components include the geological (tectonic and architectural) setting, the driver(s) of mineralising processes, metal and fluid sources, fluid pathways, depositional trap, and post-depositional modifications. All of these components link back to geodynamic processes and the tectonic system. For example, crustal architecture, which controls the spatial distribution of, and fluid flow, within mineral systems, is largely determined by geodynamic processes and tectonic systems, and the timing of mineralisation, which generally is relatively short (commonly < 1 Myr), correlates with local and/or far-field tectonic events.The geochemical characteristics of many mineral systems are a consequence of their geodynamic and tectonic settings. Settings that are characterised by low heat flow and lack active magmatism produce low temperature fluids that are oxidised, with ore formation caused largely by redox gradients or the provision of external H2S. The characteristics of these fluids are largely governed by the rocks with which they interact, rocks that have extensively interacted with the hydrosphere and atmosphere, both environments that have been strongly oxidised since the great oxidation event in the Paleoproterozoic. In settings characterised by high heat flow and active magmatism, ore fluids tend to be higher temperature and reduced, with deposition caused by cooling, pH neutralisation, depressurisation and fluid mixing. Again, the characteristics of these fluids are governed by rocks with which they interact, in this case more reduced magmatic rocks derived from the mantle or lower crust. 相似文献
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对地球系统科学的几点认识 总被引：13，自引：0，他引：13
地球系统科学将是２１世纪地球科学的主旋律,它被定义为：“将地球作为一个整体来伯全部知识;对地球的气圈、水圈、生物圈和岩石中的各种作用及各层圈间相互作用时间进行的研究”。此种学术思想可追溯到１００多年前,见於文字也有近二十年。它对当代地学的发展起了重要的推动作用,有四个特点：地球现象的远距离相互联系、影响;内动力和外动力研究一体化;地质作用和生物作用研究一体化;一类活动作为地球系统的一部分。当前地球系统科学的发展也提出了一些新问题,主要的是：在学术思路上对与岩石圈有关的地质作用有所忽视;观察研究系统不全面;还未深人到资源形成和小环境的研究中。近年来的观测试验表明,发生在岩石圈的各种地质作用正积极参与垒球各圈层间的物质能量交换。对它们的忽视,可能正是目前一些生物地球化学循环模型无法平衡的原因。 相似文献
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鉴于大陆岩浆弧上盘广泛分布有碳酸盐岩,岩体上升侵位过程使其碳通量明显的高于洋内岛弧,从而有可能影响着地质历史长时间尺度(百万年)的气候变化。陆弧碳的排放可分为两部分,一部分是与喷出岩相关的火山作用,另一部分是与侵入岩相关的脱碳过程。侵入岩的体量一般是喷出岩体量的10倍以上,由此与侵入岩有关的脱碳作用释放的碳通量不可忽视,可能类似与喷出岩有关的火山作用释放的碳通量甚至更大。火山作用能够将气体直接排入大气中,因此在以往的工作中研究较为充分。但与侵入岩相关的脱碳过程如:矽卡岩化,发生在地下,关于地下脱碳过程如何将碳释放到大气中还缺少详细的工作。本文,通过对比研究火山地区和非火山地区与侵入岩相关的深部脱碳过程,发现深部碳可以通过区域断层系统、地下水系统和热泉、火山通道、隐爆角砾岩筒、高频率的岩浆热液事件等途径瞬时地释放进入大气。通过初步估算,发现单个矽卡岩矿化事件所产生的二氧化碳通量(0.02~0.2Mt/yr)能够与目前地球绝大部分的普通单个火山的碳通量(<0.5Mt/yr)类比。因此岩浆深部脱碳过程对大气的影响至少与火山相当,其对气候的影响不可忽视。 相似文献
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根据行星探测的资料,综合分析了水星、金星、地球(包括月球)、火星的大气层和水体的发育特征,对比了金星、火星的大气层与水体同地球的差异。类地行星质量小、体积小、密度大、旋转慢、卫星少甚至没有、挥发性元素较类木行星少、距离太阳较近,早期残留的原始大气层已经被早期太阳在金牛变星阶段的强烈太阳风所驱赶,加上巨大而频繁的撞击作用,使原始大气层被驱赶殆尽。现在的大气层是次生的,是由行星内部的去气作用形成的。类地行星的大气层、水体的发育和表生作用的特征与行星的质量大小(表征行星内部能量的大小和构造活动的强烈及持续时间)及行星与太阳的距离等因素有关。在类地行星中,地球和金星质量最大,逃逸速度最大,可将更多的气体“束缚”在它们表面,因此它们的大气有着复杂的组成和较大的密度。火星质量较小,逃逸速度不到地球的一半,在漫长的演化历史中,大气逐渐逸散进入太空,大气密度变得很稀薄。水星质量更小,而且最靠近太阳,不仅太阳风的驱赶作用强烈,而且表面温度高,气体分子的热运动更加剧烈,加剧了大气的逸散,所以水星的大气层极为稀薄,并且主要为太阳风成分。月球质量最小,几乎没有大气层,更没有水体的发育。行星的热演化历史对大气层和水体发育具有重要的制 相似文献
20.
D. V. Bisikalo A. A. Cherenkov V. I. Shematovich L. Fossati C. Möstl 《Astronomy Reports》2018,62(10):648-653
A one-dimensional aeronomic model of the upper atmosphere of a giant planet is used to study the reaction of the atmosphere of the hot Jupiter HD 209458b to additional heating by a stellar flare. It is shown that the absorption of additional energy from the stellar flare in the extreme ultraviolet leads to local heating of the atmosphere, accompanied by the formation of two shocks propagating in the atmosphere. Possible observational manifestations of these shocks and the feasibility of their detection are discussed. 相似文献