洞穴滴水、石笋中元素及元素比值对气候环境变化响应的研究进展     

马源  殷建军  袁道先 《地质论评》2022,68(5):1897-1911

滴水/石笋元素是除δ18O和δ13C,研究气候环境变化的又一重要代用指标。外界气候环境变化通过改变表层岩溶带和岩溶含水层中的水文环境,甚至洞穴环境,进而影响元素的溶解、运移和沉淀过程,从而使得滴水/石笋中元素表现一定的变化规律。本文通过分析影响洞穴滴水元素及元素比值变化的因素：元素来源、水—岩相互作用和滞留时间、差异性淋滤、先期碳酸盐沉淀及分配系数的基础上,从元素对岩溶区“二元结构”和极端天气/气候事件响应的角度,探讨了滴水/石笋中元素的气候环境指示意义。取得了以下认识：① 强降水带来的冲刷作用和溶解作用,促进土壤和基岩中元素、胶体和天然有机质（NOM：Natural Organic Matter）等物质在短时间内快速溶解和运移,使滴水中元素含量增加;但随着降水增多带来的稀释作用,使得滴水/石笋中Mg,Sr和Ba等元素含量降低,因此,单一元素的解译较为复杂;② 基岩/溶液中元素溶解和沉积的差异,导致元素相对含量的变化,使得元素X/Ca值对外界环境的响应具有一致性,尤其是Mg/Ca和Sr/Ca值：在干旱条件下,降水减少导致方解石先期沉积（PCP：Prior Calcite precipitation）作用增强,使Mg/Ca和Sr/Ca值增大。但目前存在着一些问题：① Mg/Ca和Sr/Ca值变化对强降水事件的响应并不明显,可能与新、老水混合及元素溶解过程中的溶解比例差别不大有关;② 多源、多期混合水源会导致洞穴滴水元素对极端事件响应减弱;③ Mg/Ca和Sr/Ca的变化为解释δ18O的“雨量效应”及“源效应”提供了见解,但元素变化能否反映季风强度的变化,仍有待进一步的研究。基于以上认识,笔者提出开展更加系统的大气—土壤—包气带—洞穴的监测;开展更高分辨率、更长时间尺度的洞穴监测;开展多区域、多洞穴系统对比研究来更加深入地开展洞穴石笋元素研究。  相似文献   

含油气盆地蒸发盐矿物成因类型及其地质意义^*          下载免费PDF全文

郭佩  李长志 《古地理学报》2022,24(2):210-225

中国是一个多盐湖国家,然而盐湖研究主要集中于分析湖水化学性质、盐类物质来源和盐矿资源开发等,对盐类矿物沉积特征和埋藏成岩改造研究较少,造成从蒸发岩角度去理解古代盐湖盆地的油气富集规律较为困难。在广泛阅读国内外大型盐湖文献的基础上,笔者介绍了盐湖分类方案和蒸发岩中盐类矿物的主要成因类型,并总结了中国陆相含油气盆地中常见的硫酸盐、氯化物、含钠碳酸盐和硼酸盐的沉积—成岩过程及其古环境和古气候意义。同时,尝试利用盐湖沉积最新研究成果去探讨中国含油气盆地蒸发岩研究中存在争议或值得关注的问题,得出: (1)深部热液可为湖泊输送大量元素离子,但要在湖泊环境下富集大量蒸发岩,则(半)干旱气候和蒸发浓缩作用是前提条件;(2)易溶蒸发岩(如石盐)在沉积中心单层厚度大,而在斜坡—边缘区缺失,这是季节性气温变化和温跃层浮动引发“中心聚集效应”的结果;(3)温度可影响蒸发岩中盐类矿物溶解度、晶体结构形态和发育深度,而部分无水盐类矿物在常温常压下却无法结晶,这一现象可用来指示古地温和地层埋藏史;(4)碳酸盐型盐湖中的Na-碳酸盐种类可指示大气CO₂浓度和古温度。  相似文献   

砾石覆盖紫色土坡耕地水文过程   总被引：15，自引：0，他引：15       下载免费PDF全文

王小燕  李朝霞  蔡崇法 《水科学进展》2012,23(1):38-45

紫色土中砾石分布广泛,地表常为砾石覆盖,砾石覆盖对土壤水文过程有着重要影响。试验小区(2 m×1 m)为坡度23°的坡耕地, 试验降雨强度为(53.9±2.8)mm/h、 (90.8±6.1)mm/h和(134.3±14.9)mm/h, 砾石覆盖度为0%,11%,20%,33%和42%。通过原位人工模拟降雨试验,定量研究了不同降雨强度下砾石覆盖对降雨入渗、地表产流及壤中流产流的影响。结果表明:砾石覆盖对入渗过程影响显著,稳定入渗速率及稳定入渗系数与砾石覆盖度呈正相关关系,3种降雨强度下,稳定入渗系数分别为47.70%~86.59%,30.61%~82.83%、17.76%~77.44%,42%砾石覆盖度小区的稳定入渗速率分别是裸露小区的1.95~4.94倍;地表砾石覆盖延迟地表产流、减少地表径流量,地表产流时间随着砾石覆盖度的提高呈增加趋势,地表径流速率及地表径流系数随砾石覆盖度的增加而降低,相对地表径流系数与地表砾石覆盖度呈指数负相关关系;地表砾石覆盖促进壤中流的发生、增加壤中流量,壤中流产流时间随着砾石覆盖度的增加逐渐缩短,壤中流径流速率及壤中流径流系数随地表砾石覆盖度的增加而提高,相对壤中流径流系数与地表砾石覆盖度呈指数正相关关系。  相似文献   

中国庐山晚第四纪沉积岩系的石英形貌显微结构及环境过程     

胡东生  李小豫  熊卫强  张华京  弓虎军  胡文瑄  张国伟 《地质学报》2012,86(6):1020-1030

基于庐山山地晚第四纪地层典型断面的系统调查,从地层剖面层序中筛选的微粒(θ=1～3mm)石英颗粒进行环境电子显微镜观测研究,辨认出显微结构-颗粒形态-变形构造-动力化学作用等特征,运用系统过程发展中的节点事件进行层型剖面的环境响应分析,采取综合指标表征地球表层过程及环境响应情景,明确划分出四个古气候环境发展阶段,由下往上分别表现为冰期环境-间冰期环境-冰缘环境-冰后期环境,为深入研究及科学认识庐山第四纪环境演化过程及全球变化提供了新的基础依据。  相似文献   

Hydrocarbon lakes on Titan     

Giuseppe Mitri  Adam P. Showman  Ralph D. Lorenz 《Icarus》2007,186(2):385-394

The Huygens Probe detected dendritic drainage-like features, methane clouds and a high surface relative humidity (∼50%) on Titan in the vicinity of its landing site [Tomasko, M.G., and 39 colleagues, 2005. Nature 438, 765-778; Niemann, H.B., and 17 colleagues, 2005. Nature 438, 779-784], suggesting sources of methane that replenish this gas against photo- and charged-particle chemical loss on short (10-100) million year timescales [Atreya, S.K., Adams, E.Y., Niemann, H.B., Demick-Montelara, J.E., Owen, T.C., Fulchignoni, M., Ferri, F., Wilson, E.H., 2006. Planet. Space Sci. In press]. On the other hand, Cassini Orbiter remote sensing shows dry and even desert-like landscapes with dunes [Lorenz, R.D., and 39 colleagues, 2006a. Science 312, 724-727], some areas worked by fluvial erosion, but no large-scale bodies of liquid [Elachi, C., and 34 colleagues, 2005. Science 308, 970-974]. Either the atmospheric methane relative humidity is declining in a steady fashion over time, or the sources that maintain the relative humidity are geographically restricted, small, or hidden within the crust itself. In this paper we explore the hypothesis that the present-day methane relative humidity is maintained entirely by lakes that cover a small part of the surface area of Titan. We calculate the required minimum surface area coverage of such lakes, assess the stabilizing influence of ethane, and the implications for moist convection in the atmosphere. We show that, under Titan's surface conditions, methane evaporates rapidly enough that shorelines of any existing lakes could potentially migrate by several hundred m to tens of km per year, rates that could be detected by the Cassini orbiter. We furthermore show that the high relative humidity of methane in Titan's lower atmosphere could be maintained by evaporation from lakes covering only 0.002-0.02 of the whole surface.  相似文献   

Point pattern analysis of north polar crescentic dunes, Mars: A geography of dune self-organization     

Mark A. Bishop 《Icarus》2007,191(1):151-157

The geographic signature of dune distribution and self-organization as measured by the R-statistic offers a viewpoint on the geography of crescentic eolian systems and proposes an index from which to determine the degree of self-organization across a variety of spatial scales. Fields of simple dunes (dome, barchan, barchan-seif) are comparatively less regular in distribution than are those fields, or part thereof, that consist of compound (barchanoid) morphologies whose patterns are more highly regular.  相似文献   

Antarctic dry valleys: Microclimate zonation, variable geomorphic processes, and implications for assessing climate change on Mars     

David R. Marchant  James W. Head III 《Icarus》2007,192(1):187-222

The Antarctic Dry Valleys (ADV) are generally classified as a hyper-arid, cold-polar desert. The region has long been considered an important terrestrial analog for Mars because of its generally cold and dry climate and because it contains a suite of landforms at macro-, meso-, and microscales that closely resemble those occurring on the martian surface. The extreme hyperaridity of both Mars and the ADV has focused attention on the importance of salts and brines on soil development, phase transitions from liquid water to water ice, and ultimately, on process geomorphology and landscape evolution at a range of scales on both planets. The ADV can be subdivided into three microclimate zones: a coastal thaw zone, an inland mixed zone, and a stable upland zone; zones are defined on the basis of summertime measurements of atmospheric temperature, soil moisture, and relative humidity. Subtle variations in these climate parameters result in considerable differences in the distribution and morphology of: (1) macroscale features (e.g., slopes and gullies); (2) mesoscale features (e.g., polygons, including ice-wedge, sand-wedge, and sublimation-type polygons, as well as viscous-flow features, including solifluction lobes, gelifluction lobes, and debris-covered glaciers); and (3) microscale features (e.g., rock-weathering processes/features, including salt weathering, wind erosion, and surface pitting). Equilibrium landforms are those features that formed in balance with environmental conditions within fixed microclimate zones. Some equilibrium landforms, such as sublimation polygons, indicate the presence of extensive near-surface ice; identification of similar landforms on Mars may also provide a basis for detecting the location of shallow ice. Landforms that today appear in disequilibrium with local microclimate conditions in the ADV signify past and/or ongoing shifts in climate zonation; understanding these shifts is assisting in the documentation of the climate record for the ADV. A similar type of landform analysis can be applied to the surface of Mars where analogous microclimates and equilibrium landforms occur (1) in a variety of local environments, (2) in different latitudinal bands, and (3) in units of different ages. Documenting the nature and evolution of the ADV microclimate zones and their associated geomorphic processes is helping to provide a quantitative framework for assessing the evolution of climate on Mars.  相似文献   

Valley formation on martian volcanoes in the Hesperian: Evidence for melting of summit snowpack, caldera lake formation, drainage and erosion on Ceraunius Tholus     

Caleb I. Fassett 《Icarus》2007,189(1):118-135

Ceraunius Tholus, a Hesperian-aged volcano in the Tharsis region, is characterized by small radial valleys on its flanks, and several larger valleys originating near its summit caldera. All of these large valleys drain from near the lowest present portion of the caldera rim and down the flanks of the volcano. The largest valley debauches into Rahe Crater (an oblique impact crater), forming a depositional fan. Recent study of climate change on Mars suggests that many low-latitude regions (especially large volcanic edifices) were periodically the sites of snow accumulation, likely triggered by variations in spin orbital parameters. We apply a conductive heat flow model to Ceraunius Tholus that suggests that following magmatic intrusion, sufficient heating would be available to cause basal melting of any accumulated summit snowpack and produce sufficient meltwater to cause the radial valleys. The geometry of the volcano summit caldera suggests that meltwater would also accumulate in a volumetrically significant caldera lake. Analysis of the morphology and volumes of the largest valley, as well as depositional features at its base, suggest that fluvial erosion due to drainage of this summit caldera lake formed the large valleys, in a manner analogous to how valleys were formed catastrophically from a lake in Aniakchak caldera in Alaska. Moreover, the event which carved the largest valley on Ceraunius Tholus appears to have led to the formation of a temporary lake within Rahe Crater, at its base. The more abundant, small valleys on the flanks are interpreted to form by radial drainage of melted ice or snow from the outside of the caldera rim. Comparison of Ceraunius Tholus with the volcano-capping Icelandic ice sheet Myrdalsjokull provides insight into the detailed mechanisms of summit heating, ice-cap accumulation and melting, and meltwater drainage. These observations further underline the importance of a combination of circumstances (i.e., climate change to produce summit snowpack and an active period of magmatism to produce melting) to form the valley systems on some martian volcanoes and not on others.  相似文献   

Hydrologic processes at the urban residential scale     

Q. Xiao  E. G. McPherson  J. R. Simpson  S. L. Ustin 《水文研究》2007,21(16):2174-2188

In the face of increasing urbanization, there is growing interest in application of microscale hydrologic solutions to minimize storm runoff and conserve water at the source. In this study, a physically based numerical model was developed to understand hydrologic processes better at the urban residential scale and the interaction of these processes among different best management practices (BMPs). This model simulates hydrologic processes using an hourly interval for over a full year or for specific storm events. The model was applied to treatment and control single‐family residential parcels in Los Angeles, California. Data collected from the control and treatment sites over 2 years were used to calibrate and validate the model. Annual storm runoff to the street was eliminated by 97% with installation of rain gutters, a driveway interceptor, and lawn retention basin. Evaluated individually, the driveway interceptor was the most effective BMP for storm runoff reduction (65%), followed by the rain gutter installation (28%), and lawn converted to retention basin (12%). An 11 m³ cistern did not substantially reduce runoff, but provided 9% of annual landscape irrigation demand. Simulated landscape irrigation water use was reduced 53% by increasing irrigation system efficiency, and adjusting application rates monthly based on plant water demand. The model showed that infiltration and surface runoff processes were particularly sensitive to the soil's physical properties and its effective depth. Replacing the existing loam soil with clay soil increased annual runoff discharge to the street by 63% when climate and landscape features remained unchanged. Copyright © 2006 John Wiley & Sons, Ltd.  相似文献   

Investigating the use of spatial discretization of hydrological processes in conceptual rainfall runoff modelling: a case study for the meso‐scale     

H. Hellebrand  R. van den Bos 《水文研究》2008,22(16):2943-2952

In this study a simple modelling approach was applied to identify the need for spatial complexity in representing hydrological processes and their variability over different scales. A data set of 18 basins was used, ranging between 8 and 4011 km² in area, located in the Nahe basin (Germany), with daily discharge values for over 30 years. Two different parsimoniously structured models were applied in lumped as well as in spatially distributed according to two distribution classifications: (1) a simple classification based on the lithology expressed in three permeability types and (2) a more complex classification based on seven dominating runoff production processes. The objective of the study was to compare the performances of the models on a local and on a regional scale as well as between the models with a view to identifying the accuracy in capturing the spatial variability of the rainfall‐runoff relationships. It was shown that the presence of a specific basin characteristic or process of the distribution classification was not related with higher model performance; only a larger basin size promoted higher model performance. The results of this study also indicated that the permeability generally contained more useful information on the spatial heterogeneity of the hydrological behaviour of the natural system than did a more detailed classification on dominating runoff generation processes. Although model performance was slightly lower for the model that used permeability as a distribution classification, consistency in its parameter values was found, which was lacking with the more complex distribution classification. The latter distribution classification had a higher flexibility to optimize towards the variability of the runoff, which resulted in higher performance, however, process representation was applied inconsistently. Copyright © 2007 John Wiley & Sons, Ltd.  相似文献