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1.
在地球上,水是生命存在的基础之一.大量证据表明火星表面曾经存在液态水,而目前的火星表面环境不支持液态水的长期存在.因此,水可能以不同的状态赋存于火星的次表层.寻找火星次表层的水一直是火星探测的关键科学目标之一.次表层探测雷达,如探地雷达、探冰雷达,是了解地下物质结构的有效方法,近年来在地外天体上得到大量应用.在过去十余年,欧洲的火星快车(Mars Express)上搭载的火星次表层和电离层探测先进雷达(Mars Advanced Radar for Subsurface and Ionosphere Sounding,MARSIS)和美国火星勘测轨道飞行器(Mars Reconnaissance Orbiter,MRO)上搭载的浅表层雷达(Shallow Subsurface Radar,SHARAD)已在火星轨道上获取了大量数据,被广泛应用于研究火星的地下结构,尤其是地下水冰探测.我国的天问一号火星探测器也携带了高低频轨道探测雷达和高低频火星车探地雷达,有望在不同的顺轨向、交轨向和距离向分辨率上揭示火星次表层不同深部的结构.本文综述了轨道器次表层探测雷达的探测原理和优势,简要介绍了雷达数据的处理和解译方法,重点总结了 MARSIS和SHARAD近年来对火星水冰探测的最新进展,最后对天问一号环绕器雷达及其水冰探测作简要展望. 相似文献
2.
Three-phase numerical model of water migration in partially frozen geological media: model formulation,validation, and applications 总被引：3，自引：0，他引：3
Scott L. Painter 《Computational Geosciences》2011,15(1):69-85
Water in the subsurface of the Earth’s cold regions—and possibly the subsurface of Mars—resides in the liquid, vapor, and
ice phases. However, relatively few simulations addressing full three-phase, nonisothermal water dynamics in below-freezing
porous media have been undertaken. This paper presents a nonisothermal, three-phase approach to modeling water migration in
partially frozen porous media. Conservation equations for water (as ice, liquid, and vapor) and a single gas species (in the
gas phase and dissolved in water) are coupled to a heat transport equation and solved by a finite-volume method with fully
implicit time stepping. Particular attention is given to the method of spatial differencing when the pore space is partially
filled with ice. The numerical model is able to reproduce freezing-induced water redistribution observed in laboratory experiments.
Simulations of Earth permafrost dynamics and of the formation and evolution of a planetary-scale cryosphere on Mars demonstrate
the new capabilities. 相似文献
3.
4.
迄今为止,人类已经通过火星轨道探测器、火星着陆器及火星漫游车在火星上发现了碳酸盐、硫酸盐及氯化物等一 系列的盐类矿物,尽管整体上火星盐类矿物组合与地球上基本一致,但在许多细节方面还是和地球上有所不同。文中首先 对于火星盐类认知的现状作了简要综述;基于地球火星蒸发盐沉积及成盐作用规律的对比,预测火星表面及次表面可能存 在着广泛分布的钾盐;此外,发现火星轨道伽玛光谱仪所获的火星表面 K 的分布与火星表面已探测到的氯化物的分布有比 较强的相关性,喻示火星表面氯化物沉积地区的卤水浓度已经接近或达到钾盐形成的条件,同时指出这些地区存在钾盐的 可能性很大。 相似文献
5.
下边界条件对多年冻土温度场变化数值模拟的影响 总被引：1，自引：1，他引：0
在气候变暖背景下,北半球多年冻土呈现不同程度的退化趋势,冻土升温、活动层增厚、地下冰消融改变了区域工程地质条件、地形地貌,不仅对寒区环境和工程稳定性造成潜在的威胁,还影响着这些地区的气候、水文和生态过程。因此,准确评估和预估多年冻土热状况的变化具有重要科学和实践意义。现有用于模拟多年冻土热状况的各类模式重点考虑了近地表温度场变化对多年冻土的影响,主要集中于对气温和浅表层物理过程和参数化方案等改进和优化,而对于下边界条件设置对多年冻土热状况模拟的影响少有讨论。基于一维热传导冻土模型,以五道梁地区的多年冻土为研究对象,通过设置不同的下边界方案进行模拟实验,定量评估百年尺度气候变化下不同下边界条件对多年冻土温度场变化数值模拟的影响。结果表明：近地表层（<3 m）的温度场完全由年际气候变化决定,浅层（3~15 m）及中层（15~30 m）的多年冻土温度场受下边界条件的影响逐渐显著,深层（>30 m）的地温对百年尺度气候变化的响应不仅与气候变化的幅度有关,还与多年冻土相变热的多少有直接的关系。下边界条件不恰当的设置方式会对大尺度的气候变化下多年冻土消融程度的计算造成较大的影响,进而可能对深层地温乃至多年冻土区面积变化造成严重的误判。因此,开展百年尺度多年冻土温度场变化模拟时,应采用深层或多年冻土底板以下融土层的稳定地热流作为下边界条件。 相似文献
6.
多年冻土地区铁路路基的振动与环境变化对路基稳定性的影响问题日益突出,为了评价这种影响引起的青藏铁路多年冻土区冻土的变化状况,首次应用了一种简便、高效、环保的瞬态面波勘探方法对其天然地表和典型结构路基及其下部多年冻土层进行了勘探。试验数据良好、频散特征显著,通过反演分析得到了青藏高原多年冻土地区天然地表和典型结构路基下部土体的剪切波速度剖面和多年冻土的分布。勘探结果表明,青藏铁路北麓河试验段勘探区内多年冻土上限一般为2 m,层厚为20 m左右,多年冻土层Vs平均为600 m/s以上。该结果与该区地质钻探编录和钻孔波速测试结果较为一致,说明瞬态面波勘探在自然环境严峻的青藏高原多年冻土地区有着良好的适用性。 相似文献
7.
冻结层上水的分布及工程影响研究现状与展望 总被引：1，自引：1，他引：0
作为一种多年冻土区的特殊水文地质现象,冻结层上水（或多年冻土层上水）的分布受局地因素的控制,且随活动层的季节性冻融而变化,影响地表水和地下水循环以及多年冻土环境中的水热平衡。多年冻土将冻结层上水限制在一个狭窄的空间内,在暖季冻结层上水侧向和竖向的渗流传热将加剧多年冻土的退化,也会对上覆工程构筑物的稳定运营造成极大威胁。目前关于冻结层上水的研究主要集中在分布特征、变化规律、流量计算、渗流模拟、水热耦合等方面。研究发现：在全球升温背景下,多年冻土退化速率加剧,随着冻土厚度变薄和融区出现,冻结层上水的流量及其与地下水的交换量均发生变化,除了影响局地水文特征外,还与工程病害密切相关,如坡脚积水、路基沉降以及路面裂缝等。以区域分布特征为出发点,对冻结层上水的研究现状进行了归纳和总结,并对其工程影响有关的渗流传热理论研究成果进行了梳理,对今后需要进行深入研究的方向进行了展望。这有助于全面理解冻结层上水在冻土区水文过程中的功能,为相关研究提供了进一步的理论参考。 相似文献
8.
Ahmad Jan Ethan T. Coon Scott L. Painter Rao Garimella J. David Moulton 《Computational Geosciences》2018,22(1):163-177
Integrated surface/subsurface models for simulating the thermal hydrology of permafrost-affected regions in a warming climate have recently become available, but computational demands of those new process-rich simu- lation tools have thus far limited their applications to one-dimensional or small two-dimensional simulations. We present a mixed-dimensional model structure for efficiently simulating surface/subsurface thermal hydrology in low-relief permafrost regions at watershed scales. The approach replaces a full three-dimensional system with a two-dimensional overland thermal hydrology system and a family of one-dimensional vertical columns, where each column represents a fully coupled surface/subsurface thermal hydrology system without lateral flow. The system is then operator split, sequentially updating the overland flow system without sources and the one-dimensional columns without lateral flows. We show that the app- roach is highly scalable, supports subcycling of different processes, and compares well with the corresponding fully three-dimensional representation at significantly less computational cost. Those advances enable recently developed representations of freezing soil physics to be coupled with thermal overland flow and surface energy balance at scales of 100s of meters. Although developed and demonstrated for permafrost thermal hydrology, the mixed-dimensional model structure is applicable to integrated surface/subsurface thermal hydrology in general. 相似文献
9.
Francis M. McCubbin Nicholas J. Tosca Hanna Nekvasil Marc Fries Donald H. Lindsley 《Geochimica et cosmochimica acta》2009,73(16):4907-318
Low-temperature aqueous processes have been implicated in the generation of jarosite and hematite on the martian surface, but little is known regarding the role that high-temperature magmatic fluids may have played in producing similar assemblages on Mars. We have identified jarosite and hematite in a clinopyroxene-hosted melt inclusion in martian meteorite MIL 03346 that shows evidence of having been hydrothermally precipitated. In addition to jarosite and hematite, the melt inclusion contains titanomagnetite, pyrrhotite, potassic-chlorohastingsite, an iron-rich silicate glass and possibly goethite. These phases were identified and characterized using scanning electron microscopy (SEM), con-focal Raman-spectroscopy and electron probe microanalysis (EPMA).Based on observed textural relationships and the compositions of the hosted phases, we report that the jarosite-bearing melt inclusion in MIL 03346 has recorded a fluid-rich history that began in the magmatic stage and continued to low-temperatures. This history begins at entrapment of a volatile-rich silicate melt that likely reached fluid-saturation after only minor crystallization within the melt inclusion. This fluid, rich in chlorine, reacted with surrounding silicate material to produce the potassic-chlorohastingsite. As cooling proceeded, the liquid phase eventually became more oxidized and reacted with the pyrrhotite. Sulfide oxidation resulted in SO42− formation and concomitant acid production, setting the stage for jarosite formation once the fluid cooled beyond the upper thermal stability of jarosite (∼200 °C). As the fluid cooled below 200 °C, jarosite continued to precipitate with hematite and/or goethite until equilibrium was established or reactions became kinetically unfavorable.This work suggests an additional jarosite-hematite formation pathway on Mars; one that may be important wherever magmatic-hydrothermal fluids come into contact with primary sulfide grains at the martian surface or subsurface. Moreover, hydrothermal fluids rich in chlorine, sulfur, and iron are important for ore-forming processes on Earth, and their indirect identification on Mars may have important implications for ore-formation on Mars. 相似文献
10.
Change dynamics of permafrost thaw, and associated changes in subsurface flow and seepage into surface water, are analysed for different warming trends in soil temperature at the ground surface with a three-phase two-component flow system coupled to heat transport. Changes in annual, seasonal and extreme flows are analysed for three warming-temperature trends, representing simplified climate-change scenarios. The results support previous studies of reduced temporal variability of groundwater flow across all investigated trends. Decreased intra-annual flow variability may thus serve as an early indicator of permafrost degradation before longer-term changes in mean flows are notable. This is advantageous since hydrological data are considerably easier to obtain, may be available in longer time series, and generally reflect larger-scale conditions than direct permafrost observations. The results further show that permafrost degradation first leads to increasing water discharge, which then decreases as the permafrost degradation progresses further to total thaw. The most pronounced changes occur for minimum annual flows. The configuration considered represents subsurface discharge from a generic heterogeneous soil-type domain. 相似文献
11.
应用等效纬度-海拔模型进行地温及多年冻土制图 总被引：2，自引：2，他引：2
KenjiYoshikawa PrasadGogineni 《冰川冻土》2002,24(5):526-531
This research presents a method for permafrost mapping in discontinuous permafrost regions based on equivalent latitude/elevation concept in interior Alaska. In winter months, study site has a strong temperature inversion in air up to 700 m elevation. Air temperature data and the effects of slope, aspect and elevation were used to create an equivalent latitude/elevation model. This model was well correlated with mean annual surface temperature (0.79). In this watershed, the thawing index (It≈1 400 ℃*days) at the ground surface and snow depth do not vary greatly from south facing to north facing slopes. The primary controlled factor that determines the mean annual surface temperature was the winter surface temperature. The permafrost stability is effectively controlled by the freezing index. We determined 37.5% of Caribou-Poker Creeks Research Watershed has unstable or thawing permafrost. At least 2.1% of the permafrost in this watershed may have disappeared in the last 90 years due to climate warming. This method makes it possible to evaluate the permafrost stability in the present, past and future. 相似文献
12.
13.
The active-layer hydrology of a peat plateau with thawing permafrost (Scotty Creek, Canada) 总被引：2，自引：0，他引：2
The southern margin of permafrost is experiencing unprecedented rates of thaw, yet the effect of this thaw on northern water resources is poorly understood. The hydrology of the active layer on a thawing peat plateau in the wetland-dominated zone of discontinuous permafrost was studied at Scotty Creek, Northwest Territories (Canada), from 2001 to 2010. Two distinct and seasonally characteristic levels of unfrozen moisture were evident in the 0.7-m active layer. Over-winter moisture migration produced a zone of high ice content near the ground surface. The runoff response of a plateau depends on which of the three distinct zones of hydraulic conductivity the water table is displaced into. The moisture and temperature of the active layer steadily rose with each year, with the largest increases close to the ground surface. Permafrost thaw reduced subsurface runoff by (1) lowering the hydraulic gradient, (2) thickening the active layer and, most importantly, (3) reducing the surface area of the plateau. By 2010, the cumulative permafrost thaw had reduced plateau runoff to 47 % of what it would have been had there been no change in hydraulic gradient, active layer thickness and plateau surface area over the decade. 相似文献
14.
降雨对青藏高原多年冻土区地表辐射的影响——以北麓河地区为例 总被引：1，自引：0，他引：1
青藏高原地表辐射变化影响多年冻土地表能量收支平衡、热工计算温度场边界条件以及冻土热稳定性。降雨变化是影响地表辐射的重要因素,以青藏高原北麓河地区的地表辐射资料和浅层地表水热监测数据为基础,分析了降雨对多年冻土区地表辐射特征的影响。研究表明：受降雨影响,辐射分量具有明显的日变化和年际变化特征,短波辐射被严重削弱,地面长波辐射削弱程度较低,而太阳长波辐射增强。小雨作用后,太阳短波、地面短波、地面长波辐射日积分量分别减少24.6%、37.9%、4.2%,太阳长波增加了4.3%;中雨作用后,太阳短波、地面短波、地面长波辐射日积分量分别减少32.2%、43.4%、1.7%,太阳长波增加了11.6%;大雨作用后,太阳短波、地面短波、地面长波辐射日积分量分别减少56.3%、65.5%、4.4%,太阳长波增加了10.7%;降雨作用后地表反照率减小,且呈不对称“U”形变化,地表净辐射增加,长期时间尺度上降雨对净辐射影响不明显;降雨对辐射特征的影响程度与降雨强度呈正相关且地表辐射对降雨变化的响应有滞后效应。在暖湿化背景下,冻土热工计算中应考虑降雨对多年冻土区地表能量平衡和水热边界的影响。 相似文献
15.
大兴安岭北部是我国唯一的中高纬度多年冻土区,其水热特征分析对陆气能量交换、生态系统和气候变化等研究有重要意义。基于2011—2020年期间对大兴安岭森林生态站附近的湿地多年冻土开展的气温和0~2 m地温和土壤含水量数据,对大兴安岭湿地多年冻土活动层的水热特征进行了分析。结果表明：湿地多年冻土活动层内地温的变幅随深度减小,且具有滞后性。融化期地表温度高于深层地温,冻结期相反。2012年、2013年、2019年和2020年的平均融化速率分别为0.49、0.61、0.47和0.56 cm·d-1,向上平均冻结速率分别为1.34、2.12、2.58和1.65 cm·d-1。向下平均冻结速率分别为1.69、1.02、3.32和1.00 cm·d-1,最大融化深度分别为78.73、85.65、66.22和74.94 cm。2012年5月—2013年5月期间,土壤未冻水含量随地温变化的拟合关系较好,相关系数大于0.90,且深层拟合效果优于表层。融化期土壤水分变化幅度大,与地温的相关性差,随深度增加相关性减弱。湿地充足的水分为多年冻土的双向冻结提供了条件。研究成果可为大兴安岭湿地多年冻土区的冻融循环、水热耦合机理和模拟研究提供数据基础和理论依据。 相似文献
16.
An accurate assessment of the bulk chemical composition of Mars is fundamental to understanding planetary accretion, differentiation, mantle evolution, the nature of the igneous parent rocks that were altered to produce sediments on Mars, and the initial concentrations of volatiles such as H, Cl and S, important constituents of the Martian surface. This paper reviews the three main approaches that have been used to estimate the bulk chemical composition of Mars: geochemical/cosmochemical, isotopic, and geophysical. The standard model is one developed by Wänke and Dreibus in a series of papers, which is based on compositions of Martian meteorites. Since their groundbreaking work, substantial amounts of data have become available to allow a reassessment of the composition of Mars from elemental data, including tests of the basic assumptions in the geochemical models. The results adjust some of the concentrations in the Wänke–Dreibus model, but in general confirm its accuracy. Bulk silicate Mars has roughly uniform depletion of moderately volatile elements such as K (0.6 × CI), and strong depletion of highly volatile elements (e.g., Tl). The highly volatile elements are within uncertainties uniformly depleted at about 0.06 CI abundances. The highly volatile chalcophile elements are likewise roughly uniformly depleted, but with more scatter, with normalized abundances of 0.03 CI. Bulk planetary H2O is much higher than estimated previously: it appears to be slightly less than in Earth, but D/H is similar in Earth and Mars, indicating a common source of water-bearing material in the inner solar system. K/Th ranges from ∼3000 to ∼5000 among the terrestrial planets, a small range compared to CI chondrites (19,000). FeO varies throughout the inner solar system: ∼3 wt% in Mercury, 8 wt% in Earth and Venus, and 18 wt% in Mars. These differences can be produced by varying oxidation conditions, hence do not suggest the terrestrial planets were formed from fundamentally different materials. The broad chemical similarities among the terrestrial planets indicate substantial mixing throughout the inner solar system during planet formation, as suggested by dynamical models. 相似文献
17.
青藏铁路冻土路基沉降变形现场试验研究 总被引：3，自引：0，他引：3
Based on the field data of ground temperature and roadway settlement observed during the construction of the experimental embankments over permafrost along the Qinghai-Tibetan Railway, this paper discusses the differences of frost process on the roadway surface from that on the natural ground surface, the changes of permafrost table under the roadway embankment, and the peculiarities of roadway settlement. Analyses of the test results show : 1) The differences of the freezing indexes between the roadway surfaces and the natural ground surfaces are less than those of the thawing indexes for all the test sections; 2) Since the measures of permafrost protection were taken, the permafrost tables under the embankments have raised after the roadway was constructed. The minimum is about 0.4 m and the maximum is 1.2 m; 3) the settlements of the roadway are mainly from the compression and creep of the icerich frozen soils under the original permafrost tables and the maximum has reached 6 ～ 8 cm during the first year after the embankments were constructed. Moreover, concerning the processes of roadway settlement, the deformation of the embankments has no obvious trend of attenuation at present. Especially,for the roadway with high embankments, the settlement may reach a remarkable value and much consideration must be given for this problem. 相似文献
18.
东北多年冻土地区地基承载力对气候变化敏感性分析 总被引：1，自引：0，他引：1
近年来,中国东北多年冻土地区正处于显著的增温过程中。由此导致多年冻土逐渐退化,并严重影响到构筑物的稳定性。以0.05 ℃的年平均气温上升率为背景,采用带有相变的传热学有限元方法,对中国东北多年冻土地区不同初始气温条件和不同含冰量类型冻土的地基温度状况以及季节活动层厚度变化进行了模拟;利用温度场有限元数值试验结果和已有承载力试验数据分析了不同类型冻土地基的力学性质对气温变化敏感性,评估了气温变化对各类冻土地基承载力的影响。气候变化对多年冻土地区构筑物稳定性影响程度取决于两个环节：其一,冻土地基温度状况对气候变化的响应;其二,冻土地基力学性质对地基温度变化的敏感性。研究结果表明,冻土地基含冰量和温度状态对其承载力随气温变化的敏感性具有显著的影响。含土冰层地基承载力对气温变化最为敏感,气温变化对高温冻土地区浅层地基承载力以及桩-土冻结强度影响较大;而深基础桩端冻土地基承载力受气候变化影响相对较小。 相似文献
19.
合成孔径雷达差分干涉测量（D-InSAR）技术在多年冻土区地表变形监测中的应用 总被引：2，自引：2，他引：0
多年冻土区地表变形严重影响着区域内生态环境和工程设施的稳定性。合成孔径雷达差分干涉测量（differential interferometric synthetic aperture radar, D-InSAR）技术作为一种新型的空间对地观测技术, 为多年冻土区地表变形监测提供了新方法。通过近20年的不断深入研究, 利用D-InSAR技术的多年冻土区地表变形监测取得了大量研究成果。首先介绍了D-InSAR技术测量地表变形的理论基础, 进而概述了D-InSAR技术在多年冻土区地表变形测量中的应用现状, 然后总结了D-InSAR测量过程中存在的关键问题及可能的解决方法。在此认识和分析的基础上, 对D-InSAR技术今后在多年冻土区地表变形监测中的发展方向进行了探讨, 以期为D-InSAR技术在多年冻土区地表变形监测中的推广应用和深入研究提供参考。 相似文献
20.
青藏铁路碎石护坡-热管复合措施的补强效果研究 总被引：2，自引：1，他引：1
青藏铁路高温冻土区的普通路基和保温材料路基均处于热不稳定状态, 需要对它们增设碎石护坡-热管复合措施来强化处理, 新增设的补强措施对路基下部冻土的保护效果如何是人们极为关心的问题. 因此, 对北麓河高温高含冰量路段增设了碎石护坡及热管的复合补强措施后路基下部土体的热状态进行观测.结果显示:普通路基在增设补强措施后, 人为冻土上限进一步抬升, 阴阳坡下均出现显著的降温趋势, 且路基下温度场逐渐趋于对称, 降温范围逐渐向路基中心及深部发展, 路堤中心深部地温仍处于增温状态, 但增温趋势明显缓减; 保温材料路基在增设补强措施后, 人为冻土上限也进一步的抬升至保温板附近, 融化夹层在2个冻融周期后消失, 路堤中心温度在2个冻融周期后出现了降温趋势. 这些效果说明, 补强措施在调控路基内部及下部多年冻土温度时发挥了积极作用. 相似文献