罗布泊北部地区凝结水对地下水补给作用的模拟   总被引：2，自引：0，他引：2  

余绍文  孙自永  周爱国  龚绪龙 《地质科技情报》2011,30(6):116-121

在含盐量较高的罗布泊北部凹地,采用称重法进行了凝结水的野外监测.利用凝结水的观测资料,基于HYDRUS_1D软件,建立了一维饱和―非饱和模型来模拟预测凝结水对地下水的补给作用.研究结果表明:观测期间试筒质量多为减少,仅有3个时段试筒质量增加,表明在这3个时段有凝结水生成;凝结水对包气带的补给量占包气带水分总收入的50....  相似文献   

干旱区凝结水研究进展   总被引：5，自引：0，他引：5  

庄艳丽  赵文智 《地球科学进展》2008,23(1):31-38

凝结水是维系干旱、半干旱地区主要食物链的水分来源之一,具有重要的生态意义。较详细地列举了目前国内外在干旱区测定凝结量及其持续时间所采用的研究方法,从凝结水的数量特征以及时间格局两方面阐述了不同地域凝结水的时空差异性,并从气象因素、凝结面的类型及其位置、周边植被对其作用等方面综合分析了影响凝结水发生的主要因素,探讨了干旱区凝结水的生态作用及其意义,展望了干旱区凝结水未来的研究趋势。提出在未来的干旱区凝结水研究中应加强与气象学、生态学等多学科的交叉,从能量平衡角度加强对凝结水量的研究;同时,改进和规范凝结水的测量方法,开展荒漠植被对凝结水的生理响应研究以及凝结水对极端干旱胁迫植物的作用研究。  相似文献   

雾水的D和¹⁸O同位素研究进展   总被引：1，自引：0，他引：1  

孙自永  程国栋  马瑞  甘义群 《地球科学进展》2008,23(8):794-802

凝结水的D、¹⁸O同位素研究目前主要集中在雾水方面,露水和土壤吸附水的相关研究仍属空白。由于形成时的温度较高,大多数雾水的D、¹⁸O同位素较当地雨水富集,但不同类型雾的同位素特征存在差异。平流式海洋雾为单级的蒸发—冷凝封闭循环系统的首次凝结,D、¹⁸O同位素较当地雨水显著富集;热带云雾林中的地形雾与降雨同时发生,且水分源于同一云团,δD、δ¹⁸O值差异较小;内陆辐射雾因部分水汽源于当地水分的再循环,过量氘和δD、δ¹⁸O值高于降雨。目前有少量研究用D、¹⁸O同位素指示雾水对植被、地下水和地表径流的补给作用,但以定性分析为主,基于端元混合模型的定量评价极少。露水和土壤吸附水的稳定同位素研究是干旱区凝结水研究的重要方向;D、¹⁸O同位素与其它同位素或化学指标的结合有助于促进凝结水生态水文效应的研究进展;短间隔、高密度的长期观测和用于稳定同位素分析的凝结水采样器的设计是需要进一步开展的工作。  相似文献   

Early stage of critical clusters growth in phenomenological and molecular dynamics simulation models     

Romuald Puzyrewski  Jaros&#x;aw Rybicki  Micha&#x; Bia&#x;oskrski 《Atmospheric Research》2006,82(3-4):465

The growth of critical clusters is discussed in the paper according to the classical and molecular dynamics (MD) approaches. A new formula for molecule numbers in critical clusters has been derived within the framework of the classical approach. A set of equations controlling the early stage of growth in a neighborhood of a critical size is presented. As far as molecular dynamics simulation is concerned, a computational technique based on the DL_POLY code is described in brief. Computation results are presented concerning cluster formation of H₂O vapor, distribution of clusters versus time, cluster growth and radial density distribution of isolated clusters. A comparison with the classical results is made for a case of dense vapor, where the mechanism of strong condensation is predominant. The Hertz–Knudsen formula seems to be verified by the molecular dynamics results.  相似文献   

Quantitative Evaluation of Water Deposited By Dew on Monuments   总被引：1，自引：0，他引：1  

Dario Camuffo  Roberta Giorio 《Boundary-Layer Meteorology》2003,107(3):655-672

Samples of White and Green Carrara marble, and three types oflimestone and brick exposed in the field vertically and horizontally were used to evaluate condensationon monuments during clear sky nights. Experiments in a simulation chamber under controlledconditions led to a general equation for the actual amount of water deposited on a surface by dew.This is determined by: How much and for how long the surface temperature falls below the dew point,the moisture content in the air and the ventilation. On clear nights, the condensation on buildingstructures facing the sky may reach some 0.2 kg m^-2 (or 0.2 mm), whereas condensation on verticalsurfaces is very small. Computation of the seasonal trend of night-time condensationshowed that the maximum amount of water condensed per night occurs in the autumn, with the moreabundant concentration of moisture in the air. The total amount of water condensed per month isfound to be a maximum in the summer-autumn period. Morning condensationfor the thermal inertia of monuments is also relevant, and has been calculated to reach the same order of magnitude as thenocturnal dew. A detailed analysis of the temperature and mixing ratio profiles near a condensingsurface has shown two different situations. In still air, the two profiles follow an exponentiallaw and the thermal and the concentration layers lie within a few tens of millimetres. Inthe presence of turbulence, the thickness of these two layers is dramatically reduced. In still air, infront of a vertical, chilly surface, the deposition rate of air pollutants by thermophoresis and/orStefan flow is increased by 3 or 4 times in comparison with a horizontal surface. In the presence ofturbulence, the thickness of the thermal and concentration layers was dramatically reduced, makingthese two kinds of deposition much faster.  相似文献   

A new aspect of condensation theory     

James W. Telford  Steven K. Chai 《Pure and Applied Geophysics》1980,118(2):720-742

This paper examines the effects of the mixing of dry air into a cloud top from the point of view of the droplet spectra. It is shown theoretically that the resulting cycling of the air up and down in the cloud, as seems to be the essential mechanism by which cumuli have been diluted to their observed liquid water mixing ratio, can double the largest drop radius and generate cloud parcels containing drops of all sizes up to this maximum. These changes in the droplet distribution with size occur by a process which is not greatly influenced by the cloud condensation nuclei or the details of droplet growth since maritime like spectra can develop in continental type cumuli. It shows that large numbers of cloud condensation nuclei should not have much effect in inhibiting the rainforming process by reducing coalescence growth. On the contrary, the controlling parameters which determine precipitation efficiency and times seem to be those which control the mixing.  相似文献   

Amoeboid olivine aggregates and related objects in carbonaceous chondrites: records of nebular and asteroid processes     

Alexander N. Krot  Michail I. Petaev  Shoichi Itoh  Timothy J. Fagan  Hisayoshi Yurimoto  Michael K. Weisberg  Matsumi Komatsu  Klaus Keil 《Chemie der Erde / Geochemistry》2004,64(3):185-239

Amoeboid olivine aggregates (AOAs) are the most common type of refractory inclusions in CM, CR, CH, CV, CO, and ungrouped carbonaceous chondrites Acfer 094 and Adelaide; only one AOA was found in the CB_b chondrite Hammadah al Hamra 237 and none were observed in the CB_a chondrites Bencubbin, Gujba, and Weatherford. In primitive (unaltered and unmetamorphosed) carbonaceous chondrites, AOAs consist of forsterite (Fa_<2), Fe, Ni-metal (5-12 wt% Ni), and Ca, Al-rich inclusions (CAIs) composed of Al-diopside, spinel, anorthite, and very rare melilite. Melilite is typically replaced by a fine-grained mixture of spinel, Al-diopside, and ±anorthite; spinel is replaced by anorthite. About 10% of AOAs contain low-Ca pyroxene replacing forsterite. Forsterite and spinel are always ¹⁶O-rich (δ^17,18O∼−40‰ to −50‰), whereas melilite, anorthite, and diopside could be either similarly ¹⁶O-rich or ¹⁶O-depleted to varying degrees; the latter is common in AOAs from altered and metamorphosed carbonaceous chondrites such as some CVs and COs. Low-Ca pyroxene is either ¹⁶O-rich (δ^17,18O∼−40‰) or ¹⁶O-poor (δ^17,18O∼0‰). Most AOAs in CV chondrites have unfractionated (∼2-10×CI) rare-earth element patterns. AOAs have similar textures, mineralogy and oxygen isotopic compositions to those of forsterite-rich accretionary rims surrounding different types of CAIs (compact and fluffy Type A, Type B, and fine-grained, spinel-rich) in CV and CR chondrites. AOAs in primitive carbonaceous chondrites show no evidence for alteration and thermal metamorphism. Secondary minerals in AOAs from CR, CM, and CO, and CV chondrites are similar to those in chondrules, CAIs, and matrices of their host meteorites and include phyllosilicates, magnetite, carbonates, nepheline, sodalite, grossular, wollastonite, hedenbergite, andradite, and ferrous olivine.Our observations and a thermodynamic analysis suggest that AOAs and forsterite-rich accretionary rims formed in ¹⁶O-rich gaseous reservoirs, probably in the CAI-forming region(s), as aggregates of solar nebular condensates originally composed of forsterite, Fe, Ni-metal, and CAIs. Some of the CAIs were melted prior to aggregation into AOAs and experienced formation of Wark-Lovering rims. Before and possibly after the aggregation, melilite and spinel in CAIs reacted with SiO and Mg of the solar nebula gas enriched in ¹⁶O to form Al-diopside and anorthite. Forsterite in some AOAs reacted with ¹⁶O-enriched SiO gas to form low-Ca pyroxene. Some other AOAs were either reheated in ¹⁶O-poor gaseous reservoirs or coated by ¹⁶O-depleted pyroxene-rich dust and melted to varying degrees, possibly during chondrule formation. The most extensively melted AOAs experienced oxygen isotope exchange with ¹⁶O-poor nebular gas and may have been transformed into magnesian (Type I) chondrules. Secondary mineralization and at least some of the oxygen isotope exchange in AOAs from altered and metamorphosed chondrites must have resulted from alteration in the presence of aqueous solutions after aggregation and lithification of the chondrite parent asteroids.  相似文献   

卫星观测的OLR对夏季青藏高原月雨量及凝结潜热的估算   总被引：9，自引：7，他引：9  

徐国昌  蒋尚城 《高原气象》1990,9(3):256-264

本文用美国NOAA1974年6月—1984年5月(其中1978年3—12月缺测)2.5×2.5经纬度网格月平均OLR资料,以及同期青藏高原上83个站的月总降水量资料,分析发现在夏季(6—9月)两者在空间和年际变化上都有密切的负相关,而地面测站数量和高山积雪对上述相关系数的影响较小。分区求得的回归方程,可以较好地估算高原雨季的平均降水量及相应的总潜热。  相似文献   

Meteorology and haze structure during AGASP-II,Part 1: Alaskan Arctic flights, 2–10 April 1986     

G. A. Herbert  R. C. Schnell  H. A. Bridgman  B. A. Bodhaine  S. J. Oltmans  G. E. Shaw 《Journal of Atmospheric Chemistry》1989,9(1-3):17-48

The second Arctic Gas and Aerosol Sampling Program (AGASP-II) was conducted across the Alaskan and Canadian Arctic in April 1986, to study the in situ aerosol, and the chemical and optical properties of Arctic haze. The NOAA WP-3D aircraft, with special instrumentation added, made six flights during AGASP-II. Measurements of wind, pressure, temperature, ozone, water vapor, condensation nuclei (CN) concentration, and aerosol scattering extinction (b_sp) were used to determine the location of significant haze layers. The measurements made on the first three flights, over the Arctic Ocean north of Barrow and over the Beaufort Sea north of Barter Island, Alaska are discussed in detail in this report of the first phase of AGASP II. In the Alaskan Arctic the WP-3D detected a large and persistent region of haze between 960 and 750 mb, in a thermally stable layer, on 2, 8, and 9 April 1986. At its most dense, the haze contained CN concentrations >10,000 cm^–3 and b_sp of 80×10^–6 m^–1 suggesting active SO₂ to H₂SO₄ gas-to-particle conversion. Calculations based upon observed SO₂ concentrations and ambient relative humidities suggest that 10⁴–10⁵ small H₂SO₄ droplets could have been produced in the haze layers. High concentrations of sub-micron H₂SO₄ droplets were collected in haze. Ozone concentrations were 5–10 ppb higher in the haze layers than in the surrounding troposphere. Outside the regions of haze, CN concentrations ranged from 100 to 400 cm^–3 and b_sp values were about (20–40)×10^–6 m^–1. Air mass trajectories were computed to depict the air flow upwind of regions in which haze was observed. In two cases the back trajectories and ground measurements suggested the source to be in central Europe.  相似文献   

玻色-爱因斯坦凝聚和重力测量——2001年诺贝尔物理学奖评介   总被引：6，自引：0，他引：6  

张昌达 《地质科技情报》2001,20(4):107-110

介绍了2001年诺贝尔物理学奖获得者康奈尔，韦曼，克特勒的科学研究成果，实验玻色－爱因斯坦凝聚（BEC）及其在理论上的意义和应用前景，讨论了BEC在研制高精度重力仪方面的应用问题，为此回顾了重力测量现状，朱棣文等研制的原子干涉重力仪和ClauserJ提出的物质波干涉重力仪，分析表明，如果利用BEC，则重力仪的测量精度在朱棣文等工作基础上将会有很大的提高。  相似文献