Transport properties of low-sanidine single-crystals, glasses and melts at high temperature     

Maik Pertermann  Alan G. Whittington  Anne M. Hofmeister  Frank J. Spera  John Zayak 《Contributions to Mineralogy and Petrology》2008,155(6):689-702

Thermal diffusivity (D) was measured using laser-flash analysis from oriented single-crystal low-sanidine (K_0.92Na_0.08Al_0.99Fe³⁺ _0.005Si_2.95O₈), and three glasses near KAlSi₃O₈. Viscosity measurements of the three supercooled liquids, in the range 10^6.8 to 10^12.3 Pa s, confirm near-Arrhenian behavior, varying subtly with composition. For crystal and glass, D decreases with T, approaching a constant near 1,000 K: D _sat ∼ 0.65 ± 0.3 mm² s⁻¹ for bulk crystal and ∼0.53 ± 0.03 mm² s⁻¹ for the glass. A rapid decrease near 1,400 K is consistent with crossing the glass transition. Melt behavior is approximated by D = 0.475 ± 0.01 mm² s⁻¹. Thermal conductivity (k _lat) of glass, calculated using previous heat capacity (C _P) and new density data, increases with T because C _P strongly increases with T. For melt, k _lat reaches a plateau near 1.45 W m⁻¹ K⁻¹, and is always below k _lat of the crystal. Melting of potassium feldspars impedes heat transport, providing positive thermal feedback that may promote further melting in continental crust.  相似文献   

The significance of meteorite density and porosity   总被引：2，自引：1，他引：1  

G.J. Consolmagno  D.T. Britt  R.J. Macke 《Chemie der Erde / Geochemistry》2008,68(1):1-29

Non-destructive, non-contaminating, and relatively simple procedures can be used to measure the bulk density, grain density, and porosity of meteorites. Most stony meteorites show a relatively narrow range of densities, but differences within this range can be useful indicators of the abundance and oxidation state of iron and the presence or absence of volatiles. Typically, ordinary chondrites have a porosity of just under 10%, while most carbonaceous chondrites (with notable exceptions) are more than 20% porous. Such measurements provide important clues to the nature of the physical processes that formed and evolved both the meteorites themselves and their parent bodies. When compared with the densities of small solar system bodies, one can deduce the nature of asteroid and comet interiors, which in turn reflect the accretional and collisional environment of the early solar system.  相似文献   

288.15 K-323.15 K下氯化锂、硫酸锂溶液的密度及摩尔体积研究          下载免费PDF全文

马修臻  胡斌  高丹丹  李武  董亚萍 《盐湖研究》2017,25(4):32-32

用振荡管密度计测定了常压下,温度在288.15-323.15 K范围内不同离子强度的LiCl和 Li₂SO₄溶液的密度,计算了两种锂盐在不同温度下的表观摩尔体积,溶液的浓度范围分别为(0.1~18.9) mol·kg-1及(0.03~3.0)mol·kg-1。用Pitzer离子相互作用模型拟合了LiCl和Li₂SO₄不同温度下的的Pitzer单电解质体积参数,模型的计算值与实验值相吻合良好。  相似文献   

乌鲁木齐河源雪密度观测研究   总被引：15，自引：0，他引：15  

杨大庆  张寅生 《地理学报》1992,47(3):260-266

乌鲁木齐河源高山区积雪形成期(10月)积雪层的月平均密度为140kg/m~3,稳定积雪前期(11—2月)和稳定积雪后期(3—4月)雪层的月平均密度分别为190—210kg/m~3和175kg/m~3,非稳定积雪期(5—9月)的新雪密度介于90—125kg/m~3,平均值为112kg/m~3。统计分析表明,冬季积雪层的平均密度不随积雪深度而变化,但与5日平均气温和5日合计降水量呈反相关关系,夏季新雪的密度随雪深的增大而上升,风速对冬季积雪层平均密度和夏季新雪密度均无明显影响作用。  相似文献   

Density‐Dependent Effects in Jehlius cirratus (Darwin, 1854) (Cirripedia: Chthamalidae) under Different Growth Conditions     

Daniel A. Lpez  María L. Gonzlez 《Marine Ecology》2003,24(4):289-302

Abstract. We analyse the effects of crowding (‘hummocking’) on the growth, reproduction and mortality of the chthamaloid barnacle Jehlius cirratus ( Darwin, 1854 ) on the coast of Chile. Recruitment intensity, ranging from solitary individuals to dense groups, generates different growth conditions. Density‐dependent effects are reflected in the shape, growth parameters, fecundity, sexual maturity and mortality of solitary and crowded specimens. The skewing of size distribution during growth was not significant at the beginning of the growth period, irrespective of initial density. Nevertheless, skewness in size increased with time, both at high and low densities, indicating that the dominance and suppression exerted by larger specimens over smaller ones generate a density‐dependent effect on size during growth. Mortality was greatest when high‐density recruitment occurred immediately before the period when water temperature and food quantity are highest (spring), when it is assumed that growth is greatest; this seasonal effect was not detected at lower levels of recruitment density. Similarly, no differences in mortality were detected between recruitment densities during the period when temperatures are lowest (autumn) and growth is probably slower. In the middle‐high intertidal zone, where J. cirratus co‐exists with Notochthamalus scabrosus ( Darwin, 1854 ), the proportion of dead J. cirratus specimens was directly related both to the relative abundance of N. scabrosus and the total barnacle density. Although the mortality of J. cirratus was density dependent, the increase in the number of N. scabrosus towards the lower section of the middle intertidal zone could have a greater effect on J. cirratus mortality than intra‐specific competition.  相似文献   

浮游植物密度和池水透明度对中国对虾增长速率的影响   总被引：1，自引：1，他引：1       下载免费PDF全文

矫晓阳 《海洋科学》1993,17(4):65-67

1991年6月20日～9月11日,于大连市营城子镇东小磨对虾养殖场3号虾池采水样,固定后,检测浮游植物数量,同时测定透明度和对虾体长。实验结果见图1、图2,表1。结果表明,浮游植物密度、池水透明度和对虾体长增长速率三者之间有着密切的相互关系。  相似文献   

Meiobenthos in Nha trang bay of the south China sea (Vietnam)   总被引：1，自引：0，他引：1  

Olga N. Pavlyuk  Julia A. Trebukhova 《Ocean Science Journal》2006,41(3):139-148

The distribution of the taxonomical composition and the density of meiobenthos depending on the sediment type has been studied in bottom sediments of Nha Trang Bay. The maximal population density and the taxonomical diversity were observed in the silted coarse and heterogeneous sand (1031.4μ419.7 ind. 10 cm^-2), whereas the minimal level of density and diversity (588.1μ152.5 ind. 10 cm^-2) was in the coarse and heterogeneous sand with shell debris and corals. The correlation between the median diameter of sediment particles and population density of meiobenthos has been revealed (r=0.82, p<0.05). In bottom sediments of Nha Trang Bay, twenty six taxonomic groups of meiobenthos were observed. Nematodes dominated in all sediment types. Representatives of four orders, twenty eight families and ninety seven genera of marine nematodes were identified. The vertical distribution of meiobenthos in different sediment types was considered. A sediment column (10 cm height) was sectioned by five 2 cm portions. In the last layer (8-10 cm) the most number of meiobenthic groups was found in sandy sediments. In the lower layers of silt sediments, only nematodes were found.  相似文献   

密度孔压静力触探的测试理论和工程应用综述     

加瑞  赵栋 《工程地质学报》2022,30(1):270-280

孔压静力触探试验(CPTU)是目前使用最为广泛的原位测试方法之一,但CPTU不能原位测量土体最基本的指标——密度。密度孔压静力触探试验(DCPTU)是把核子密度仪结合到孔压静力触探系统中,贯入过程中可以同时测量锥尖阻力、侧壁摩阻力、孔隙水压力和密度的一种新型原位测试方法。本文首先介绍了DCPTU的试验装置和密度测试理论;然后通过与室内试验结果对比评价了利用DCPTU测量砂土、黏土、填土地层以及海底淤泥的密度的可靠性,分析了非均质地层中DCPTU测量密度与真实密度的区别、并提出了真实密度剖面的推求方法;然后综述了DCPTU在判别软弱夹层、评价砂土的液化势、检验地基处理效果、检测块状填土中的空隙、调查浮泥层的厚度和密度分布等方面的工程应用;最后展望了DCPTU在工程勘察中的发展趋势和应用前景。  相似文献   

基于GEOROC大数据分析地壳厚度地球化学指标     

葛粲  汪方跃  李永东  李晓晖  李修钰  周宇章  袁峰  李建设  陆三明 《岩石学报》2018,34(11):3179-3188

前人研究认为,火山岩中部分地球化学指标与岩浆弧地壳厚度之间存在一定的相关性,并通过统计主量元素K2O、Ca O和Na2O指标及微量元素Ce/Y、Sm/Yb、Dy/Yb、Sr/Y、La/Yb指标与地壳厚度之间关系,约束地质史上某些区域的地壳厚度发展和变化。本文基于GEOROC数据库,以Si O2含量57%和火山岩年龄23Ma为界,将全球火山岩数据分成年轻-壳源( 57%,23Ma)、年轻-幔源(57%,23Ma)、古老-壳源( 57%, 23Ma)和古老-幔源(57%, 23Ma)四个数据集,并通过核函数估计方法获得了各个地球化学指标与地壳厚度的归一化联合概率密度分布图。本文统计结果表明,年轻-幔源火山岩中的K2O含量分布与壳源火山岩呈现指数正相关关系、Ca O含量分布于地壳厚度呈现线性负相关关系,年轻-壳源火山岩中Ce/Y、La/Yb和Sm/Yb与现今地壳厚度有指数正相关关系。由以上5种地化指标建立的回归方程确定系数R2均大于0. 7,可以认为相关关系显著。本文认为幔源岩浆在穿透地壳到达地表过程中,地壳厚度控制了富K壳源物质进入地幔熔体和富Ca矿物结晶分异过程,导致了火山岩中K2O和Ca O含量的相关变化;而下地壳部分熔融形成的壳源岩浆,不同深度压力控制了残留相矿物比例,导致Ce/Y、La/Yb和Sm/Yb体现出与地壳厚度的相关性。本文建立的回归函数是基于大量数据概率密度分布的统计分析得出的,由于离群数据普遍存在,回溯历史地壳厚度变化需要大量数据统计支撑,否则难以获得可靠的结果。  相似文献   

Prediction of satellite orbits contraction due to diurnally varying oblate atmosphere and altitude-dependent scale height using KS canonical elements     

Xavier James Raj 《Planetary and Space Science》2009,57(11):1312-1320

A new non-singular analytical theory for the motion of near-Earth satellite orbits with the air drag effect is developed in terms of uniformly regular KS canonical elements. Diurnally varying oblate atmosphere is considered with variation in density scale height dependent on altitude. The series expansion method is utilized to generate the analytical solutions and terms up to fourth-order terms in eccentricity and c (a small parameter dependent on the flattening of the atmosphere) are retained. Only two of the nine equations are solved analytically to compute the state vector and change in energy at the end of each revolution, due to symmetry in the equations of motion. The important drag perturbed orbital parameters: semi-major axis and eccentricity are obtained up to 500 revolutions, with the present analytical theory and by numerical integration over a wide range of perigee height, eccentricity and inclination. The differences between the two are found to be very less. A comparison between the theories generated with terms up to third- and fourth-order terms in c and e shows an improvement in the computation of the orbital parameters semi-major axis and eccentricity, up to 9%. The theory can be effectively used for the re-entry of the near-Earth objects, which mainly decay due to atmospheric drag.  相似文献