土壤中热量传输计算的研究进展与展望   总被引：11，自引：2，他引：9  

张立杰  江灏  李磊 《冰川冻土》2004,26(5):569-575

土壤中热量传输计算的研究分为土壤热通量计算方法和土壤导温率计算方法两方面的成果. 目前已有土壤热通量的计算方法, 在土壤表层可以得到较好结果, 但在土壤深层的适用性无法确定. 多孔介质模型和考虑水的渗流造成的影响, 是多年冻土区土壤导温率的计算方法的研究方面新的进展. 为研究青藏铁路沿线冻土演化趋势找到合适的土壤热量传输计算方案, 应是今后工作的一个重点.  相似文献   

山东东营凹陷古近系碎屑岩储层特征及控制因素   总被引：25，自引：10，他引：15       下载免费PDF全文

张琴  朱筱敏  钟大康  宋刚 《古地理学报》2004,6(4):493-502

通过对大量储层物性数据的分析和整理,结合薄片观察和扫描电镜分析结果,研究了不同构造背景、不同沉积类型及不同埋深的储层物性特征及其控制因素。东营凹陷近系碎屑岩储层类型多样,大多形成在冲积扇-河流、扇三角洲、近岸水下扇、深水浊积扇、三角洲前缘滑塌浊积扇以及滨浅湖滩坝等多种沉积环境中。碎屑岩储层类型主要包括砾岩、含砾砂岩、中粗砂岩、细砂岩及粉砂岩。其中中砂岩和细砂岩是最好的储层。但是不同地区、不同类型储层物性存在较大的差异。物性最好的储层为河道、（扇）三角洲前缘水下分流河道及河口坝砂体。在相同深度条件下,中央隆起带的物性最好,北部和南部次之。另外,本区随埋藏深度增加,碎屑岩储层物性逐渐变差（剔除次生孔隙的影响）。根据碎屑岩储层物性差异性分析和储层成岩演化研究结果,其储层物性主要受压实作用、碳酸盐溶蚀与胶结作用及沉积条件四大因素控制,其中压实作用、溶蚀作用及胶结作用是主要控制因素,而沉积条件对物性的影响主要表现在控制原生孔隙的发育程度,并进一步控制溶蚀、胶结等成岩作用。  相似文献   

The Classification and Model of Coalbed Methane Reservoirs   总被引：8，自引：0，他引：8  

SU Xianbo  LIN Xiaoying  SONG Yan  ZHAO Mengjun Henan University of the Sciences  Jiaozuo  Henan Research Institute of Petroleum Exploration  Development  PetroChin  Beijing 《《地质学报》英文版》2004,78(3):662-666

Coalbed methane has been explored in many basins worldwide for 30 years, and has been developed commercially in some of the basins. Many researchers have described the characteristics of coalbed methane geology and technology systematically. According to these investigations, a coalbed methane reservoir can be defined: "a coal seam that contains some coalbed methane and is isolated from other fluid units is called a coalbed methane reservoir". On the basis of anatomization, analysis, and comparison of the typical coalbed methane reservoirs, coalbed methane reservoirs can be divided into two classes: the hydrodynamic sealing coalbed methane reservoirs and the self-sealing coalbed methane reservoirs. The former can be further divided into two sub-classes: the hydrodynamic capping coalbed methane reservoirs, which can be divided into five types and the hydrodynamic driving coalbed methane reservoirs, which can be divided into three types. The latter can be divided into three types. Currently, hydrodynamic s  相似文献   

Classification of 24 New Ordinary Chondrites from the Grove Mountains, Antarctica   总被引：1，自引：0，他引：1  

LU Ren  MIAO Bingkui  WANG Guiqing  DAI Deqiu  LIN Yangting  OUYANG Ziyuan  LI Chunlai Institute of Geochemistry  Chinese Academy of Sciences  Guiyang  Guizhou  Graduate School  Chinese Academy of Sciences  Beijing Institute of Geology  Geophysics  Chinese Academy of Sciences  Beijing Guangzhou Institute of Geochemistry  Chinese Academy of Sciences  Guangzhou  Guangdong National Astronomical Observatories  Chinese Academy of Sciences  Beijing 《《地质学报》英文版》2004,78(5):1052-1059

Petrography and mineral chemistry of 24 ordinary chondrites from the Grove Mountains, Antarctica, have been studied in order to identify their chemical-petrographic types. These samples were selected from a total of 4448 Grove Mountains (GRV) meteorites collected during the 19th Chinese Antarctic Research Expedition so as to make an estimation of the large GRV meteorite collection. The chemical-petrographic types of these meteorites are presented below: 1 H3,2 H4, 4 H5, 2 H6, 1 L4, 7 L5, 5 L6, 1 LL4 and 1 LL6. The new data weaken the previous report that unequilibrated ordinary chondrites are unusually abundant in the Grove Mountains region. However, this work confirms significant differences in distribution patterns of chemical-petrographic types between the Grove Mountains and other  相似文献   

The brightness of the galactic radio loops at 1420 MHz: Some indications for the existence of Loops V and VI     

V. Borka  J. Milogradov‐Turin  D. Uro&#x;evi&#x; 《Astronomische Nachrichten》2008,329(4):397-402

In this article we use 1420 MHz data to demonstrate the likely reality of Galactic radio Loops V and VI. We further estimate distances and spectral indices for both these and the four main radio loops. In the cases of Loops I–IV, radio spectral indices are calculated from the mean brightnesses at 1420 and 820/404 MHz. The spectral indices of Loops V and VI are obtained from T –T plots between 1420 and 408 MHz. Using the supernova remnant (SNR) hypothesis for the origin of radio loops, distances are calculated from the surface brightnesses and the angular diameters at 1420 MHz. We also study how results for brightnesses and distances of radio loops agree with current theories of SNR evolution. For this purpose, the ambient density and initial explosion energy of the loops are discussed. We also discuss applications of different Σ–D relations. The results obtained confirm a non‐thermal origin and nearby locations for the Galactic radio loops. Therefore, we have indications that they are very old SNRs that evolve in low ambient densities, with high initial explosion energies. (© 2008 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

Venus upper atmospheric CO, temperature, and winds across the afternoon/evening terminator from June 2007 JCMT sub-millimeter line observations     

R.T. Clancy  B.J. Sandor 《Planetary and Space Science》2008,56(10):1344-1354

The Venus mesosphere constitutes a highly variable transition region between the zonal rotation of the lower atmosphere and the diurnal circulation of the upper atmosphere. It further serves as the primary photochemical region of the Venus atmosphere. We obtained James Clerk Maxwell Telescope (JCMT, Mauna Kea Hawaii) sub-millimeter line observations of mesospheric ¹²CO and ¹³CO during coordinated space (MESSENGER and Venus Express) and ground-based observations of Venus in June of 2007. Such CO spectra line measurements support temperature, CO mixing ratio, and wind retrievals over the 80-110 km altitude range, encompassing the upper mesosphere and lower thermosphere of Venus. Five-point beam integrations were obtained across the observed Venus disk, allowing distinction of afternoon (noon to 6 p.m.) versus evening (6 p.m. to midnight) local times and northern (0-60N) versus southern (0-60S) latitudes. Distinctive diurnal variations (noon to midnight) are retrieved for both temperatures above 95 km and CO mixing ratios above 85 km altitudes. Separate CO line maps obtained on (UT) June 2, 3, 6, and 11 indicate moderate daily variability in afternoon and evening CO mixing ratios (20-50%) and temperatures (5-10 K). Average Venus mesospheric temperatures over this period were 10 K warmer than returned from 1978 to 1979 Pioneer Venus or 2000-01 sub-millimeter measurements, without evidence for the very large temperature inversions indicated by Venus Express SPICAV measurements at 90-100 km altitudes (Bertaux, J.L., Vandaele, A.-C., Korablev, O., Villard, E., Fedorova, A., Fussen, D., Quémerais, E., Belyaev, D., Mahieux, A., Montmessin, F., Muller, C., Neefs, E., Nevejans, D., Wilquet, V., Dubois, J.P. Hauchecorne, A., Stepanov, A., Vinogradov, I., Rodin, A., Bertaux, J.-L., Nevejans, D., Korablev, O., Montmessin, F., Vandaele, A.-C., Fedorova, A., Cabane, M., Chassefière, E., Chaufray, J.Y., Dimarellis, E., Dubois, J.P., Hauchecorne, A., Leblanc, F., Lefèvre, F., Rannou, P., Quémerais, E., Villard, E., Fussen, D., Muller, C., Neefs, E., Van Ransbeeck, E., Wilquet, V., Rodin, A., Stepanov, A., Vinogradov, I., Zasova, L., Forget, F., Lebonnois, S., Titov, D., Rafkin, S., Durry, G., Gérard, J.C., Sandel, B., 2007. A warm layer in Venus’ cryosphere and high-altitude measurements of HF, HCl, H₂O and HDO. Nature 450, 646-649). Measured Doppler shifts associated with June 2 and 11 ¹²CO line center absorptions indicate nearly supersonic (200 m/s, Mach 1) afternoon-to-evening (retrograde) circulation; composed of additive subsolar-to-antisolar (SSAS) and zonal retrograde wind components, which are not separable due to the particular observational geometry.  相似文献   

Spatially distributed modelling of soil erosion and sediment yield at regional scales in Spain   总被引：4，自引：0，他引：4  

Joris de Vente  Jean Poesen  Gert Verstraeten  Anton Van Rompaey  Gerard Govers 《Global and Planetary Change》2008,60(3-4):393-415

Initiated by the need to quantify erosion rates and the impacts of global changes on erosion, several attempts have been made to apply erosion models at regional scales. However, these models have often been directed towards on-site soil erosion estimates, emphasising sheet and rill erosion processes, and disregarding gully erosion, channel erosion and sediment transport. These models are therefore of limited use for the assessment of sediment yield, off-site impacts of erosion, and for the development of environmental management to control these impacts at regional scale. This study analyses and compares three spatially distributed models for the prediction of soil erosion and/or sediment yield at regional scales: the WATEM-SEDEM model that is based on the empirical Revised Universal Soil Loss Equation (RUSLE) in combination with a sediment transport equation, the physics-based Pan European Soil Erosion Risk Assessment model (PESERA), and a newly developed Spatially Distributed Scoring model (SPADS). The three models were applied to 61 Spanish drainage basins and model predictions were evaluated against data on measured reservoir sedimentation rates. Global data sets on land use, climate, elevation and soil characteristics were used as model input for WATEM-SEDEM and SPADS, whereas published soil erosion estimates of PESERA at 1 km² resolution were used directly. SPADS and WATEM-SEDEM provided best results after separate calibration for basins with a Sediment Delivery Ratio (SDR) higher than 5% and those with an SDR lower than 5%. In this way, SPADS explained 67% of variation in sediment yield, while WATEM-SEDEM explained 48% of the variation. PESERA represents a promising alternative to the use of empirical models at the regional scale as it can be applied to very diverse environments with little calibration. However, PESERA provides soil erosion rates and not sediment yield estimates. For most basins PESERA soil erosion rates vary between fifty and close to zero percent of total sediment yield. Two major factors may explain this discrepancy between modelled soil erosion rates and measured sediment yield. First, it may be that PESERA underestimates soil erosion under Mediterranean conditions, although PESERA soil erosion rates are of the same order of magnitude as erosion rates measured in erosion plot studies. Second, gully-, river channel erosion and sediment transport processes may be much more important than sheet- and rill erosion for regional scale sediment yield in these environments. These issues therefore require further attention in future model development. Although spatially lumped models provide better predictions of sediment yield at the basin scale, and while validation of the predicted spatial patterns of sources and sinks of sediment requires further research, spatially distributed models are expected to be of value to support management decisions regarding the assessment of on-site and off-site impacts of erosion at the regional scale.  相似文献   

济阳坳陷西部惠民凹陷第三纪火山岩型油藏成藏机理研究   总被引：12，自引：4，他引：8  

初宝杰  向才富  姜在兴  夏斌  于俊峰 《大地构造与成矿学》2004,28(2):201-208

在全面剖析济阳坳陷惠民凹陷第三纪火成岩空间分布规律的基础上 ,对本区火山岩的成藏机理进行了深入研究 ,总结了惠民凹陷火山岩型油气藏的成藏模式。惠民凹陷的主要烃源岩来自于南部的临南洼陷和北部的滋镇洼陷 ,由于本区火成岩主要沿 2个生烃凹陷间隆起带的临邑帚状断裂带展布 ,保证了火山岩带有充足的油源条件。油气运移的输导体系是由渗透性砂岩、断层、裂缝和不整合面的三维空间组合 ,研究区的临邑帚状断裂带、多期发育的裂缝和不整合面对油气向火山岩储层的运移至关重要。储集空间是储层质量好坏的决定因素 ,惠民凹陷的火山岩储层存在各种的原生储集空间 ,同时由于次生的断层活动和火成岩拱张作用形成了丰富的次生储集空间 ,极大地改善了本区火成岩的储层物性 ,是本区形成各类火成岩圈闭和油藏的保证。本区火成岩存在 3种类型的油气藏 ,即火成岩作为储层、火成岩作为盖层或遮挡层以及火成岩侵入动力型油气藏  相似文献   

东营凹陷下第三系层序地层研究与隐蔽油气藏预测   总被引：18，自引：3，他引：15  

张德武  冯有良  邱以钢  闵伟  郭玉新  赵乐强  向立宏 《沉积学报》2004,22(1):67-72

应用层序地层学理论,利用地震、测井、岩心和分析化验资料,建立了东营凹陷下第三系层序界面识别标志,把东营凹陷下第三系划分为 1个超层序组,4个超层序,10个层序,进行体系域划分,建立了东营凹陷下第三系层序地层格架。构造坡折带是指由同沉积构造长期活动引起的沉积斜坡明显突变的地带,对盆地充填的可容纳空间和沉积作用可产生重要影响。通过层序地层格架与构造坡折带的研究,建立东营凹陷层序发育模式。受构造坡折带控制的层序低位域砂体和湖侵体系域砂体,成藏条件良好,最有利于形成隐蔽油气藏。  相似文献   

辽宁省大民屯凹陷流体化学场特征及油气成藏意义   总被引：8，自引：3，他引：5  

史建南  姜建群  李明葵 《地质科技情报》2004,23(1):63-68

从地层水化学场、油气组成的非均质性两方面对辽宁省大民屯凹陷前第三系古潜山和下第三系沙河街组的流体化学场特征进行了分析.结果表明,该区地层水运动规律与油气运移模式吻合较好,即流体以"垂向流动"为主,受断裂和沉积砂体的控制,由沉积中心的中、深部沿断裂垂向运移,而后在各断块内侧向运移至各断块的高部位,横向运移效应只在局部小范围内规律显著,构成了典型的离心状渗流体系.在地层水水头压力、浮力动力场控制下该区形成了自生自储、下生上储、新生古储型油藏.  相似文献