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981.
由于冰雪的存在及缺乏地面观测站点资料,高寒地区的水文模拟研究一直面临很大的困难。遥感数据能够提供大范围时空尺度上的地面信息对无资料地区有很大帮助。MODIS数据具有较高的时空分辨率深受人们关注。本文以长江上游泥曲流域为例,探求将MODIS遥感数据与地面气温数据相结合对新安江模型径流模拟的帮助,方法步骤如下:(1)建立MODIS雪覆盖面积与流域周围站气温关系,获取气温阈值;(2)依据气温阈值判别降水形式并计算融雪水当量;(3)将雨雪分离后的降水信息输入新安江模型模拟径流,并与新安江模拟结果(未考虑雨雪分离)和实测径流进行比较。研究结果显示改进方案(考虑雨雪分离)模拟效果更好,将有助于提高新安江模型在高寒无资料地区的径流模拟精度,为高寒无资料地区水资源管理及生态需水研究提供帮助。 相似文献
982.
Jonny Rutqvist Deborah Barr Jens T. Birkholzer Kiyoshi Fujisaki Olaf Kolditz Quan-Sheng Liu Tomoo Fujita Wenqing Wang Cheng-Yuan Zhang 《Environmental Geology》2009,57(6):1347-1360
This paper presents an international, multiple-code, simulation study of coupled thermal, hydrological, and mechanical (THM)
processes and their effect on permeability and fluid flow in fractured rock around heated underground nuclear waste emplacement
drifts. Simulations were conducted considering two types of repository settings (1) open emplacement drifts in relatively
shallow unsaturated volcanic rock, and (2) backfilled emplacement drifts in deeper saturated crystalline rock. The results
showed that for the two assumed repository settings, the dominant mechanism of changes in rock permeability was thermal–mechanically
induced closure (reduced aperture) of vertical fractures, caused by thermal stress resulting from repository-wide heating
of the rock mass. The magnitude of thermal–mechanically induced changes in permeability was more substantial in the case of
an emplacement drift located in a relatively shallow, low-stress environment where the rock is more compliant, allowing more
substantial fracture closure during thermal stressing. However, in both of the assumed repository settings in this study,
the thermal–mechanically induced changes in permeability caused relatively small changes in the flow field, with most changes
occurring in the vicinity of the emplacement drifts. 相似文献
983.
二次光化学氧化剂与气溶胶间的非均相过程 总被引:5,自引:0,他引:5
光氧化剂和气溶胶颗粒物在大气环境中普遍存在,影响着大气氧化能力和气候,威胁着人类健康。而大气光氧化剂与气溶胶颗粒物间复杂的耦合相互作用能产生二次污染物,使得大气污染过程更为复杂,成为国际大气化学研究的前沿和热点课题。挥发性有机物(VOCs)和氮氧化物(NOx)等一次污染物在大气中经过复杂的光化学反应可形成以臭氧(O3)为主的二次光化学氧化剂,并以大气气溶胶为平台发生非均相反应,使大气污染更严重,引起人们普遍关注。二次光化学氧化剂和气溶胶颗粒物之间非均相过程的实验室研究是深入认识这两者间耦合相互作用的关键,实验室研究可以为分析和深入认识外场观测结果提供基础,还能为数值模式模拟研究提供基本参数。概括了大气二次光化学氧化剂的形成过程,总结了国际上近年来二次光化学氧化剂与大气气溶胶颗粒物非均相反应的实验室研究进展以及研究方法,最后提出了现有的一些主要科学问题,对未来这一重要领域的研究前景进行了展望。 相似文献
984.
利用三维强风暴动力-电耦合模式,数值模拟了风暴演变过程 中电活动对冰雹增长及地面降雹的影响. 结果指出,带电冰雹与云内强电场作用使地面降雹 量增加约50[HTK]髎[HTSS],雹块直径增大0.7mm,降雹时间滞后约3min. 文中还讨论了强电 场通过对水成物降落速度的调制来影响冰雹微观增长过程,即主要是影响碰并过程和冰雹融 化过程. 电活动使冰雹源、汇总量都减少,但汇总量减少更多,总体效果使冰雹总量增加, 数目减少,冰雹长得更大,更易降落到地面. 相似文献
985.
1 INTRODUCTION In recent years, due to the increase in population and industrial developments, mankind has faced manyproblems associated with rivers, coastal waters and reservoirs. Some of these problems are flood control,water supply, power generation, and irrigation. In addition, making new hydraulic structures changesnatural conditions. Prediction of these changes is necessary for designing such constructions. For solutionof these problems usually an assessment of flow pattern, sedim… 相似文献
986.
The Sequence of Magmatic-Tectonic Events and Orogenic Processes of the Yanshan Belt, North China 总被引:11,自引:0,他引:11
DENG Jinfu SU Shangguo MO Xuanxue ZHAO Guochun XIAO Qinghiu JI Guangyi QIU Ruizhao ZHAO Hailing LUO Zhaohu WANG Yang LIU Cui China University of Geosciences Beijing and Key Laboratory of Lithospheric Tectonics Lithoprobe Techniques Ministry of Education of China 《《地质学报》英文版》2004,78(1):260-266
This paper emphasizes that the interactive constraints of geology and isotopic dating is the best approach to construct the geological event sequence, and has compiled 106 data of reasonable isotopic ages for the igneous rocks of the Yanshan belt. We propose a sequence of mgmatic-tectonic events in the Jurassic-Cretaceous Yanshan orogen of North China. Five orogenic episodes are divided, (1) pre-and initial orogenic episode (Early Jurassic); (2) early orogenic episode (Middle Jurassic); (3) peak orogenic episode (Late Jurassic); (4) late orogenic episode (early Early Cretaceous), and (5) post-orogenic episode. Each episode is a short cycle, all of the orogenic processes construct a longer cycle, and they, in general, followed a counter-clockwise (ccw) PTt path. Finally, it is suggested that the Yanshanian movement was so intensive that the magmatism and tectonic deformation had involved all the lithosphere thickness and the late-Achaean-formed cratonic lithosphere had been significantly reworked. 相似文献
987.
流体包裹体中微量气体组成及其成矿示踪体系研究新进展 总被引:2,自引:0,他引:2
N2 Ar He体系可用以示踪成矿流体及温泉等与火山有关的水流体的来源 ,当体系中He含量低于检出限 ,N2 Ar He体系不能用时 ,CO2 /CH4 N2 /Ar体系可用于识别成矿流体中岩浆水、建造水和大气降水 ,CO2 CH4 H2 体系可以鉴别成矿流体是否发生过沸腾作用以及沸腾是在开放体系还是封闭体系中形成 ,一般开放体系中沸腾有利于成矿。CO2 CH4 C2 H6体系可用于判别岩浆作用是否直接影响成矿或对成矿流体的贡献 ,从而确定热液矿床的成因。CH4 C2 H6 C3 H8体系可用来示踪一些与干酪根热解有关的成矿流体长距离、大规模迁移过程。C2 H6 C3 H8 C6H6体系可用于判定成矿流体的大地构造环境 ,因岛弧与裂谷环境下C2 H6/C3 H8比值有明显差异。以广东长坑 (Au Ag)和嵩溪 (Ag Sb)矿床为例 ,概述了这些体系各自的应用 相似文献
988.
Photometric and spectral analysis of data from the Cassini Visual and Infrared Mapping Spectrometer (VIMS) has yielded significant results regarding the properties and composition of the surface of Saturn's satellite Enceladus. We have obtained spectral cubes of this satellite, containing both spatial and spectral information, with a wavelength distribution in the infrared far more extensive than from any previous observations and at much higher spatial resolution. Using a composite mosaic of the satellite, we map the distribution of crystalline and amorphous ices on the surface of Enceladus according to a “crystallinity factor” and also the depth of the temperature- and structure-dependent 1.65 micron water-ice band. These maps show the surface of Enceladus to be mostly crystalline, with a higher degree of crystallinity at the “tiger-stripe” cracks and a larger amorphous signature between these stripes. These results suggest recent geological activity at the “tiger stripe” cracks and an intriguing atmospheric environment over the south pole where amorphous ice is produced either through intense radiative bombardment, flash-freezing of cryovolcanic liquid, or rapid condensation of water vapor particles on icy microspherules or on the surface of Enceladus. 相似文献
989.
For in situ astrobiological studies of Mars or other planets, we must employ strategies that will enable us to verify whether our approach and prototype instruments are actually capable of distinguishing life from non-life. This must be done against a background of rigorously conducted scientific characterization of the environment or sample types being considered for measurement by the instruments under development. In this study we show how a combination of mineralogical and textural features can be considered a biosignature in an early Mars analogue environment, Death Valley, California. We propose that it is a combination of features in context of the geologic matrix which allows determination of biogenicity to be made. Polymineralic microbialites (organosedimentary formations constructed by microorganisms) from a spring pool at Badwater, within Death Valley National Park, are composed of alternating biogenic and abiogenic minerals in a distinct triplet sequence related to wet and dry seasons. A microbial community, occurring as a black biofilm, produced paired layers of two different mineral types: manganese oxyhydroxides and calcite. These biogenic layers are separated from the next pair by a gypsum layer and appear to be laid down in the wet season, with the gypsum (a mineral positively identified on Mars) precipitating in the dry part of the year, abiogenically (i.e., not dependent on microbial metabolic activity for its deposition). In addition, textural features (smaller grain size and less geometric morphology) unique to the biogenic vs the abiogenic layers, were consistently observed so that texture served as a biosignature in this environment. 相似文献
990.
We simulate the production and orbital evolution of escaping ejecta due to cometary impacts on Io. The model includes the four Galilean satellites, Amalthea, Thebe, Jupiter's gravitational moments, Saturn and the Sun. Five scenarios are examined: an impact at the apex, the sub-jovian point, the anti-jovian point, the antapex, and at the south pole of Io. We estimate that on average a cometary impact injects thrice its mass (in the form of Io surface material) into jovicentric orbit. The majority of the escaping debris comes back to Io, but a sizeable fraction (between 5.0 and 8.7%) manages to reach Europa, and a smaller fraction Ganymede (between 1.5 and 4.6%). Smaller fractions reached Amalthea Thebe, Callisto, and Jupiter itself. For million year time scales, the mass transfer to Europa is estimated as 1.8-3.1×1014 g/Myr. The median time for transfer of ejecta from Io to Europa is ∼56 years. 相似文献