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1.
为建立高精度的边坡位移预测模型,采用相空间重构(PSR)将边坡位移时间序列数据转换为多维数据,同时构造小波核函数改进的支持向量机模型,建立PSR-WSVM模型并应用于边坡位移预测。将PSR-WSVM模型预测结果与传统支持向量机(SVM)模型、小波支持向量机(WSVM)模型和基于相空间重构的支持向量机(PSR-SVM)模型预测结果进行对比,通过平均绝对误差(MAE)、平均绝对误差百分比(MAPE)和均方根误差(RMSE)3个精度评价指标验证PSR-WSVM模型的可行性。工程实例结果表明,PSR-WSVM模型预测结果的3个精度评价指标都优于另外3种模型,边坡位移预测的精度明显提升。 相似文献
2.
TANGYa XIEJiasui SUNHui 《山地科学学报》2004,1(1):38-45
Dry valleys are a striking geographic landscape in Hengduan Mountains Region and are characterized by low rainfall, desert type of vegetation and fragile environment. Past efforts and resources have been concentrated mainly on rehabilitation of degraded ecosystem and fragile environment, particularly reforestation, while socio-economic development has been largely overlooked. Despite successes in pocket areas, the overall trend of unsustainability and environmental deterioration are continuing. It is important to understand that uplift of the Tibetan Plateau is the root cause of development of dry valleys, and development and formation of dry valleys is a natural process. Human intervention has played a secondary role in development of dry valleys and degradation of dry valleys though human intervention in many cases has speeded up environmental degradation of the dry valleys. It is important to understand that dry valleys are climatic enclaves and an integrated approach that combines rehabilitation of degraded ecosystems and socio-economic development should be adopted if the overall goal of sustainable development of dry valleys is to be achieved. Promotion of niche-based cash crops, rural energy including hydropower, solar energy, biogas and fuelwood plantation is recommended as the priority activities. 相似文献
3.
The Siberian Solar Radio Telescope: the current state of the instrument,observations, and data 总被引:2,自引:0,他引:2
Grechnev V.V. Lesovoi S.V. Smolkov G. Ya. Krissinel B.B. Zandanov V.G. Altyntsev A.T. Kardapolova N.N. Sergeev R.Y. Uralov A.M. Maksimov V.P. Lubyshev B.I. 《Solar physics》2003,216(1-2):239-272
The Siberian Solar Radio Telescope (SSRT) is one of the world's largest solar radio heliographs. It commenced operation in
1983, and since then has undergone several upgrades. The operating frequency of the SSRT is 5.7 GHz. Since 1992 the instrument
has had the capability to make one-dimensional scans with a high time resolution of 56 ms and an angular resolution of 15 arc sec.
Making one of these scans now takes 14 ms. In 1996 the capability was added to make full, two-dimensional images of the solar
disk. The SSRT is now capable of obtaining images with an angular resolution of 21 arc sec every 2 min. In this paper we describe
the main features and operation of the instrument, particularly emphasizing issues pertaining to the imaging process and factors
limiting data quality. Some of the data processing and analysis techniques are discussed. We present examples of full-disk
solar images of the quiet Sun, recorded near solar activity minimum, and images of specific structures: plages, coronal bright
points, filaments and prominences, and coronal holes. We also present some observations of dynamic phenomena, such as eruptive
prominences and solar flares, which illustrate the high-time-resolution observations that can be done with this instrument.
We compare SSRT observations at 5.7 GHz, including computed `light curves', both morphologically and quantatively, with observations
made in other spectral domains, such as 17 GHz radio images, Hα filtergrams and magnetograms, extreme-ultraviolet and X-ray
observations, and dynamic radio spectra. 相似文献
4.
Radio astronomy experiments designed to probe the interplanetary plasma close to the Sun have been carried out at the wavelength = 2.92 m using the occultation method. The experiments are based on a modification of the occultation method by which the sources, in this case quasars, are used to measure the radial dependence of the apparent source size, the scattering angle (R). The radial dependence of this source size (R) reveals that an anomalous enhancement in the scattering appears at radial distances from about 16 to 30 R
, which is associated with the solar wind transsonic region. It is shown by analysis of the theoretical equations that the radial profiles of both the source size (R) and the scintillation index m(R) are consistent in the near solar interplanetary medium (R 40 R
). Combining these two independent applications of the occultation method extends the range of the investigation and provides a powerful new diagnostic of the solar wind transsonic region. 相似文献
5.
鱼卡煤田大煤沟组高分辨率层序地层特征及聚煤规律 总被引:1,自引:0,他引:1
利用高分辨率层序地层学理论和技术方法,综合地震、测井、岩芯和煤质资料对柴达木盆地北缘鱼卡煤田中下侏罗统大煤沟组地层河湖三角洲沉积体系进行高分辨率层序地层学分析,从中识别出短期、中期、长期3个级别的基准面旋回层序,划分出向上"变深"非对称型、向上"变浅"非对称型及对称型3种短期基准面旋回基本结构类型。依据等时地层对比法则进行不同级次基准面旋回层序的联井对比,建立了大煤沟组的等时地层格架,在等时地层格架内进行了煤层对比,并在等时地层格架内分析了聚煤规律。 相似文献
6.
7.
冈底斯驱龙斑岩铜钼矿床的岩浆侵位中心和矿化中心:破裂裂隙和矿化强度证据 总被引:8,自引:1,他引:7
驱龙斑岩铜钼矿床是迄今为止在西藏冈底斯成矿带上发现的规模最大的铜矿床.文章根据对驱龙矿区各类岩石破裂裂隙的野外实测数据,结合矿区已有钻孔品位资料,分别绘制了矿区地表破裂裂隙等值线图、走向投影图及梅花图、钻孔5 000 m海拔标高水平切面Cu、Mo品位等值线图.研究结果表明,驱龙斑岩铜钼矿床的岩石中破裂裂隙相当发育,连成一片,没有明显的多个高值中心,空间上破裂裂隙呈放射状产出;5 000 m海拔标高水平切面显示Cu、Mo矿化较强、较均匀,矿化呈面状,为典型的由单一斑岩体侵位造成的中心式矿化特征.据破裂裂隙和Cu、Mo矿化空间分布,可确定驱龙矿区岩浆中心和矿化中心均位于钻孔405、1205、801、809所围成的矩形区域附近. 相似文献
8.
V. S. Kulikov Ya. V. Bychkova V. V. Kulikova Yu. A. Kostitsyn O. S. Pokrovsky M. V. Vasil’ev 《Petrology》2008,16(6):531-551
The Ruiga differentiated mafic-ultramafic intrusion in the northwestern part of the Vetreny Belt paleorift was described for the first time based on geological, petrological, geochronological, and geochemical data. The massif (20 km2 in exposed area) is a typical example of shallow-facies peridotite-gabbro-komatiite-basalt associations and consists of three zones up to 810 m in total thickness (from bottom to top): melanogab-bronorite, peridotite, and gabbro. In spite of pervasive greenschist metamorphism, the rocks contain locally preserved primary minerals: olivine (Fo 75–86), bronzite, augite of variable composition, labradorite, and Cr-spinels. A mineral Sm-Nd isochron on olivine melanogabbronorite from the Ruiga Massif defines an age of 2.39 ± 0.05 Ga, while komatiitic basalts of the Vetreny Belt Formation were dated at 2.40–2.41 Ga (Puchtel et al., 1997). The rocks of the Ruiga intrusion and lava flows of Mt. Golets have similar major, rare-earth, and trace element composition, which suggests their derivation from a single deep-seated source. Their parent magma was presumably a high-Mg komatiitic basalt. In transitional crustal chambers, its composition was modified by olivine-controlled fractionation and crustal contamination, with the most contaminated first portions of the ejected melt. In terms of geology and geochemistry, the considered magmatic rocks of the Vetreny Belt are comparable with the Raglan Ni-PGE komatiite gabbro-peridotite complex in Canada (Naldrett, 2003). 相似文献
9.
两千年来黑河流域水资源平衡估算与下游水环境演变驱动分析 总被引:1,自引:0,他引:1
利用地方史志、历史地理、树木年轮和近代器测记录相关的黑河流域历史时期人口变动、水土资源开发利用、下游湖泊变化、流域水资源和气候变化等资料, 通过对比上游出山水资源量、中游人类活动水资源利用量和下游湖泊面积变化, 在千年-百年时间尺度上对流域水资源平衡进行了估算, 并分析了历史时期各阶段下游湖泊水环境和天然绿洲演变过程和驱动机制. 研究结果表明: 在黑河流域, 气候变化条件下的上游山区水资源总量和中游走廊平原区绿洲人类活动用水后下泄的水资源量, 决定了下游水环境演变过程;在两千年来显现出不同历史阶段的流域水资源平衡模式和下游水环境演变特征, 以及气候变化和人类活动在不同历史时期的耦合驱动机制. 相似文献
10.
北疆阿尔泰南缘泥盆系浅变质碎屑沉积岩地球化学特征及其形成环境 总被引:12,自引:4,他引:8
对于北疆阿尔泰地区泥盆纪所处的大地构造环境,目前仍旧存在不同观点。前人基于阿尔泰南缘泥盆纪火山岩地球化学研究,分别提出了活动大陆边缘和被动大陆边缘裂谷等不同构造观点。阿尔泰造山带南缘的泥盆纪浅变质碎屑沉积岩地球化学研究表明,该套浅变质碎屑沉积岩原岩主要为泥质或砂质沉积岩。尽管不同岩性样品主量元素含量不同,但其化学蚀变指数(CIA)小于75,成分变异指数(ICV)接近或小于1.0,斜长石蚀变指数(PIA)平均70,说明其源区物质比较新鲜,成熟度相对较低,化学风化作用较弱。同样,不同岩性样品微量元素含量差别较大,但表生过程中不活泼的微量元素比值却比较一致,轻稀土(LREE)中度富集(La_N/Yb_N=2.88~9.90),重稀土(HREE)比较平坦,并伴有明显的Eu负异常(Eu/Eu~*= 0.45~0.89)。绝大多数样品具有高的La/Sc(1~3)、La/Y(0.5~1)和Ti/Zr(10~35),以及较低的Sc/Cr(0.1~0.3)比值,类似于大陆岛弧相关环境碎屑沉积物。在La-Th-Sc和Th-Sc-Zr/10构造环境判别图解中,除一千枚岩样品外,其他所有样品均落入大陆岛弧区。以上地球化学特征明显不同于大洋岛弧和被动陆缘沉积物,说明该套浅变质碎屑沉积岩可能沉积于活动大陆边缘的大陆岛弧相关环境,为认识阿尔泰造山带泥盆纪岛弧增生构造演化过程提供了一个重要证据。 相似文献