基于高光谱技术的黑土地微量金属元素探测方法及地学意义     

王建华  左玲  李志忠  穆华一  周萍  杨佳佳  赵英俊  秦凯 《地质力学学报》2021,27(3):418-429

在土壤中重金属含量较低的情况下,重金属的高光谱特征响应非常微弱,不易构建精确的高光谱直接反演模型。为了解决上述问题,依据土壤化学变量间的理化性质,将重金属富集特征转移到与之相关的化学主量元素上,使重金属微弱的信息得以间接定量反演。文中以海伦市黑土土壤为研究对象,通过主成分分析、聚类分析确定了主量元素氧化铁（Fe₂O₃）与微量重金属As、Zn、Cd之间存在明显吸附赋存关系。选用偏最小二乘法构建了研究区氧化铁含量的最佳反演模型（决定系数为0.704,均方根误差为0.148,F检验为12.732）,并利用氧化铁与As、Zn、Cd之间的赋存关系,通过神经网络构建了氧化铁预测值与重金属真实值间的非线性拟合模型,得出As含量的拟合程度最高,Zn的拟合程度较好,Cd的拟合效果较理想,总体相关性分别为0.796、0.732、0.530。研究结果表明,基于氧化铁含量的间接预测模型能对微量重金属As、Zn、Cd进行较好的定量预测,为微量重金属含量的定量分析提供了新的方法参考,为高光谱遥感技术预测土壤重金属含量提供了依据,增强了土壤微量重金属反演可行性,对细化自然资源质量监测、深化开展地学系统综合分析与评价有重要意义。   相似文献   

太湖流域降雨与太湖水位关系分析   总被引：1，自引：0，他引：1  

章杭惠  刘曙光  季同德 《水文》2021,41(1):85-89,41

太湖流域快速城镇化、水利工程建设等人类活动对流域水文过程产生了较大影响。基于1981~2018年太湖流域日降雨、太湖水位实测资料,分析了流域降雨与太湖水位涨幅关系,旨在揭示变化环境下该地区降雨与水位关系的变化特征及可能的驱动因素。研究表明,2000年以来太湖水位抬高趋势明显,但同等时段降雨量条件下对应的太湖水位涨幅有所下降,且降雨量越大,太湖水位涨幅减小的越明显;流域各时段降雨与太湖水位涨幅相关关系约0.9,流域10d雨强每增加50mm,太湖水位涨幅约16cm。该研究成果可为太湖水位的中长期预报,尤其是对入汛前、入梅前等关键时间节点的太湖水位调控、雨洪资源利用等流域管理工作提供参考。  相似文献   

冻融循环下初始含水率对非饱和膨胀土剪切特性试验     

张琦  杨忠年  时伟  凌贤长  涂志斌 《吉林大学学报(地球科学版)》2021,51(5):1544-1550

为探究冻融循环条件下初始含水率对膨胀土偏应力-应变关系和剪切特性的影响,本文对不同初始含水率的非饱和膨胀土进行了不固结不排水三轴剪切试验。结果表明：1）非饱和膨胀土的偏应力-应变曲线的形式随含水率增大由应变软化逐渐转变为应变硬化,偏应力峰值随含水率增大而降低;2）非饱和膨胀土的抗剪强度随初始含水率的增加呈线性下降趋势;3）非饱和膨胀土在第1次冻融循环后偏应力及抗剪强度大幅度下降,在3~7次冻融循环后达到稳定。初始含水率是影响非饱和膨胀土力学性质的主要原因。  相似文献   

The Characteristics and Related Problems of the Orbits Around the Earth-Moon Libration Points     

Liu Lin  Tang Jing-shi  Hou Xi-yun 《Chinese Astronomy and Astrophysics》2019,43(2):278-291

Due to the specific dynamics, the probes located at the halo orbits or Lissajous orbits around the Earth-Moon collinear libration point L₁ or L₂ are always studied in the synodic system to understand their trajectories. In fact, they are also orbiting the Earth in a distant Keplerian ellipse. Because of their intrinsic orbital instability, in the orbit prediction the initial errors propagate more prominently than those of the normal orbiting satellites, this requires special attention in the orbit design, maneuver, and control. Despite of all this, they are similar to the normal orbiting satellites in orbit determination and hardly require other special attentions. In this paper, the quantitative results of error propagation under the unstable dynamics, together with the theoretical analysis are presented. The results of precise orbit determination and short-arc orbit predictions are also shown, and compared with the results from the Beijing Aerospace Control Center.  相似文献   

2012年唐山4.8级地震强震动记录特征及场地相关特性分析     

齐玉妍  孙丽娜  吕国军  李慧 《地震》2019,39(4):172-180

2012年5月28日河北省唐山市古冶区与滦县交界发生4.8级地震, 国家强震动台网中心在河北、 天津和北京的94个强震动台站记录到了本次地震的加速度。 本文给出了获取记录的强震动台站分布及强震动记录结果, 统计了强震动记录数量随震中距的变化, 给出了3个较小震中距台站记录到的加速度时程; 绘制了空间地震动峰值加速度等值线图及周期0.2 s、 2.0 s加速度反应谱值的等值线, 发现峰值加速度等值线与长周期加速度反应谱等值线极值分布具有明显地域差异, 分析认为是由于厚沉积层对长周期地震动具有放大作用造成的。 通过强震动记录与适用于本区的三个衰减关系对比, 分析了此次地震的峰值加速度衰减特征, 同时研究了周期0.2 s、 2.0 s加速度反应谱值的衰减特征, 周期2.0 s反应谱值随震中距的衰减与衰减关系能较好地对应, 然而在震中距100～130 km沉积层较厚的集中地区, 表现出了实际记录较衰减关系值偏大的现象, 认为同样是由于厚沉积层对地震动加速度反应谱长周期的放大作用导致的。 研究了震中距差别不大的情况下, 场地类型与沉积层厚度对反应谱特征周期的影响, 对比基岩台站与软弱地基土层台站的强震动记录反应谱, 发现软弱土层台站的土层对地震动有一定的放大作用, 导致中长周期地震动被放大, 对比位于沉积层较薄的隆起区台站与位于沉积层较厚的凹陷区台站强震动记录反应谱, 发现厚的沉积层不仅对反应谱长周期有放大的作用, 同时也会使得反应谱特征周期值变大。  相似文献   

Corrigendum to “Pb,Cu and Cd distribution in five estuary systems of Marche,central Italy” [Mar. Pollut. Bull. 96 Issue 1–2, (15 July 2015) 441–449]     

Anna Annibaldi  Silvia Illuminati  Cristina Truzzi  Giulia Libani  Giuseppe Scarponi 《Marine pollution bulletin》2017,114(1):635

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Study on wetting deformation characteristics of coarse granular materials and its simulation in core-wall rockfill dams     

Xiongxiong Zhou  Shichun Chi  Maohua Wang  Yufeng Jia 《国际地质力学数值与分析法杂志》2020,44(6):851-873

The wetting deformation of coarse granular materials is often considered to be an important cause of the core wall rockfill dam cracks during impounding. By analyzing existing research results, this paper proposes a hyperbolic relationship between the wetting axial strain and wetting stress level and puts forwards a warped surface relationship among spherical stress, shear stress, and the ratio of wetting volumetric strain to wetting axial strain. To illustrate its practicability, the wetting strain model's parameter determination process is introduced and the rockfill materials wetting parameters are determined using the triaxial wetting test data. Moreover, the collapse settlement of Guanyinyan rockfill dam during first impounding is numerically simulated using the proposed method to calculate rockfill wetting deformation and verified by field measurements and monitoring data. The results show that the calculative method of wetting deformation proposed in this paper is reasonable and practical; the wetting deformation of upstream rockfill materials would cause an adverse deformation trend, which may lead to crack occurrence at the upstream slope and dam crest; and the Guanyinyan rockfill dam cracks on the top of junction mainly caused by the wetting deformation of upstream rockfill.  相似文献   

Evidence for the Retrograde Accretion onto Supermassive Black Holestwo     

Wang Kai  Huang Zheng-peng  Wang Jian-min 《Chinese Astronomy and Astrophysics》2019,43(2):217-224

Recently, Sloan Digital Sky Survey successfully carried out the reverberation mapping of a sky area, aiming to test the R ? L relation that has been already widely used. Here, R is the responsivity-weighted radius of the broad line region, and L is the optical luminosity at 5100 Å. Two results have been obtained from the data in the first year: (1) The time lags of AGNs (Active Galactic Nuclei) with a high accretion rate are much shorter than that estimated from the R ? L relation, which confirmed the results of reverberation mapping observations made by the Lijiang 2.4 meter telescope. (2) Some AGNs with a lower accretion rate also have very short time lags. The shortening of the time lags of the AGNs with a low accretion rate is caused by the retrograde accretion of black holes. This result has verified from observations the theoretical prediction made by Wang et al. (2014). The discovery of the black holes with a retrograde accretion has important significance, it indicates that the cosmological evolution of the black holes in quasars is implemented via the inherently random accretion.  相似文献   

Neptune Trojans: a Revisit and a New Membertwo     

Wu Rui-jun  Zhou Lei  Zhou Li-yong 《Chinese Astronomy and Astrophysics》2019,43(2):262-277

Up to now, 17 Neptune Trojan asteroids have been detected with their orbits being well determined by continuous observations. This paper analyzes systematically their orbital dynamics. Our results show that except for two temporary members with relatively short lifespans on Trojan orbits, the vast majority of Neptune Trojans located within their orbital uncertainties may survive in the solar system age. The escaping probability of Neptune Trojans, through slow diffusion in the orbital element space in 4.5 billion years, is estimated to be ～50%. The asteroid 2012 UW177 classified as a Centaur asteroid by the IAU Minor Planet Center currently is in fact a Neptune Trojan. Numerical simulations indicate that it is librating on the tadpole-shaped orbit around the Neptune's L₄ point. It was captured into the current orbit approximately 0.23 million years ago, and will stay there for at least another 1.3 million years in the future. Its high inclination of i ≈ 54^° not only makes it the most inclined Neptune Trojan, but also makes it exhibit the complicated and interesting co-orbital transitions between the leading and trailing Trojans via the quasi-satellite orbit phase.  相似文献   

新疆皮山地区地震动衰减关系研究     

李文倩  魏斌  何金刚  张振斌  朱皓清 《中国地震》2017,33(1):81-90

利用2015年7月3日皮山M_S6.5地震序列的波形资料,采用微遗传算法反演得到震源区的5个介质参数,即应力降Δσ为75.95bars,品质因子Q_0为186.33,η值为0.26,几何衰减分段点R_1为72.18km,R_2为139.70km;并由此计算得到的傅氏谱再配合随机相位谱,进而得到地震动时程,建立了震源区地震动衰减关系。由于缺乏强震记录,本文还收集了2008年10月5日乌恰M_S6.9地震、2008年10月6日阿克陶M_S6.2地震、2012年3月9日洛浦M_S6.0地震的强震数据,将计算结果与经验性衰减关系以及3次强震记录进行比较后发现,皮山地震、洛浦地震的强震数据普遍高于经验性衰减关系,乌恰地震的强震数据与俞言祥等文中的衰减关系吻合较好,在远场低于本文的计算结果。  相似文献