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41.
Small‐area patch merging is a common operation in land use data generalization. However, existing research on small‐area patch merging has mainly focused on local compatibility measures, which often lead to area imbalances among land use types from a global perspective. To address the shortcomings of previous studies by resolving local and global concerns simultaneously, this article proposes a merging method that considers both local constraints and the overall area balance. First, a local optimization model that considers three constraints—namely, the areas of neighboring patches, the lengths of shared arcs, and semantic similarity—is established. The areas of small patches are first pre‐allocated. Subsequently, in accordance with an area change threshold for individual land use types, land use types with area changes that exceed this threshold are identified. The patches corresponding to these land use types are subjected to iterative adjustments while considering the overall area balance. Based on their area splitting abilities, the split lines for small‐area patches are determined, and small‐area patches are merged. Finally, actual data from Guangdong Province are used for validation. The experimental results demonstrate that the proposed method is capable of preserving the local compatibility of patches while balancing the overall area associated with each land use type. 相似文献
42.
新疆白杨河大型铍铀矿床成矿流体特征及矿床成因初探 总被引:5,自引:0,他引:5
新疆和布克赛尔县白杨河大型铍铀矿床是亚洲最大的铍矿床,其矿体产出于晚石炭世微晶花岗斑岩与上泥盆统塔尔巴哈台组(D3t)中酸性火山岩的接触带上,该矿床为典型的热液矿床.萤石作为白杨河铍铀矿床中与成矿作用密切相关的脉石矿物,发育大量气液包裹体.通过对萤石中流体包裹体的显微测温,获得了其主成矿期包裹体的均一温度,为237~372℃(n=40),平均为308.5℃,反映该矿床为中高温热液矿床.萤石以相对富集中稀土(MREE) ((La/Yb)N=3.18~3.55),强烈亏损Eu (δEu=0.01),REE分布模式呈“V”字型为特征.萤石锶钕同位素数据显示出较高的锶同位素初始比值(0.7106),以及正εNd(t)值(3.50~2.95),相似于微晶花岗斑岩的锶钕同位素组成((87Sr/86Sr)i=0.7143~0.7466,εNd(t)=4.06~5.29),由此提出成矿流体主要来自微晶花岗斑岩岩浆分异的晚期热液.主成矿期的萤石包裹体显示高温、低盐度的特征,推断成矿流体源于微晶花岗斑岩晚期岩浆热液与大气降水的混合. 相似文献
43.
石榴石是沉积物中常见的重矿物,其可来源于多种岩石,而且不同类型母岩中石榴石具有多样的地球化学组成,因此碎屑石榴石的地球化学分析在沉积物源研究中应用广泛。通过电子探针分析可以容易地获得单颗粒碎屑石榴石的主量元素地球化学组成,可借此探讨其母岩类型,但也存在一定的局限性,比如中酸性火成岩和部分变沉积岩来源的石榴石通常都具有高Fe、Mn的特征,不易于区分。本文系统地收集了不同岩石类型的石榴石微量元素数据,尝试利用微量元素地球化学的差异性对碎屑石榴石物源分析进行补充。最终得出以下结论:(1)石榴石的稀土元素(REE)组成与钇(Y)元素指标可区分中酸性火成岩和变沉积岩来源的碎屑石榴石;(2)基性岩(橄榄岩、辉石岩)及所对应的变基性岩石(榴辉岩)中石榴石的微量元素地球化学组成相近,但部分橄榄岩来源的石榴石在镨/钬(PrN/HoN)值和重稀土总量(ΣHREE含量)上与辉石岩和榴辉岩的有显著差别,这一特点可运用于以基性岩母岩为主的碎屑沉积物源研究中;(3)夕卡岩中的石榴石在主量元素地球化学组成上表现为高度一致的高Ca特征,而稀土元素组成具有两种典型的分配模式,岩浆型(指示富铁、氧化环境)与热液型(指示富铝、还原环境)。综上所述,石榴石微量元素地球化学可以有效地运用于沉积物源分析研究中,是其主量元素物源分析方法的重要补充。 相似文献
44.
淮南采煤塌陷湖泊浮游植物优势种的营养动力学 总被引:2,自引:1,他引:2
在淮南潘谢矿区选取3个营养盐结构差异较大的塌陷湖泊,于2014—2015年4个季度分别对浮游植物群落结构组成进行调查,选取3个湖泊中的优势种(属)具尾蓝隐藻(Chroomonas caudata)、链形小环藻(Cyclotella catenata)和伪鱼腥藻(Pseudanabaena sp.)作为研究对象,设置不同的氮(N)、磷(P)浓度梯度进行营养动力学培养实验,并结合Monod方程,获得3个藻种在不同营养盐限制下的营养动力学参数.N限制下具尾蓝隐藻、小环藻和伪鱼腥藻的最大生长速率(μmax)和半饱和常数(Ks)分别为:0.66 d~(-1)、1.66 mg/L;0.37 d~(-1)、1.06 mg/L;0.71 d~(-1)、2.26 mg/L;P限制下它们的μmax和Ks则分别为:0.51 d~(-1)、0.023 mg/L;0.31 d~(-1)、0.035 mg/L;0.90 d~(-1)、0.015 mg/L.综上所述,在N充足时,伪鱼腥藻能够在竞争中形成优势,同时在P限制情况下易成为优势种,从营养动力学的角度揭示了其在塌陷湖泊中占据优势的营养盐动力学机制.研究结果可以为沉陷区水域开发利用和营养盐管理提供科学依据. 相似文献
45.
针对当前省级区域测震台网在判别边界地震是否需要速报的问题,基于内蒙古自治区行政区域的边界数据,利用几何学中包络线原理,在Matlab中将内蒙古地震速报范围以包络线的形式呈现,解译Msdp地震分析软件的数据接口,实现内蒙古地震速报区域在Msdp软件中的自动确认;对比分析地震速报区域自动确认功能的结果与现阶段手动量取方式判别地震事件是否需要速报的结果,表明地震速报区域的自动确认可提高速报业务软件系统的自动化程度,简化地震速报工作的操作流程,减少速报用时,提高速报工作的准确度。 相似文献
46.
47.
The midwinter suppression(MWS) of the North Pacific storm track(NPST) has been an active research topic for decades. Based on the daily-mean NCEP/NCAR reanalysis from 1948 to 2018, this study investigates the MWS-related atmospheric circulation characteristics in the Northern Hemisphere by regression analysis with respect to a new MWS index, which may shed more light on this difficult issue. The occurrence frequency of the MWS of the upper-tropospheric NPST is more than 0.8 after the mid-1980 s. The MWS is accompanied by significantly positive sea-level pressure anomalies in Eurasia and negative anomalies over the North Pacific, which correspond to a strengthened East Asian winter monsoon. The intensified East Asian trough and atmospheric blocking in the North Pacific as well as the significantly negative low-level air temperature anomalies, lying upstream of the MNPST, are expected to be distinctly associated with the MWS. However, the relationship between the MWS and low-level atmospheric baroclinicity is somewhat puzzling.From the diagnostics of the eddy energy budget, it is identified that the inefficiency of the barotropic energy conversion related to the barotropic governor mechanism does not favor the occurrence of the MWS. In contrast, weakened baroclinic energy conversion, buoyancy conversion, and generation of eddy available potential energy by diabatic heating are conducive to the occurrence of the MWS. In addition, Ural blocking in the upstream region of the MNPST may be another candidate mechanism associated with the MWS. 相似文献
48.
保存条件是中扬子地区页岩气富集的关键因素之一,宜地2井是中扬子寒武系页岩气发现井,通过对该井全井段岩芯裂缝古流体的地球化学分析,探讨了寒武系古流体成因和对水井沱组页岩气保存条件的指示意义。结果认为:① 覃家庙组膏岩层之上方解石脉缺少Fe2+、Mn2+,且δ13C和δ18O值较围岩偏负,指示其形成于氧化的环境,石牌组方解石脉δ13C偏负,黄铁矿脉δ34S值与膏盐相似,表明其成因与TSR密切相关;水井沱组脉体δ13C和δ18O与围岩相似,形成于封闭的环境。② 方解石脉包裹体群SO42-、Ca2+、Mg2+含量整体上由覃家庙组向上向下分别递减,钠氯系数以水井沱组最低,整体上向上升高,表明覃家庙组是高盐度卤水的主要来源,水井沱组受外来流体影响弱;包裹体水溶液δD和δ18O也指示娄山关组、石牌组方解石脉成因分别与大气水、TSR相关。③ 古流体地球化学研究表明宜昌地区页岩气保存条件整体较好,页岩气散失的主要通道是垂直裂缝,页岩气保存条件好与膏盐盖层发育、后期构造破坏弱、脉体对裂缝的及时封闭以及白垩系盖层等因素密切相关。 相似文献
49.
针对数字航空摄影作业技术流程中的作业标准、精度要求以及各关键指标的控制等问题,从数字航空摄影的技术计划制定、航线规划和各项技术指标的确定等方面入手,对基于海岸带、海岛(礁)特征的航摄分区、航线敷设、地面分辨率的确定、航摄季节与时间选择以及POS辅助航空摄影方案选择等内容进行了研究,为获取满足海洋测绘指标要求的航空摄影数据源提供支持。 相似文献
50.
Emmanuel Jacquet Marine Paulhiac‐Pison Olivier Alard Anton T. Kearsley Matthieu Gounelle 《Meteoritics & planetary science》2013,48(10):1981-1999
We report trace element analyses by laser ablation inductively coupled plasma mass spectrometry (LA‐ICP‐MS) of metal grains from nine different CR chondrites, distinguishing grains from chondrule interior (“interior grains”), chondrule surficial shells (“margin grains”), and the matrix (“isolated grains”). Save for a few anomalous grains, Ni‐normalized trace element patterns are similar for all three petrographic settings, with largely unfractionated refractory siderophile elements and depleted volatile Au, Cu, Ag, S. All three types of grains are interpreted to derive from a common precursor approximated by the least‐melted, fine‐grained objects in CR chondrites. This also excludes recondensation of metal vapor as the origin of the bulk of margin grains. The metal precursors were presumably formed by incomplete condensation, with evidence for high‐temperature isolation of refractory platinum‐group‐element (PGE)‐rich condensates before mixing with lower temperature PGE‐depleted condensates. The rounded shape of the Ni‐rich, interior grains shows that they were molten and that they equilibrated with silicates upon slow cooling (1–100 K h?1), largely by oxidation/evaporation of Fe, hence their high Pd content, for example. We propose that Ni‐poorer, amoeboid margin grains, often included in the pyroxene‐rich periphery common to type I chondrules, result from less intense processing of a rim accreted onto the chondrule subsequent to the melting event recorded by the interior grains. This means either that there were two separate heating events, which formed olivine/interior grains and pyroxene/margin grains, respectively, between which dust was accreted around the chondrule, or that there was a single high‐temperature event, of which the chondrule margin records a late “quenching phase,” in which case dust accreted onto chondrules while they were molten. In the latter case, high dust concentrations in the chondrule‐forming region (at least three orders of magnitude above minimum mass solar nebula models) are indicated. 相似文献