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121.
本文介绍了一种面向数字测图系统的摄影测量数据库,着重讨论了该数据库的基本框架及数据结构。尤其是对数据块动态串作了深入的探讨。实践表明,这种数据库的设计方案是可行的。 相似文献
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茅山东侧断裂的断层运动及其与溧阳地震关系的动力学模型 总被引:1,自引:0,他引:1
本文依据近年来江苏省茅山地区进行野外调查得到的新资料,对茅山东侧断裂带(简称茅东断裂)的基本特征作了概括和分析,在多种观察资料的约束条件下建立了三维动力学模型,以解释茅东断裂现代运动的力学机制及其与溧阳地震的关系,指出控制断层运动的应力状态是随深度而改变的。最后对有关溧阳地震发生原因的一些力学问题进行了讨论。 相似文献
125.
Mateus Dantas de Paula Marta Gómez Giménez Aidin Niamir Martin Thurner Thomas Hickler 《International Journal of Digital Earth》2020,13(2):262-277
ABSTRACTGlobal, fast and accessible monitoring of biodiversity is one of the main pillars of the efforts undertaken in order to revert it loss. The Group on Earth Observations Biodiversity Observation Network (GEO-BON) provided an expert-based definition of the biological properties that should be monitored, the Essential Biodiversity Variables (EBVs). Initiatives to provide indicators for EBVs rely on global, freely available remote sensing (RS) products in combination with empirical models and field data, and are invaluable for decision making. In this study, we provide alternatives for the expansion and improvement of the EBV indicators, by suggesting current and future data from the European Space Agencýs COPERNICUS and explore the potential of RS-integrated Dynamic Global Vegetation Models (DGVMs) for the estimation of EBVs. Our review found that mainly due to the inclusion of the Sentinel constellation, Copernicus products have similar or superior potential for EBV indicator estimation in relation to their NASA counterparts. DGVMs simulate the ecosystem level EBVs (ecosystem function and structure), and when integrated with remote sensing data have great potential to not only offer improved estimation of current states but to provide projection of ecosystem impacts. We suggest that focus on producing EBV relevant outputs should be a priority within the research community, to support biodiversity preservation efforts. 相似文献
126.
A technique to detect man-made interference in the visibility data of the Mauritius Radio Telescope (MRT) has been developed.
This technique is based on the understanding that the interference is generally ‘spiky’ in nature and has Fourier components
beyond the maximum frequency which can arise from the radio sky and can therefore be identified. We take the sum of magnitudes
of visibilities on all the baselines measured at a given time to improve detectability. This is then high-pass filtered to
get a time series from which the contribution of the sky is removed. Interference is detected in the high-pass data using
an iterative scheme. In each iteration, interference with amplitudes beyond a certain threshold is detected. These points
are then removed from the original time series and the resulting data are high-pass filtered and the process repeated. We
have also studied the statistics of the strength, numbers, time of occurrence and duration of the interference at the MRT.
The statistics indicate that most often the interference excision can be carried out while post-integrating the visibilities
by giving a zero weight to the interference points. 相似文献
127.
O. K. Manuel 《Journal of Earth System Science》2000,109(1):195-203
The notion of remote element synthesis has recently been modified to explain the presence of nucleogenetic isotopic anomalies
and decay products of short-lived nuclides by injection of a small amount ofexotic nucleogenetic material. Even with this modification, remote element synthesis seems inconsistent with the following observations:
相似文献
– | Evidence of coupled variations in the chemical and isotopic compositions of the source material for meteorites. |
– | Residual coupling of chemical and isotopic heterogeneities across planetary distances in the solar system today. |
– | The mass-fractionation relationship seen across isotopes of elements in the planetary system, in the solar wind, and in solar flares. |
– | Linkage of short-lived radioactivities with isotopic anomalies and with physical properties of their host grains, as expected for early condensate of fresh stellar debris. |
– | Temporal and spatial distributions of short-live nuclides and their decay products. |
– | Mirror-image (+ and −) isotopic anomalies in meteorite grains that sum to “normal” isotopic ratios, as expected of unmixed products of the same nuclear reactions that produced our bulk elements. |
– | The lac supporting evidence for “presolar” grains or nearby stars that injectedexotic material into the early solar nebula. |
128.
合成了1-(4-硝基苯基)-3-(3,5-二溴吡啶)三氮烯(NPDBPDT),并研究了NPD-BPDT与镍的显色反应。在pH 10.0的Na2B4O7-NaOH缓冲溶液介质中,表面活性剂Triton X-100存在下,镍与试剂生成摩尔比为1∶4的络合物在470 nm处有最大正吸收峰,表观摩尔吸光系数为1.02×105L.mol-1.cm-1;在540 nm处有最大负吸收峰,表观摩尔吸光系数为1.15×105L.mol-1.cm-1;以540 nm为参比波长、470 nm为测量波长进行双波长测定,表观摩尔吸光系数为2.17×105L.mol-1.cm-1。镍含量在0~480μg/L内符合比尔定律。方法用于合金样品中镍的测定,结果与原子吸收法相符,加标回收率为98.0%~102.0%;精密度小于5%(RSD,n=6)。 相似文献
129.
动态高压下斜长石的熔融和玻璃化研究 总被引:3,自引:0,他引:3
斜长石在冲击波产生的动态高温高压作用下较易熔融和淬火为非晶态物质,其矿物学名为熔长石。在随州陨石冲击变质特征的研究中,发现橄榄石、辉石等矿物除出现微裂隙外均保存完好,而多数斜长石颗粒则已熔融和玻璃化。可区分出两种形态的熔长石,一种是保持了原有矿物颗粒外形的‘继形熔长石’,另一种则以熔池状和脉状体形式产出的‘改形熔长石’。两种熔长石的光学和物理性质相似,它们的化学成分与晶质斜长石也基本相同,说明斜长石在高压下熔融时没有与周围物质发生明显的组分交换。在吉林陨石的人工冲击实验产物中,斜长石是最先熔融的硅酸盐矿物,也多以填隙的他形颗粒或脉状体和熔池的形式产出。经与其它陨石的静态高压淬火实验研究结果的比较,推定继形和改形熔长石的形成条件为≈20GPa和≤1100℃。本研究结果对了解地幔橄榄岩和俯冲的大洋板片部分熔融作用,以及地球火山岩玻璃和超基性岩中铬尖晶石的玻璃相岩浆包襄体物理化学性质有一定参考价值。 相似文献
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