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61.
合成平面波数据的Rytov近似叠前深度偏移 总被引:6,自引:0,他引:6
作者把Berkhout(1992)提出的合成平面波技术应用于线性Rytov近似叠前深度偏移,提高了波动方程叠前深度偏移的计算效率。通过在Marmousi模型数据试验,我们认为在达到基本相同成像效果的条件下,利用合成平面波技术的波动方程叠前深度偏移相对于基本共炮集数据的波动方程叠前深度偏移可提高计算效率约10倍。 相似文献
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在高温高压下,六方晶格的石墨转变为立方晶格的金刚石。选用灰分含量少、气孔分布均匀的T621A石墨为碳源,选择化学成分范围偏值小、杂质含量少的镍锰钴合金为触媒以及优质粉压叶腊石为传压介质,在高温、适压、长时间及其它条件下,合成高强度粗颗粒的优质金刚石取得了良好的效果。 相似文献
64.
本文在分析自动脉冲数字测相基本原理的基础之上,推出了不仅与测距频率有关,而且还与填充脉冲频率及低频测相频率有关的新的频率改正公式,并给出新的频率改正公式与传统频率改正公式之间等同的条件,即有锁相环路(或频率跟踪电路)的正常工作来保证。 相似文献
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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
67.
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. |
68.
Abstract Slices of oceanic lithosphere belonging to the neo‐Tethys realm crop out discontinuously in the northern Calabrian Arc, Southern Apennines. They consist of high‐pressure–low‐temperature metamorphic ophiolitic sequences formed from metaultramafics, metabasites and alternating metapelites, metarenites, marbles and calcschist. Ophiolites occupy an intermediate position in the northern Calabrian Arc nappe pile, situated between overlying Hercynian continental crust and the underlying Apenninic limestone units. In the literature, these ophiolitic sequences are subdivided into several tectonometamorphic units. Geochemical characteristics indicate that metabasites were derived from subalkaline basalts with tholeiitic affinity (transitional mid‐oceanic ridge basalt type), and a harzburgitic‐lherzolitic protolith is suggested for the serpentinites. The pressure–temperature‐deformation paths of the metabasites from different outcrops display similar features: (i) the prograde segment follows a typical Alpine geothermal gradient up to a metamorphic climax at 350°C and 0.9 GPa and crystallization of the high‐pressure mineral assemblage occurs along a pervasive foliation developed during a compressive tectonic event; and (ii) the retrogression path can be subdivided in two segments, the first is characterized by nearly isothermal decompression to approximately 400°C and 0.3 GPa and the second follows a cooling trajectory. During low‐pressure conditions, a second deformation event produces millimetric to decametric scale asymmetric folds that describe west‐verging major structures. The third deformation event is characterized by brittle extensional structures. The tectonometamorphic evolution of the ophiolitic sequences from the different outcrops is similar. Both thermobarometric modeling and tectonic history indicate that the studied rocks underwent Alpine subduction and exhumation processes as tectonic slices inside a west‐verging accretionary wedge. The subduction of oceanic lithosphere was towards the present east; therefore, the Hercynian continental crust, overthrusted on the ophiolitic accretionary wedge after the neo‐Tethys closure, was part of the African paleomargin or a continental microplate between Africa and Europe. 相似文献
69.
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
70.