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1.
宋现锋 《地球信息科学学报》1996,(1):72-77
本文扼要地叙述了信息高速公路的概念、结构与特点。详细地阐述了信息高速公路的前沿技术发展动态,国外的产业对策,以及信息高速公路建设带给我们的策略启示。 相似文献
2.
Xian-Feng Zhao 《Astrophysics and Space Science》2011,332(1):139-144
The effect of the Σ-meson well depth on the gravitational redshift is examined within the framework of relativistic mean field
theory for the baryon octet system. It is found that, for a stable neutron star, the gravitational redshift increases with
the central energy density increase or with the mass increase but decreases as the radius increases. Considering a change
of US(N)U_{\Sigma}^{(N)} from −30 MeV to 30 MeV, for a stable neutron star the gravitational redshift near to the maximum mass increases. In addition,
it is also found that the growth of the US(N)U_{\Sigma}^{(N)} makes the gravitational redshift as a function of M
max /R increase, the higher the US(N)U_{\Sigma}^{(N)} the less the change in the gravitational redshift. 相似文献
3.
地图信息的网络共享问题探讨 总被引：1，自引：0，他引：1
前言 信息社会的全球化网络将使人类的生存空间发生质的飞跃,即物理空间向信息空间的转移。在以数字化生存为基本特征的虚拟社会里,模拟旅游、购物、工作等虚拟生活方式将替代大部分真实社会中的社会活动。尽管人类的实际活动空间缩小了,但是人类的抽象活动空间却遍及全球。 这种“物理空间缩小和抽象空间膨胀”是以各类专题地理信息的快速共享为基础的。用户在网络地图信息的帮助下,就可以非常清楚地把握他在网络空间中的位置及其相关信息。专题地图信息就好象是生活在虚拟社会中公民的指南针。 相似文献
4.
赣南淘锡坑钨矿床流体包裹体特征及其地质意义 总被引：1，自引：0，他引：1
淘锡坑钨矿是赣南一个重要的大型石英脉型钨多金属矿床。矿床主要矿化阶段含矿石英脉中石英和黄玉中的流体包裹体类型有单一水溶液相H2O-NaCl(Ⅰa型)、富液L+V两相H2O-NaCl(Ⅰb型)、两相H2O-NaCl-CO2体系包裹体(Ⅱa型)和三相H2O-NaCl-CO2包裹体(Ⅱb型)。Ⅰb型包裹体均一温度范围为80~370℃,具有多峰态分布特征,可识别出140~190℃,200~250℃和340~360℃几个峰。成矿流体的盐度相对较低,一般<8w(NaCleq)%。用流体包裹体组合的方法获得四组包体的相关参数,结果表明同一包体组合内不同包体的盐度、均一温度及密度基本一致,而不同包体组合中包体的盐度、均一温度及密度则相差较大,显示出不同包体组合所捕获的流体存在较大的差异。Ⅰb型包裹体均一温度分别分布在329~355℃,214~240℃和141~189℃三个温度区间,经压力校正后的捕获温度分别为400~425℃,275~300℃,210~260℃。这些特征表明,淘锡坑钨矿至少存在三期热液流动,其中前两期为成矿期的热液活动,第三期(次生包体)为成矿后的热液活动。根据Ⅱ型包裹体的CO2部分均一温度与最终均一温度计算出成矿流体的捕获压力67.3~97.8 Mpa,平均压力74.8 Mpa,按静岩压力换算成成矿深度为2.59~3.77 km,平均为2.88 km。 相似文献
5.
The performance of the Climate version of the Regional Eta-coordinate Model (CREM), a regional climate model developed by State Key Laboratory of Nu- merical modeling for Atmospheric Science and Geophysical Fluid Dynamics/Institute of Atmospheric Physics (LASG/IAP), in simulating rainfall anomalies during the ENSO decaying summers from 1982 to 2002 was evaluated. The added value of rainfall simulation relative to reanalysis data and the sources of model bias were studied. Results showed that the model simulated rainfall anomalies moderately well. The model did well at capturing the above-normal rainfall along the Yangtze River valley (YRV) during El Nio decaying summers and the below and above-normal rainfall centers along the YRV and the Huaihe River valley (HRV), respectively, during La Nia decaying summers. These features were not evident in rainfall products derived from the reanalysis, indicating that rainfall simulation did add value. The main limitations of the model were that the simulated rainfall anomalies along the YRV were far stronger and weaker in magnitude than the observations during El Nio decaying summers and La Nia decaying summers, respectively. The stronger magnitude above-normal rainfall during El Nio decaying summers was due to a stronger northward transport of water vapor in the lower troposphere, mostly from moisture advection. An artificial, above-normal rainfall center was seen in the region north to 35°N, which was associated with stronger northward water vapor transport. Both lower tropospheric circulation bias and a wetter model atmosphere contributed to the bias caused by water vapor transport. There was a stronger southward water vapor transport from the southern boundary of the model during La Nia decaying summers;less remaining water vapor caused anomalously weaker rainfall in the model as compared to observations. 相似文献
6.
The constraints on the properties of neutron star matter from the mass of neutron star PSR J1614-2230 are examined in the framework of the relativistic mean field theory. We find that there are little differences between the σ potentials of large mass neutron star and those of canonnical mass neutron star. For potentials of ω, ρ, neutrons and electrons, the values corresponding to the large mass neutron star are larger than those to the canonnical mass neutron star as the baryon number density is more than a certain value. We also find that for the relative particle number density of electrons, muons, neutrons and protons and the pressure of the neutron star, the values corresponding to the large mass neutron star are far larger than those to the canonnical mass neutron star. For the relative particle number density of hyperons Λ, Σ?, Σ0, Σ+ and Ξ?, the values corresponding to the large mass neutron star are far smaller than those to the canonnical mass neutron star. These mean that the larger mass of neutron star is more advantageous to the production of protons but is not advantageous to the production of hyperons. 相似文献
7.
Acta Geotechnica - This study systematically presents the application of machine learning (ML) algorithms for constructing a constitutive model for soils. A genetic algorithm is integrated with ML... 相似文献
8.
环介导等温扩增联合横向流动试纸条快速检测扁浒苔(Ulva compressa)的研究 总被引：2，自引：1，他引：1
本研究将环介导等温扩增技术(loop-mediated isothermal amplification,LAMP)与横向流动试纸条(lateral flow dipstick,LFD)的可视化检测方法结合,建立了扁浒苔(Ulva compressa)的LAMPLFD快速检测技术。该方法以扁浒苔的内转录间隔区(ITS1-5.8S-ITS2)序列为检测靶标,设计了3对特异性引物(其中,上游内引物由生物素标记)和1条异硫氰酸荧光素标记的探针。结果表明,LAMP最适反应温度为63°C,扩增时间为60 min,从核酸扩增到LFD结果判读需70 min。利用LAMP-LFD可特异性检出扁浒苔,对浒苔、曲浒苔、缘管浒苔和孔石莼等石莼属绿藻以及塔玛亚历山大藻、无纹环沟藻、东海原甲藻、锥状斯克里普藻和赤潮异弯藻等常见微藻的检测结果为阴性。该方法最低可检测到0.1 pg的扁浒苔基因组DNA,是以Uco ITS-F3和Uco ITS-B3为特异性引物的PCR方法的100倍。对实际样品的检测结果表明,LAMP-LFD方法检测扁浒苔与传统的形态学观察的结果一致。因此,该方法可快速、特异地检测出扁浒苔,而且操作简单,仪器设备依赖性低,有潜力成为扁浒苔现场检测的常规技术手段。 相似文献
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10.
Xian-Feng Liu Jeroen Tromp Adam M Dziewonski 《Earth and Planetary Science Letters》1998,160(3-4):343-351
In 1983, Lay and Helmberger [Geophys. J. R. Astron. Soc. 75 (1983) 799–837] reported the detection of a precursor to the seismic phase ScS. They attributed this precursor to a sharp seismic discontinuity located several hundred kilometers above the core–mantle boundary. Such a lowermost mantle discontinuity implies the existence of a sharp phase change or a chemical boundary. Precursors to ScS and, less frequently, PcP have since been observed in numerous locations, but are not a global phenomenon. Frequently, PcP precursors are weak or absent when ScS precursors are observed in the same location, and vice versa. There can be significant variations in the amplitude and arrival time of the precursor relative to the main phase. The presence or absence of these precursors has led to speculations about the nature of the lowermost mantle. Here we demonstrate that ScS or PcP precursors may be produced by gradients in seismic wave speed associated with large-scale lowermost mantle heterogeneity. Rather than a phase or chemical boundary with substantial topography, such gradients require lateral variations in temperature and, close to the core–mantle boundary, composition. 相似文献