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141.
142.
介绍了企业网IP电话系统的设计和实现方法。系统利用企业网这一高效的通讯介质 ,并针对目前Ethernet的特性进行优化 ,辅以三层数据应用实现了局域网内的话音文字通讯和局域网与PSTN电话网间的拨号及话音通讯。 相似文献
143.
春运期大气15—25天振荡的传播与江苏连阴雨(雪)过程 总被引:1,自引:1,他引:0
本文对6年春运期江苏附近几个经圈和纬圈850hPa温度格点序列, 分别计算15-25天带通滤波。结果表明110°E和35°N剖面的低频波与江苏连阴 雨(雪)天气过程有较好的对应关系。 相似文献
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G. Beekman M. Somers T. Naylor C. Hellier 《Monthly notices of the Royal Astronomical Society》2000,318(1):9-17
We present red spectra in the region ∼ λ 7000–8300 Å of the eclipsing dwarf nova IP Peg, with simultaneous narrow-band photometry centred at 7322 Å. We show that by placing a second star on the slit we can correct for the telluric absorption bands which have hitherto made the TiO features from the secondary star unusable. We use these TiO features to carry out a radial velocity study of the secondary star, and find this gives an improvement in the signal-to-noise ratio of a factor of 2 compared with using the Na i doublet. In contrast with previous results, we find no apparent ellipticity in the radial velocity curve. As a result we revise the semi-amplitude to K 2 =331.3±5.8 km s−1 , and thus the primary and secondary star masses to 1.05-0.07 +0.14 M⊙ and 0.33-0.05 +0.14 M⊙ respectively. Although this is the lowest mass yet derived for the secondary star, it is still overmassive for its observed spectral type. However, the revised mass and radius bring IP Peg into line with other cataclysmic variables in the mass–radius–period relationships.
By fitting the phase-resolved spectra around the TiO bands to a mean spectrum, we attempt to isolate the light curve of the secondary star. The resulting light curve has marked deviations from the expected ellipsoidal shape. The largest difference is at phase 0.5, and can be explained as an eclipse of the secondary star by the disc, indicating that the disc is optically thick when viewed at high inclination angles. 相似文献
By fitting the phase-resolved spectra around the TiO bands to a mean spectrum, we attempt to isolate the light curve of the secondary star. The resulting light curve has marked deviations from the expected ellipsoidal shape. The largest difference is at phase 0.5, and can be explained as an eclipse of the secondary star by the disc, indicating that the disc is optically thick when viewed at high inclination angles. 相似文献
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147.
本文从当前天文观测所受自然环境的影响入手 ,提出远程控制观测是解决目前观测所遇到的困扰的好方法 ,并介绍了中科院云南天文台太阳射电组的 1 0m口径抛物面天线的计算机远程控制系统。本文着重讨论了远程控制的实施方案 ,包括天线当前的性能测试、如何安全地做到远程通信、前端控制 (即现场控制 )等问题 ,把TCP/IP协议族原理和Client/Server原理与模糊逻辑控制思想相结合 ,对 1 0m口径天线实施自动控制 ,并开发了用于现场控制、远程控制的网络控制软件。 相似文献
148.
改善VSAT卫星链路网际互联的技术途径 总被引:1,自引:0,他引:1
在卫星通信网上运行TCP/IP协议时,因电波空间传播产生的卫星链路时延,严重降低了TCP协议数据流的传输速率和通信效率。选择适当的TCP数据流发送窗口值,不能从根本上提高TCP数据流的传输速率。对于采用卫星通信链路作为传输信道的计算机广域网,在卫星站网关上使用TCP“协议欺骗”技术,能够显著提高TCP/IP协议在卫星通信网上运行的效率。文中给出了采用TCP/IP“协议欺骗”后实测的结果。 相似文献
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150.
The identification of reservoir oil–gas–water layers is a fundamental task in petroleum exploration and exploitation, but is difficult, especially in cases of complex hydrocarbon migration and accumulation. In such cases, hydrocarbon remigration and dysmigration take place very commonly, leading to the presence of residual or paleo-oil accumulations and layers, which cannot be easily identified or misinterpreted as oil layers by conventional logging and geophysical data. In this paper, based on a case study in the Luxi area of the central Junggar Basin, NW China, we seek to characterize such layers in terms of organic geochemistry. We suggest specific indicator parameters of organic geochemistry such as the chloroform bitumen content of reservoir extracts, which is usually >1.0% in oil layers. We explore the application of grains containing oil inclusions (GOI) (the ratio of mineral grains containing oil inclusions to the total number of mineral grains) for the identification of oil–gas–water layers in the Junggar Basin for the first time; this method has been used elsewhere. The maximum GOI values for the oil layers, oil–water layers, water layers and dry layers are >11%, 7%–11%, 6%–7% and <6%, respectively. In addition, gas layers and heavy-oil layers that are difficult to identify by conventional organic geochemical parameters were identified using biomarkers. The typical characteristics of the soluble reservoir bitumen in the gas layers include a much greater abundance of tricyclic terpanes (two times in general) relative to pentacyclic terpanes and a tricyclic terpane distribution of C20 > C21 > C23. In contrast, the typical characteristic of the heavy-oil layers is the presence of 25-norhopanes in reservoir bitumen extracts. These specific indicators can be applied in the Junggar Basin and in similar settings elsewhere. 相似文献