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排序方式: 共有170条查询结果,搜索用时 15 毫秒
1.
寇新建 《大地测量与地球动力学》1994,(3)
由于观测条件的变化,观测值方差将产生随机波动。本文根据Bayes估计理论,推导了线性模型待估参数的分布函数及观测值方差估计公式,并将其用于位移检验。计算结果表明,在同样的置信度下,本方法更符合实际。文中还对参数估值的统计性质进行了讨论。 相似文献
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Sedimentary Features of Shallow Ancient River Channels on the Northern Shelf of the South China Sea 总被引:1,自引:0,他引:1
Kou Yangqi Du Deli nd Marine Geological Investigation Party MGMR Guangzhou Guangdong Jiang M inxi 《《地质学报》英文版》1995,69(1)
Quaternary buried ancient river channels are widespread in the shallow-level sediments of the northern shelf of the South China Sea. The sedimentary sequence mainly of fluvial deposits comprise an important component part of the low-stand system tract and transgressive system tract in the study region. The plannar variation and spatial association of the sedimentary features such as incised valley fillings, deltaic foreset wedges and block slides of shelf-marginal fans reflect the palaeogeographic environment during the fall of the regional sea level in the northern part of the South China Sea. Based on the high-resolution seismic reflection data and gelogical data from boreholes, the present paper makes an integrated interpretation of the Quaternary ancient river channels in the shallow sediments of the study area, studies the sedimentary features of the ancient channels such as their spatial distribution, seismic facies reflection indicators, sedimentary facies and sand -body types, and discusses thei 相似文献
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水灾遥感实时监测与快速评估的实践与思考 总被引:2,自引:0,他引:2
总结了参加1991 ̄1995年间3次水灾遥感监测与评估科学实验所取得的结果,并结合国情分析,提出进一步发挥航天遥感作用,航天与航空相结合,建立一个花费较少,切实可行,能满足水灾实时监测与快速评估需要的设想。 相似文献
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Acta Geotechnica - In this paper, the strength, ductility and microstructure behavior of cement-treated silt with polypropylene fiber was studied by a host of experimental studies. The influence of... 相似文献
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Tan Bao-lin Cheng Jun Tan Cheng-ming Kou Hong-xiang 《Chinese Astronomy and Astrophysics》2019,43(1):59-74
Radio observation is one of important methods in solar physics and space science. Sometimes, it is almost the sole approach to observe the physical processes such as the acceleration, emission, and propagation of non-thermal energetic particles, etc. So far, more than 100 solar radio telescopes have been built in the world, including solar radiometers, dynamic spectrometers, and radioheliographs. Some of them have been closed after the fulfillment of their primary scientific objectives, or for their malfunctions, and thus replaced by other advanced instruments. At the same time, based on some new technologies and scientific ideas, various kinds of new and much more complicated solar radio telescopes are being constructed by solar radio astronomers and space scientists, such as the American E-OVSA and the solar radio observing system under the framework of Chinese Meridian Project II, etc. When we plan to develop a new solar radio telescope, it is crucial to design the most suitable technical parameters, e.g., the observing frequency range and bandwidth, temporal resolution, frequency resolution, spatial resolution, polarization degree, and dynamic range. Then, how do we select a rational set of these parameters? The long-term observation and study revealed that a large strong solar radio burst is frequently composed of a series of small bursts with different time scales. Among them, the radio spike burst is the smallest one with the shortest lifetime, the narrowest bandwidth, and the smallest source region. Solar radio spikes are considered to be related to a single magnetic energy release process, and can be regarded as an elementary burst in solar flares. It is a basic requirement for the new solar radio telescope to observe and discriminate these solar radio spike bursts, even though the temporal and spatial scales of radio spike bursts actually vary with the observing frequency. This paper presents the scaling laws of the lifetime and bandwidth of solar radio spike bursts with respect to the observing frequency, which provide some constraints for the new solar radio telescopes, and help us to select the rational telescope parameters. Besides, we propose a spectrum-image combination mode as the best observation mode for the next-generation solar radio telescopes with high temporal, spectral, and spatial resolutions, which may have an important significance for revealing the physical essence of the various non-thermal processes in violent solar eruptions. 相似文献
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在高精度卫星定位数据处理中,对精密星历内插处理是一项基础工作。利用拉格朗日多项式插值法,从三方面对北斗导航系统精密星历进行了内插精度分析,分别是非滑动式拉格朗日插值法在不同插值阶数下的插值精度,滑动式拉格朗日插值法在不同插值阶数下的插值精度,以及非滑动式和滑动式拉格朗日插值法在同一插值阶数下的插值精度。算例结果表明,如果将插值阶数作为横坐标,且向右为正,插值精度为纵坐标,向上为正,那么非滑动式拉格朗日插值法的插值精度与插值阶数呈现一个开口向下的抛物线关系;滑动式拉格朗日插值法的插值阶数高于7后,插值精度处于稳定且高的状态,插值误差最大值为1. 1 mm左右,均方差在0. 4 mm左右;在同一插值阶数下,滑动式拉格朗日插值法的精度高于非滑动式拉格朗日插值法的精度。 相似文献