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71.
首先给出时域频率稳定性分析中各种方差的实用计算公式,并在此基础上分析各种方差特性,总结归纳其适用范围。分析表明:①阿仑方差是时域频率稳定性分析中最常用的方法,但不能区分调相白噪声和调相闪变噪声;②改进阿仑方差通过相位平滑运算能识别这2种噪声;③时间方差和时间总方差主要用于描述频率源的时间波动,主要用于分析调相噪声;④当频率漂移项较大或受甚低频噪声影响时,哈达玛系列方差能给出很好的测量特性。 相似文献
72.
从分析双混频时差(DMTD)测量系统的测量误差着手,对系统设计和使用中常磁到的一些理论和技术问题进行了探讨,这涉及到公共源的影响、移相器的作用、自校和测量中的其它问题。 相似文献
73.
Future piloted missions to explore asteroids, Mars, and other targets beyond the Moon will experience strict limitations on communication between vehicles in space and control centers on Earth. These limitations will require crews to operate with greater autonomy than any past space mission has demonstrated. The Antarctic Search for Meteorites (ANSMET) project, which regularly sends small teams of researchers to remote parts of the southern continent, resembles a space mission in many ways but does not rely upon a control center. It provides a useful crew autonomy model for planners of future deep space exploration missions. In contrast to current space missions, ANSMET gives the crew the authority to adjust competing work priorities, task assignments, and daily schedules; allows the crew to be the primary monitor of mission progress; demands greater crew accountability for operational errors; requires the crew to make the most of limited communication bandwidth; adopts systems designed for simple operation and failure recovery; and grants the crew a leading role in the selection and stowage of their equipment. 相似文献
74.
V.V. Guryanov A.N. Fahrutdinova 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
The height–season and year-to-year regularities of parameters of first and second spatial harmonics determine the structure of the stratosphere and mesosphere circulation and its variability. In the period 1992–2002 at heights 0–55 km, the amplitudes and phases of the first and second spatial harmonics in the field of temperature, geopotential height, zonal and meridional wind were calculated by the method of harmonic decomposition. Dispersion (standard or mean square deviation) of their day-to-day and year-to-year variations was calculated by their wavelength constants. Height and season patterns of variability have been estimated. The difference in height–longitude variability for wave numbers m = 1 and 2 has been discovered. At the same time, the intensity of wave disturbances for m = 1 is less than for m = 2 excluding the polar areas, where a significant variability appears at the heights 0–55 km. There is also a tendency for the intensity of year-to-year variations to decrease in comparison with day-to-day variations. In cold and warm periods the amplitude of perturbation waves with m = 2 both for day-to-day and year-to-year variations is greater than for waves with m = 1. Transient height areas in the interval of 20–30 km are more distinct for day-to-day variations of polar area. 相似文献
75.
76.
高职院校图书馆的纸本工具书具有重要的应用价值,并拥有广泛、稳定的读者群,其地位和作用是网络信息所无法取代的。重视和加强图书馆工具书库的建设与管理,是高职院校建设与发展的重要环节。因此,工具书库应主动适应高职院校的专业发展的要求,不断加强设施建设和资源补充,及时加工、整理工具书的再版文献,努力向读者提供有效的服务措施;要充分利用学校的报刊、校园网、宣传橱窗和读书座谈会来加强图书宣传,引导和帮助读者加深对工具书的认识,只有这样才能充分发挥出工具书库应有的作用,最大限度地向读者提供优质服务,满足不同读者的需要。 相似文献
77.
78.
Raul Orus Perez 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(5):1607-1618
In the last 20?years, and in particular in the last decade, the availability of propagation data for GNSS has increased substantially. In this sense, the ionosphere has been sounded with a large number of receivers that provide an enormous amount of ionospheric data. Moreover, the maturity of the models has also been increased in the same period of time. As an example, IGS has ionospheric maps from GNSS data back to 1998, which would allow for the correlation of these data with other quantities relevant for the user and space weather (such as Solar Flux and Kp). These large datasets would account for almost half a billion points to be analyzed. With the advent and explosion of Big Data algorithms to analyze large databases and find correlations with different kinds of data, and the availability of open source code libraries (for example, the TensorFlow libraries from Google that are used in this paper), the possibility of merging these two worlds has been widely opened. In this paper, a proof of concept for a single frequency correction algorithm based in GNSS GIM vTEC and Fully Connected Neural Networks is provided. Different Neural Network architectures have been tested, including shallow (one hidden layer) and deep (up to five hidden layers) Neural Network models. The error in training data of such models ranges from 50% to 1% depending on the architecture used. Moreover, it is shown that by adjusting a Neural Network with data from 2005 to 2009 but tested with data from 2016 to 2017, Neural Network models could be suitable for the forecast of vTEC for single frequency users. The results indicate that this kind of model can be used in combination with the Galileo Signal-in-Space (SiS) NeQuick G parameters. This combination provides a broadcast model with equivalent performances to NeQuick G and better than GPS ICA for the years 2016 and 2017, showing a 3D position Root Mean Squared (RMS) error of approximately 2?m. 相似文献
79.
利用MCNP程序对450kV X光机建立模型,计算各参考辐射质下的原级谱、平均光子能量。对ISO 4037-1中已有范围的管电压与附加过滤片厚度关系曲线进行二次拟合,确定模拟厚度范围。利用MCNP计算各附加过滤组合下的平均光子能量值,并与外推法得出的平均光子能量值进行对比,将相对偏差最小时的附加过滤作为最终确定值。从部分能量点的模拟与测量结果的对比可看出,模拟得出的平均光子能量在2%以内与PTB及中国计量院测量结果保持一致,附加过滤最大相对偏差为18%。 相似文献
80.