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281.
将一个坐标系平移、旋转到第二个坐标系位置,以建立坐标系的三个点九个坐标为自变量,应用单纯形加速法优化,通过调整步长,最大程度地消除建轴误差。 相似文献
282.
角速率输入下圆锥补偿算法的一般形式 总被引:1,自引:0,他引:1
传统圆锥补偿算法直接应用于由速率陀螺组成的捷联惯导系统时,算法误差明显增大.为抑制算法误差,提出了一种以角速率为输入信号,任意子样数圆锥补偿算法(包括改进算法)的一般形式,并在典型圆锥运动条件下以算法漂移误差最小为优化准则,推导了相应的圆锥补偿系数方程和算法误差表达式.利用给出的公式,求解一个线性方程组即可得到圆锥补偿系数,可方便快捷的设计任意子样数的角速率圆锥补偿算法以及改进算法.仿真结果表明,所设计的改进算法比同子样数常规角速率圆锥补偿算法在精度上有明显提高. 相似文献
283.
D. Maravilla B. Mendoza E. Juregui 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,42(9):1593-1600
Minimum extreme temperature series from several meteorological stations of the Gulf of Mexico are spectrally analyzed using the Maximum Entropy Method.We obtained significant periodicities similar to those found in meteorological and solar activity phenomena. This indicates that probably the solar activity signals are present in the minimum extreme temperature records of this Mexican region. 相似文献
284.
T. Dudok de Wit M. Kretzschmar J. Aboudarham P.-O. Amblard F. Auchère J. Lilensten 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
The solar EUV irradiance is of key importance for space weather. Most of the time, however, surrogate quantities such as EUV indices have to be used by lack of continuous and spectrally resolved measurements of the irradiance. The ability of such proxies to reproduce the irradiance from different solar atmospheric layers is usually investigated by comparing patterns of temporal correlations. We consider instead a statistical approach. The TIMED/SEE experiment, which has been continuously operating since February 2002, allows for the first time to compare in a statistical manner the EUV spectral irradiance to five EUV proxies: the sunspot number, the f10.7, Ca K, and Mg II indices, and the He I equivalent width. 相似文献
285.
M. Poje B. Vuković M. Varga V. Radolić I. Miklavčić D. Faj J. Planinić 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
Cosmic radiation bombards us at high altitude with ionizing particles; the radiation has a galactic component, which is normally dominant, and a component of solar origin. Cosmic ray particles are the primary source of ionization in the atmosphere above 1 km; below 1 km radon is a dominant source of ionization in many areas. 相似文献
286.
287.
The five main types of antisunward propagating energetic fluxes (particles and emission) may be thought of as well established to date, the effects of which lead to a particilar character of disturbance in the near-terrestrial environment (the Earth's magnetosphere, ionosphere and atmosphere). The strongest global restructuring of the magnetosphere and ionosphere is caused by fluxes of relatively dense n of 1-70 cm-3 at the Earth's orbit) Solar Wind (SW) quasi-neutral, low-energy (E < 10 keV) plasma which cause magnetospheric and ionospheric storms lasting 24 hours or longer. For that reason, main attention is given to their study at the initial stage of research. The physical essence of the method of predicting disturbances in the near-terrestrial space environment, the amplitude of which can be expressed in, for example, the Kp index units, involves:(1) identifying all the most geo-effective SW streams of type, (2) determing their sources on the solar disk,and (3) quantifying the correlations between the characteristics of their solar sources with a maximum value of the Kp-index that is caused by the concerned type of SW stream. Semi-phenomenological relations have been obtained, which relate parameters of type SW stream sources to characteristics of geomagnetic storms:storm commencement, the time at which the storm intensity reaches its maximum values, the storm duration,as well as to the storm amplitude expressed in terms of geomagnetic indeces. 相似文献
288.
The high flux of energetic electron on geostationary orbit can induce many kinds of malfunction of the satellite there, within which the bulk-charging is the most significant that several broadcast satellite failures were confirmed to be due to this effect. The electron flux on geostationary orbit varies in a large range even up to three orders accompanied the passage of interplanetary magnetic cloud and the following geomagnetic disturbances. Upon the investigation of electron flux enhancement events, two types of events were partitioned as recurrent events and random ones. Both of the two kinds of events relate to the interplanetary conditions such as solar wind parameters, IMF etc and their evolution characters as well. As for the recurrent events, we found that, (1) all of the events exhibits periodic recurrence about 27 days, (2) significant increase of electron flux relates to interplanetary index and characters of their distribution, (3) the electron flux also has relation to solar activity index. An artificial neural network was constructed to estimate the flux I day ahead. The random electron flux enhancement events are rare and present different distribution figures to the recurrent ones. The figure of the random events and the conditions of their occurrence is also discussed in this paper. 相似文献
289.
乐贵明 《中国空间科学技术》2004,24(5):62-66
介绍了第 2 0 0 9卡林顿周大黑子群AR484,AR486和AR488产生的太阳活动以及这些太阳活动对地球空间环境造成的影响。依据对太阳活动的统计研究 ,简要分析了三个大黑子群活动的差异。分析结果指出 ,关注某一时期太阳活动的活动经度带以及太阳活动在某一半球的主次是解决太阳活动短期预报非常重要的思路 相似文献
290.