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排序方式: 共有347条查询结果,搜索用时 15 毫秒
1.
针对垂直起降运载火箭一子级在返回着陆的过程中存在的参数不确定性,提出了一种基于非侵入式多项式混沌展开的序列优化和可靠度评估的返回轨迹不确定性优化方法。首先,建立了返回多飞行段轨迹在确定性条件下的优化模型。然后,为同时兼顾轨迹的鲁棒性和可靠性,建立了由鲁棒最优目标函数、基于可靠度的路径约束和鲁棒等式约束组成的不确定性返回轨迹优化模型。最后,基于非侵入式多项式混沌展开方法对鲁棒目标函数和等式约束进行量化处理,将原随机鲁棒优化问题转化为高维状态空间中的等价确定性优化问题;为提高路径约束的可靠度评估效率,基于非侵入式多项式混沌展开方法对最可能点法进行改进,进一步发展了序列优化和可靠度评估策略。数值仿真结果表明,所提出的不确定性优化方法具有较好的鲁棒性,可以满足工程可靠性指标要求,同时还具有较高的精度和计算效率。 相似文献
2.
针对我国下一代静止轨道微波探测器资料应用的需求,对微波50~60GHz和183GHz的温湿遥感通道开展了不同大气条件下探测敏感高度的模拟,发现大气散射对微波探测影响明显,尤其是近地面通道,在未来数据应用时需加以注意。提出一种基于一维变分的大气温湿度廓线物理反演算法。以美国最新一代气象卫星Suomi NPP搭载的ATMS(Advanced Technology Microwave Sounder)获取的观测资料为研究对象,RTTOV(Radiative Transfer for TOVS)快速辐射传输模式为前向算子,利用一维变分算法开展了温湿度廓线反演单点试验。研究发现:地表参数对微波亮温,尤其是地面通道影响较大。同时,反演所需背景场对反演结果影响较明显,反演所得温度与背景场较接近。 相似文献
3.
Rajat Acharya Saibal Majumdar 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(6):1892-1904
The vertical ionospheric TEC values obtained from GAGAN grid based ionospheric delay correction values over the sea in the Indian equatorial region have been compared with the corresponding values derived from the International Reference Ionosphere model, IRI-2016. The objective of this work is to study the deviation of the vertical TEC derived from the IRI model from ground truths over the sea for different conditions. This will serve the basic intention of assessing the candidature of the IRI model as an alternative ionospheric correction model in navigation receivers in terms of accuracy. We have chosen different solar activity periods, seasons, geomagnetic conditions, locations etc. for our comparison and analysis. The TEC values by the IRI-2016 were compared with the actual measured values for the given conditions and errors were obtained. The measured vertical TEC values at the ionospheric grid points were derived from the GAGAN broadcast ionospheric delay data and used as reference. The IRI model with standard internal functions was used in estimating the TEC at the same ionospheric grid points. The errors in the model derived values are statistically analysed. Broadly, the results show that, for the Indian sector over the sea, the IRI model performs better on quiet days in off equatorial regions, particularly in the northern region. The overall performance degrades for other conditions with the model generally underestimating the true TEC values and most severely in the equatorial region. The performance is worst in this region for the disturbed days of the equinoctial period. The comparison study is also done with the TEC data measured directly by dual frequency GPS receivers. The results were found to be in general agreement with those obtained by comparing the model with GAGAN broadcast data as reference. This study will be useful in considering the IRI-2016 model for real time estimates of TEC as an alternative to the current parametric model in a satellite navigation receiver in absence of other options. 相似文献
4.
Sicheng Wang Libin Weng Hanxian Fang Yanqiong Xie Shenggao Yang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
We investigate the intra-annual variations of globally averaged thermospheric density at 400 km altitude from 1996 to 2006 by using Artificial Neural Network Method (ANNM). The results indicate that thermospheric density is governed by solar activity, and the absolute error of our model is 13.67%, less than NRLMSISE-00 model. Fourier representation can catch the intra-annual variations more accurately than NRLMSISE-00 model and JB2008 model especially during 2002. We find that the Autumn maximum is slightly greater than Spring maximum during solar minimum, while the reverse is correct during solar maximum. There is a strong linear relation between solar activity and the amplitude of annual/semiannual variations, and the correlation coefficients are 0.9534 and 0.9424, respectively. Moreover, the amplitude ratio of the annual to semiannual variation is about 1.3 averaged, and changes in different years, but it has little relation with solar activity. Besides that, the amplitude of annual variation is larger than semiannual variation during 1996 and 2006 except 1998 and 2000. The relative error of NRLMSISE-00 model is 14.95%, decreasing to 12.49% after revising, and the correlation coefficients between this empirical model and its improved results and the observation are 0.8185 and 0.9210, respectively. Finally, we suggest the revised version of MSIS series of model should use the Fourier representation to express the intra-annual variations. 相似文献
5.
为研究复合固体推进剂损伤演化规律,基于分子动力学颗粒填充算法构建了HTPB(hydroxyl terminated polybutadiene)推进剂细观结构模型,通过在AP(ammonium perchlorate)颗粒/HTPB基体界面处引入黏接接触替代传统的黏接单元,并基于Hooke Jeeves的参数优化算法反演得到颗粒/基体界面处内聚力模型参数,利用双线性和自定义指数型损伤内聚力模型模拟了AP颗粒和HTPB基体黏接界面处损伤的萌生、发展、聚合直至宏观裂纹破坏的过程。通过数值仿真与实验结果对比发现,指数型损伤内聚力模型比双线性模型能更准确描述推进剂单轴拉伸过程中颗粒与HTPB基体界面间脱黏过程。最后对比了多阶段加载实验结果与仿真结果曲线,发现两者变化趋势基本一致,最大偏差仅为10%,验证了所建细观模型的可靠性及反演所得界面参数的准确性。 相似文献
为研究装载工况和路面条件对弯道路段安全车速阈值的影响,运用TruckSim仿真软件建立大型车辆整车动力学模型、道路场景模型和驾驶人控制策略模型,从装载质量和道路附着系数2个方面分别设计实验进行仿真,分析车辆在弯道路段发生侧滑、侧翻的影响因素及其影响程度。以陕西省某高速公路一弯道路段为例,研究了车辆在双因素影响下,通过弯道的安全车速阈值。结果表明:随着装载质量的增加,弯道安全车速阈值减小,安全车速阈值与装载质量之间为幂函数关系;道路附着系数在0.1~0.6范围内时,随着弯道路面附着系数的增加,弯道安全车速阈值减小,且二者为指数函数关系;当道路附着系数在0.6~1.1范围内时,随着弯道路面附着系数的增加,弯道安全车速阈值变化趋于平缓。根据模型仿真分析结果,针对超载超限问题,进一步对交通管理部门、装载人员和驾驶人提出相应的安全建议,旨在提高公路弯道行车主动安全性,也为公路安全运营研究提供理论及技术支持。 相似文献
7.
Facundo L. Poblet Francisco Azpilicueta 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(9):2275-2289
The Earth and the near interplanetary medium are affected by the Sun in different ways. Those processes generated in the Sun that induce perturbations into the Magnetosphere-Ionosphere system are called geoeffective processes and show a wide range of temporal variations, like the 11-year solar cycle (long term variations), the variation of ~27?days (recurrent variations), solar storms enduring for some days, particle acceleration events lasting for some hours, etc.In this article, the periodicity of ~27?days associated with the solar synodic rotation period is investigated. The work is mainly focused on studying the resulting 27-day periodic signal in the magnetic activity, by the analysis of the horizontal component of the magnetic field registered on a set of 103 magnetic observatories distributed around the world. For this a new method to isolate the periodicity of interest has been developed consisting of two main steps: the first one consists of removing the linear trend corresponding to every calendar year from the data series, and the second one of removing from the resulting series a smoothed version of it obtained by applying a 30-day moving average. The result at the end of this process is a data series in which all the signal with periods larger than 30?days are canceled.The most important characteristics observed in the resulting signals are two main amplitude modulations: the first and most prominent related to the 11-year solar cycle and the second one with a semiannual pattern. In addition, the amplitude of the signal shows a dependence on the geomagnetic latitude of the observatory with a significant discontinuity at approx. ±60°.The processing scheme was also applied to other parameters that are widely used to characterize the energy transfer from the Sun to the Earth: F10.7 and Mg II indices and the ionospheric vertical total electron content (vTEC) were considered for radiative interactions; and the solar wind velocity for the non-radiative interactions between the solar wind and the magnetosphere. The 27-day signal obtained in the magnetic activity was compared with the signals found in the other parameters resulting in a series of cross-correlations curves with maximum correlation between 3 and 5?days of delays for the radiative and between 0 and 1?days of delay for the non-radiative parameters. This result supports the idea that the physical process responsible for the 27-day signal in the magnetic activity is related to the solar wind and not to the solar electromagnetic radiation. 相似文献