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11.
C. De Jager 《Space Science Reviews》2005,120(3-4):197-241
12.
A non-local vectorial total variational model for multichannel SAR image speckle suppression 总被引：1，自引：0，他引：1
This paper aims at the multichannel synthetic aperture radar(SAR)image speckle reduction.This paper proposes a novel energy minimized regularization model for multichannel image denoising,which is an extension of the non-local total variational model for gray-scale image.It contains two terms,namely the vectorial data fidelity term and the non-local vectorial total variation term.The latter is constructed by high-dimensional non-local gradient that contains the structure information of the multichannel image.The existence and the uniqueness of the solution of the model are proved.A fixed point iterative algorithm is designed to acquire the solution of this model.The convergence property of this algorithm is proved as well.This model is applied to the multipolarimetric and multi-temporal RADARSAT-2 images despeckling.The result shows that this model performs better than the original vectorial total variational model on texture preserving. 相似文献
13.
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
14.
Emirant Bertillas Amabayo Lee-Anne McKinnell Pierre J. Cilliers 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The occurrence of mid-latitude spread F (SF) over South Africa has not been extensively studied since the installation of the DPS-4 digisondes in 1996 and 2000 at Grahamstown (33.32 °S, 26.50 °E) and Madimbo (22.38 °S, 30.88 °E) respectively. This study is intended to quantify the probability of occurrence of F region disturbances associated with SF over South Africa. A study was conducted using data for 8 years (2001–2008) over Madimbo (with a time resolution of 30 min) and Grahamstown (with a variable time resolution of 15 and 30 min). In this study, SF has been classified into frequency SF (FSF), range SF (RSF) and mixed SF (MSF). The SF events were identified by manually identifying ionograms showing SF and tabulating them according to type for further statistical analysis. The results show that the diurnal pattern of SF peaks strongly between 01:00 and 02:00 local time, LT (LT = UT + 2 h), where UT is the universal time. This pattern is true for all seasons and types of SF at Madimbo and Grahamstown in 2001 and 2005, except for RSF which had peaks during autumn and spring in 2001 at Madimbo. The probability of both MSF and FSF tends to increase with decreasing solar activity, with a peak in 2005 (a moderate solar activity period). The seasonal peaks of MSF and FSF are more frequent during winter months at both Madimbo and Grahamstown. In this study, SF was evident in ∼0.03% and ∼0.06% of the available ionograms at Madimbo and Grahamstown respectively during the 8 years. 相似文献
15.
姚楠 《南京航空航天大学学报》1998,30(4):359-365
讨论中介逻辑命题演算扩张系统ＭＰ＊中在等值意义下的完全析取范式的存在性和唯一性。引入ＭＰ＊中等值全板范式的概念,并用分步构造法证明这种范式在等值意义下是存在的,且是唯一的。 相似文献
16.
针对纹理图像的去噪问题,通过分析全变分（TV）去噪模型与方向全变分（DTV）去噪模型,提出了一种具有鲁棒性的基于p 由图像的结构来确定在（0,2）中自适应地选取。由于该模型是含有可分性算子的非光滑优化问题,可用交替方向乘子法（ADMM）求解,并能保证算法的收敛性。数值实验结果表明:与其他经典模型相比,提出的模型取得了更高的峰值信噪比和结构相似度,在去除噪声的同时能有效保持图像的细节信息。 相似文献
17.
考虑太阳风动压与行星电离层中的带电粒子热压及磁压之和平衡,建立了有大气（电离层）的行星磁层顶形成的理论模型,结合卫星对火星的观测数据,对子午面内向日侧火星磁层顶位形进行了数值计算和分析,研究了火星磁层顶位形及其与太阳风动压之间的变化关系．结果认为,火星磁层顶位形与地球磁层顶相似．太阳风动压越大,火星磁层顶越靠近火星;太阳风动压越弱,火星磁层顶越远离火星．根据火星内秉磁矩从古到今逐渐减小的观点,探索了大尺度磁场（内禀磁矩）对火星磁层顶的贡献作用,结果认为大尺度磁场越强,火星磁层顶越远离行星．这对于进一步研究火星磁层的长期演化以及其他行星磁层的位形变化都具有重要的意义． 相似文献
18.
波分复用光(WDM)网络是目前较好的航空电子网络解决方案之一,具有高带宽、强灵活性、对协议和比特率透明、强扩展性等优点。但在实时性方面,WDM网络的消息传输存在不确定性,无法满足未来航空电子网络对于时间关键消息强实时性保障的要求。本文将时间触发机制引入WDM网络,设计了时间触发航空电子WDM(TTAWDM)网络的体系结构,包含协议栈、消息类型、调度流程等。TTAWDM用时刻调度表规划时间关键性消息的传输,保障消息传输过程和传输延时的确定性,以满足强实时性要求。在TTAWDM体系结构设计的基础上分析了网络消息的实时性,基于网络演算推导出速率限制消息的延时上界计算方法,并构造仿真实验展示了TTAWDM对于强实时性保障,同时验证了延时上界计算方法的有效性。 相似文献
19.
用于导弹系统性能统计分析的统计线性化伴随法 总被引：1，自引：0，他引：1
本文在研究ＳＬＡＭ方法基础上,进行了理论推导和计算方法方面的改进,并将此方法应用于导弹系统性能的统计分析,计算机仿真结果表明该方法与采用ＣＡＤＥＴ方法的结果完全一致。 相似文献
20.