水准网中起算点的选用方法探讨     

徐万祥  柴本红  于松 《山东国土资源》2009,25(10):50-52

水准网平差中起算点质量好坏不仅影响平差精度,而且如果采用不好的点位,直接影响成果的使用,带来严重后果。该文以青州市水准网的布设为例,分析讨论了起算点对水准网精度的影响,提出了根据较差中误差大小选用起算点的方法,阐述了该方法的步骤,达到的效果,以及水准网布设方法等。  相似文献   

控制点数量与DEM分辨率对海岸带遥感影像正射校正精度影响分析   总被引：1，自引：0，他引：1       下载免费PDF全文

刘善伟  张杰  马毅 《海洋科学》2009,33(4):9-13

在保证海岸带区域控制点均匀分布的基础上，对3景SPOT-5影像分别使用1：5万DEM和SRTM90m数据，开展6个、9个、12个控制点的影像正射校正。结果表明：在海岸带区域，基于传感器物理模型的1景SPOT-5影像正射校正，6个控制点即可保证较高的精度，控制点数量的增多对精度的提高并不显著；1：5万DEM比SRTM90m数据对影像的正射校正精度略高，但并不明显，在缺少1：5万DEM时，用SRTM90m数据代替亦能满足908课题的精度要求，进一步验证了SRTM90m数据在高分辨率遥感影像正射校正中的可用性。  相似文献   

Thermodynamics under the extended uncertainty principle background: Q−ϕ criticality analysis     

《New Astronomy》2024

The study of thermodynamics in the background of the “extended uncertainty principle (EUP)” comes into interest in recent eras. In this article, we consider a charged black hole (BH) in higher dimensional space–time and present the thermodynamic parameters, based on a semiclassical framework, initially. Then we extend the same within the EUP background. We also analyze the $Q-\varphi$ criticality and find the critical points (${\varphi }_c,Q_c$ and $T_c$) when $Q-\varphi$ criticality appears. We study the effects of EUP on phase transition for higher dimensions ($d=5$) by plotting the $Q-\varphi$ diagrams. Further, we investigate the stability (thermal and global) of the BHs by employing the specific heat and the Gibbs free energy without and within EUP correction and compare the results with the Schwarzschild BHs in higher dimensions.  相似文献   

The influence of third order terms on basins of convergence in the Hénon–Heiles type system     

《New Astronomy》2022

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Automatic detection of sunspots on solar continuum HMI images blending local–global threshold     

《New Astronomy》2024

A huge collection of solar images to visualize sunspot are acquired by various solar observatories spread across the globe. This necessitates efficient tools for detecting and analyzing the sunspots encompassing diverse solar features. One such contribution is delivered in this work by exploiting the intrinsic intensity variations of solar images associated with sunspots and their attributes. The presented mechanism initially, pre-processes the acquired solar images by correcting the intensity variations introduced while profiling from the sun center to the limb followed by smoothening using a localized window. The resultant is then differenced from the global threshold that is obtained as a result of the statistical analysis computed over the probability distribution function of the input image. This arrangement offers higher discerning variations concerned with the local contextual structures related to sunspot, umbra, and penumbra. Also, it captures the major gradient variation between these regions that adds to the pixel heterogeneity surrounding them to finally render an automatic sunspot detection mechanism distinguishing the diverse solar regions. Receiver Operating Characteristics (ROC) investigation on annual solar images in Flexible Image Transport System (FITS) format reveals the presented method’s efficacy. Also, Pearson correlation analysis of the evaluated sunspot numbers from the detected sunspots with the solar catalog reveals the scheme’s detection closeness. Moreover, the model’s simplicity analyzed along the time and space dimensions affirms its extension to real-time analysis  相似文献   

Fractal basins of convergence in the restricted rhomboidal six-body problem     

《New Astronomy》2022

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