Research on energy conservation method of the image compression coding based on wavelet transform for WVSNs

Author(s):  
Xu Lin ◽  
Fu Anqi
2012 ◽  
Vol 433-440 ◽  
pp. 5324-5328
Author(s):  
Guang Li Wu ◽  
Zhen Sen Wu ◽  
Shen Miao Han ◽  
Guang Ling Wu

This paper introduced some significant applications of aurora images, listed the main factors of choosing wavelet basis in image compression coding and analyzed the influence of aurora image compression effect caused by different wavelet basis were experimentally. The results of two kinds of significant wavelet transform algorithms EZW and SPIHT were analyzed, compared and also experimentally improved.


2013 ◽  
Vol 380-384 ◽  
pp. 3815-3817
Author(s):  
Yan Yang

This paper presents a new method of scalable image compression coding based on the wavelet transform. This method delimits the region of interest of the original image, and give a high-quality encoding to this region and a rough encoding to the rest. The result shows that in the limited memory space, this algorithm provides the coarser reconstruct image to satisfy the basal subject quality. Using this method, we can give a high quality encoding to the region for interest.


2003 ◽  
Vol 1 ◽  
pp. 1-4 ◽  
Author(s):  
E. Howe ◽  
L. Stenseng ◽  
C. C. Tscherning

Abstract. The energy conservation method is based on knowledge of the state vector and measurements of nonconservative forces. This is or will be provided by CHAMP, GRACE and GOCE. Here the analysis of one month of CHAMP state vector and accelerometer data is described. The energy conservation method is used to estimate the gravity potential at satellite altitude. When doing so we consider the tidal potential from the sun and the moon, the explicit time variation of the gravity potential in inertial space and loss of energy due to external forces. Fast Spherical Collocation have been used to estimate a gravity field model to degree and order 90, UCPH2002 04. This gravity field model is compared to EGM96 and EIGEN-2. The largest differences with respect to EGM96 are found at those places where the gravity data used to determine EGM96 had the largest uncertainty. EIGEN-2 and UCPH2002 04 are similar, though there are some differences in Antarctica and Central Asia.


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