Throughput Optimization of non-real-time flows with delay guarantee of real-time flows in WLANs

Author(s):  
Yayu Gao ◽  
Lin Dai ◽  
Xiaojun Hei
2003 ◽  
Vol 26 (12) ◽  
pp. 1365-1375 ◽  
Author(s):  
F.Xabier Albizuri ◽  
Manuel Graña ◽  
Bogdan Raducanu

Author(s):  
Mohammad Rafi Lone ◽  
Najeed- Ud-Din

For real-time applications, efficient VLSI implementation of DWT is desired. In this paper, DWT architecture based on retiming for pipelining and unfolding is presented. The architecture is based on lifting one-dimensional Cohen-Daubechies-Feauveau (CDF) (5,3) wavelet filter, which is easily extended to 2-D implementation. It consists of low complexity and easily repeatable components. This paper is focused on the critical path minimization and throughput optimization at the same time. The architecture has been implemented on Virtex 6 Xilinx FPGA platform. The implementation results show that the critical path is minimized four to five times, while throughput is doubled, making the overall architecture approximately ten times faster when compared with the conventional lifting-based DWT architecture. Further with parallel implementation, the throughput has doubled without any increase in number of row buffers, implying that the architecture is memory efficient as well. The even and odd rows of the image are scanned in parallel fashion. To perform the 2-D DWT transform of an image of size 15 Megapixels, it takes 16.86 ms, which implies 59 images of that size can be processed in one second. This can be utilized for real-time video processing applications even for high resolution videos.


2011 ◽  
Vol 9 (1) ◽  
pp. 50 ◽  
Author(s):  
Sofiane Ouni ◽  
Salsabil Gherairi ◽  
Farouk Kamoun

2019 ◽  
Vol 6 (6) ◽  
pp. 10077-10092 ◽  
Author(s):  
Changwei Zhang ◽  
Xinghua Sun ◽  
Jun Zhang ◽  
Xianbin Wang ◽  
Shi Jin ◽  
...  

1979 ◽  
Vol 44 ◽  
pp. 41-47
Author(s):  
Donald A. Landman

This paper describes some recent results of our quiescent prominence spectrometry program at the Mees Solar Observatory on Haleakala. The observations were made with the 25 cm coronagraph/coudé spectrograph system using a silicon vidicon detector. This detector consists of 500 contiguous channels covering approximately 6 or 80 Å, depending on the grating used. The instrument is interfaced to the Observatory’s PDP 11/45 computer system, and has the important advantages of wide spectral response, linearity and signal-averaging with real-time display. Its principal drawback is the relatively small target size. For the present work, the aperture was about 3″ × 5″. Absolute intensity calibrations were made by measuring quiet regions near sun center.


Sign in / Sign up

Export Citation Format

Share Document