scholarly journals Optimal multiplexing gain of K-user line-of-sight interference channels with polarization

Author(s):  
Sung ho Chae ◽  
Sang Won Choi ◽  
Sae-Young Chung
2011 ◽  
Vol 59 (10) ◽  
pp. 2905-2915 ◽  
Author(s):  
Sung Ho Chae ◽  
Sang Won Choi ◽  
Sae-Young Chung

Frequenz ◽  
2021 ◽  
Vol 0 (0) ◽  
Author(s):  
Darko Cvetkovski ◽  
Thomas Schlegel ◽  
Eckhard Grass

Abstract For the next generation wireless networks, backhaul links with data rates of several Gbit/s are required. Line-of-Sight-MIMO with optimally arranged antennas can exploit the full multiplexing gain of orthogonal MIMO streams to achieve high throughput, as shown in recent works utilizing the 60 GHz mm wave band. In contrast, conventional MIMO systems operating at sub-6 GHz carrier frequencies, as utilized in modern WLAN networks, rely on rich scattering channels to enable reliable transmissions. In this work, we explore the feasibility of applying the LoS-MIMO concept to wireless single-carrier links operating at sub-6 GHz frequencies. For this, we investigate the sub-6 GHz LoS-MIMO channel in a 4 × 4 MIMO configuration by performing measurements in an anechoic chamber and an outdoor backhaul-like environment. In addition, different adaptive equalizers are evaluated. The results show, that the LoS-MIMO concept holds for sub-6 GHz frequencies both in pure LoS and in outdoor environments. It provides high multiplexing gain; however, the multipath propagation limits the potential performance of the equalizers in terms of achievable BER.


1967 ◽  
Vol 31 ◽  
pp. 171-172
Author(s):  
Th. Schmidt-Kaler

The integralNHof neutral-hydrogen density along the line of sight is determined from the Kootwijk and Sydney surveys. The run ofNHwith galactic longitude agrees well with that of thermal continuous radiation and that of the optical surface brightness of the Milky Way.


1994 ◽  
Vol 144 ◽  
pp. 421-426
Author(s):  
N. F. Tyagun

AbstractThe interrelationship of half-widths and intensities for the red, green and yellow lines is considered. This is a direct relationship for the green and yellow line and an inverse one for the red line. The difference in the relationships of half-widths and intensities for different lines appears to be due to substantially dissimilar structuring and to a set of line-of-sight motions in ”hot“ and ”cold“ corona regions.When diagnosing the coronal plasma, one cannot neglect the filling factor - each line has such a factor of its own.


1968 ◽  
Author(s):  
ANDREW J. ECKLES ◽  
THOMAS A. GARRY ◽  
WILLIAM C. MULLEN

2016 ◽  
Vol E99.B (6) ◽  
pp. 1362-1370 ◽  
Author(s):  
Maki ARAI ◽  
Tomohiro SEKI ◽  
Ken HIRAGA ◽  
Kazumitsu SAKAMOTO ◽  
Tadao NAKAGAWA
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