Solar panel scattering effects on reflector antenna performance

1997 ◽  
Vol 33 (8) ◽  
pp. 650 ◽  
Author(s):  
S.U. Hwu ◽  
L.A. Johnson ◽  
R.J. Panneton
1992 ◽  
Author(s):  
SHIAN HWU ◽  
LARRY JOHNSON ◽  
JON FOURNET ◽  
ROBERT PANNETON ◽  
DONALD EGGERS ◽  
...  

2019 ◽  
Vol 2019 ◽  
pp. 1-15
Author(s):  
Binbin Xiang ◽  
Congsi Wang ◽  
Peiyuan Lian

In this paper, a method based on the Zernike distribution and the optical aberration is proposed to investigate the effects of the distribution characteristics of surface distortions of a reflector antenna on its electromagnetic performance (EMP). For large-scale errors, an analytical model is introduced to describe the arbitrary distortions, based on the orthogonal Zernike polynomials. The effects of error distribution described by the Zernike series on typical EMP are analyzed. The numerical results indicate that the distortions in the distribution feature of defocus or spherical aberration have a greater impact on gain, and the distribution feature of tilt or coma mainly influences boresight offset; the distribution feature of defocus, astigmatism, and spherical aberration has a greater impact on sidelobe levels. The results indicate that the beam contour patterns are related to the distribution forms of distortions and are similar with the same aberration feature. On the basis of the Seidel aberration, the relationships between typical EMP and the aberration coefficient are presented. Based on these, the error profile of the primary influence and the approximate feature of EMP can be determined, and the antenna performance can be predicted in a simple manner.


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