The measured results are as follows: the antenna gain is 21.5 dB with an aperture efficiency of about 46%,the reflection coefficient is about 0.07~0.39 in the range of 6.5~7.5 GHz.
The calculated results of the antenna are as follows: the antenna gain is 22.2 dB with an aperture efficiency of 53.7%,the reflection coefficient is 0.07 at the center frequency and less than 0.3 in the range of 6.5~7.5 GHz.
In the range of 3.6~4.1 GHz,the experiment result shows the antenna VSWR is below 1.4,the antenna gain is over 22.9 dB and the aperture efficiency is more than 65%.
At 4.0 GHz,the calculated aperture efficiency reaches 78.2% and the axial ratio at the normal direction is 1.73.In the range of 3.8 GHz to 4.2 GHz,the aperture efficiency is over 73.2%,the axial ratio is below 2.0,the reflectance is less than 0.28,and the radiation efficiency is more than 93%.
In the range of 3.7 -4.05 GHz, the simulated result shows an antenna VSWR of below 1.5. At 4.0GHz, antenna Directivity is 24.26 dB and the aperture efficiency is 78.4%, and the axial ratio is 1.65. In the end, array antenna's power capacity is analyzed and simulated, which proves that this array antenna can radiate high power microwave of 1GW.
Slotted waveguide array antenna has been used widely in radar and microwave communication systems because of their flat, compact structure, power capacity, realizing low side-lobe and very low side-lobe.
Since the double-ridged horn antenna owns many seductive characteristics, such as ultra broadband, relatively small size, high calibre efficient and gain etc.
The computation results compared with our previous method "Multi-Step Amplitude Quantization (MSAQ)" on peak sidelobe level, aperture efficiency, normalized input power and sidelobe degradation with tolerance are given.
This expression showed that the average brightness temperature of antenna aperture related with three factors: the noise temperature of noise source, the reflection coefficient of noise source, and the aperture efficiency.
The title telescope - in operation since 1982 - gives a surface accuracy of better than 0.2 mm (r.m.s.), with an aperture efficiency of about 25% at 115 GHz.
This paper deals mainly with the project of high performance antenna with only sub-reflector modified and simple step dual mode conical horn as feeder source, and its practicable results have already achieved on antennas of microwave relay communication system. A brief introduction of the development process and some basic points regarding scheme selection are presented. The gist of antenna design, the performance of each individual part and the practically measured results are also given. Satisfactory expe...
Several representations of the field-correlation theorem are derived wi- th their application conditions indicated, and an illustrative example is presented. The example shows that the fie1d-correlation method is a very effective approach when it is applied to shape the subrefleetor of cassegrain antennas, and that the theoretical impro- vement of aperture efficiency by greater than O.5 dB has been achieved.
A new concept on the top-plate blockage in a dual-reflector antenna system is described in this paper, It is shown that a "top-plate shadow circle" will be produced on the main reflector aperture when a matching top-plat is placed on the shaped subreflector. Thus, the aperture blockage of the main reflector is augmented and the related antenna efficiency is decreased. To auoid this effect the relevant equation has been corrected.