Design and Simulation of V-Type Dipole Antenna
The VHF low band(30MHz-100MHz)is a very important spectrum in radio astronomy.In this band Galactic noise is often quite strong.This thesis introduces the design and simulation of a blade-type vibrator antenna.Antenna operating in 30MHz-70MHz can satisfy the requirement of low-frequency radio observation.A blade-type vibrator antenna based on HFSS simulation software is introduced.The VSWR(voltage standing wave ratio)of antenna satisfies the galaxy noise-limit condition in the working frequency band,and the antenna has the characteristics of simplicity,low cost and easy production.Its a attractive candidate for large lowfrequency radio telescope arrays.
Low frequency radio observation galaxy noise dipole antenna voltage standing wave ratio
Xiaowei Yuan Liang Dong Min Wang Shaojie Guo Guannan Gao
University of Chinese Academy of Sciences Beijing,China Yunnan Observations Chinese Academy of Sciences Kunming,China
国际会议
杭州
英文
1-4
2018-12-03(万方平台首次上网日期,不代表论文的发表时间)