Design of Ultra-Wideband Phased Array Feed for Radio Telescope
Paper i proceeding, 2020

This paper presents an ultra-wideband Phased Array Feed (PAF) based on novel flat bend crossed dipole fed by 50Ohm coaxial line. The PAF is dual-polarized and made from all-metal to minimize Ohmic losses and simplify cryogenic integration. It is optimized for 1-2 GHz band and can be good PAF candidate for the Five hundred meter Aperture Spherical Telescope (FAST) and Qi Tai Telescope (QTT) as well as other radio telescopes.

Författare

Jin Fan

Chinese Academy of Sciences

Yihua Yan

Chinese Academy of Sciences

Kai Zhu

Chinese Academy of Sciences

Heng Qian Gan

Chinese Academy of Sciences

Linjie Chen

Chinese Academy of Sciences

Jian Yang

Chalmers, Elektroteknik, Kommunikations- och antennsystem, Antennsystem

Hailin Cao

Chongqing University

Bin Li

Shanghai Astronomical Observatory

Jun Ma

Chinese Academy of Sciences

2020 33rd General Assembly and Scientific Symposium of the International Union of Radio Science, URSI GASS 2020

9232362

33rd General Assembly and Scientific Symposium of the International Union of Radio Science, URSI GASS 2020
Rome, Italy,

Ämneskategorier

Astronomi, astrofysik och kosmologi

Annan fysik

Diskret matematik

DOI

10.23919/URSIGASS49373.2020.9232362

Mer information

Senast uppdaterat

2021-01-07