Strategy and Overview for Development of Beyond-Decade-Bandwidth Quad-ridge Flared Horns for Radio Astronomy
Paper in proceeding, 2021

This paper considers the potential of the dielectrically loaded Quad-ridge Flared Horn (QRFH) feed to provide continuous beyond-decade bandwidth in reflector telescopes for radio astronomy. An overview of the beam pattern evolution over frequency in a recent ultra-wideband feed designed for 1.5–15.5 GHz is presented.

Shape

Bandwidth

Receiving antennas

quad-ridge flared horn

ultra-wideband

Telescopes

Propagation losses

Sensitivity

dielectric load

Radio astronomy

reflector feed

radio astronomy

Author

Jonas Flygare

Chalmers, Space, Earth and Environment, Onsala Space Observatory, Electronics Laboratory

Jian Yang

Chalmers, Electrical Engineering, Communication and Antenna Systems, Antennas

15th European Conference on Antennas and Propagation (EuCAP 2021)

978-88-31299-02-2 (eISSN)

9410964

15th European Conference on Antennas and Propagation (EuCAP 2021)
Dusseldorf, Germany,

RadioNet 4

European Commission (EC), 2017-01-01 -- 2020-12-31.

Infrastructure

Onsala Space Observatory

Subject Categories

Electrical Engineering, Electronic Engineering, Information Engineering

DOI

10.23919/EuCAP51087.2021.9410964

More information

Latest update

5/24/2021