B Dong, J Yang, J Dahlström, J Flygare… - … on Antennas and …, 2018 - ieeexplore.ieee.org
In this communication, we present a new optimization and realization of a quadruple-ridge flared horn (QRFH) as a feed for reflector antennas of the square kilometer array (SKA) …
DIL de Villiers, R Lehmensiek - IEEE Transactions on Antennas …, 2022 - ieeexplore.ieee.org
Antenna noise temperature calculation for a reflector antenna system can be a computationally expensive operation if the structure is electrically large. Several …
J Flygare, M Pantaleev - IEEE Transactions on Antennas and …, 2019 - ieeexplore.ieee.org
We present the design, manufacture, and measured performance of a dielectrically loaded quad-ridge flared horn (QRFH) feed for decade bandwidth radio astronomy application. The …
J Flygare, J Yang, AW Pollak… - … on Antennas and …, 2023 - ieeexplore.ieee.org
In this article, we present a novel dielectrically loaded quad-ridge flared horn (QRFH) as a reflector feed with beyond-decade ultrawideband performance. The dielectric is machined in …
The accuracy of geodetic Very Long Baseline Interferometry (VLBI) is affected by water vapour in the atmosphere in terms of variations in the signal propagation delay at the …
L Marzall, P Danielson, G Lasser… - IEEE Antennas and …, 2021 - ieeexplore.ieee.org
This letter presents the design and characterization of an octave-bandwidth, small-aperture, linearly polarized, high-gain horn antenna operating in the 6–12 GHz band for active arrays …
X Du, T Johnson, T Landecker… - IEEE Transactions on …, 2021 - ieeexplore.ieee.org
We describe a new type of ultrawideband feed antenna based on nested coaxial waveguides. The feed is for radio astronomy applications and covers two closely spaced …
R Lehmensiek, DIL De Villiers - 2022 16th European …, 2022 - ieeexplore.ieee.org
The design of an all-metal quadruple-ridged flared horn (QRFH) feed antenna for the ngVLA optics is presented. The feed is required to operate over the 1.2 GHz-3.5 GHz frequency …
Reflector-based radio telescopes are used as tools for observations in both radio astronomy and space geodesy. To observe the weak sources in space, highly sensitive receivers …