Analysis of the EMBRACE aperture array antenna by the characteristic Basis Function Method
Paper in proceeding, 2011
This paper describes the use of the Characteristic Basis Function Method for the simulation of large phased array antennas for radio astronomy. It will be shown how the antenna effective area and the receiver noise temperature depend on array size. Also the receiving sensitivity Aeff /T sys normalised with respect to the physical area of the array will be shown for different array sizes and scan angles.
Scan angle
Effective area
Array sizes
Antenna phased arrays
Receiver noise temperatures
Large phased arrays
Antennas
Electromagnetism
Radar astronomy
Aperture arrays
Radio astronomy
Characteristic basis function methods
Author
M. J. Arts
Netherlands Institute for Radio Astronomy (ASTRON)
Rob Maaskant
Chalmers, Signals and Systems, Communication, Antennas and Optical Networks
G. W. Kant
Netherlands Institute for Radio Astronomy (ASTRON)
Proceedings - 13th International Conference on Electromagnetics in Advanced Applications, ICEAA'11, Torino, 12-16 September 2011
959-962 6046469
978-161284978-2 (ISBN)
Subject Categories
Electrical Engineering, Electronic Engineering, Information Engineering
DOI
10.1109/ICEAA.2011.6046469
ISBN
978-161284978-2