Term | Acronym | Definition |
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Beam cut | A one-dimensional slice through a two-dimensional radiation pattern, for example with constant θ (see "Coordinate System" below for definition of θ). Common beam cuts are E-, D-, and H-planes (see below). Within each beam cut the co- and cross-polarized response can be measured. | |
Beam deviation factor | BDF | The relation between the offset angle of a feed and the angular offset of the beam. For a flat plat reflector the angles are the same but for curved surfaces they are not. Ref.: Lo, 1960 |
Blockhouse | A cinder-block building near the middle of the Synthesis Telescope array. This building houses the control electronics for the ST with digital electronics inside a screened room. | |
CFI | Canadian Foundation for Innovation | |
CHORD | ||
Co-polarization | The polarization that the antenna is intended to radiate/receive. Commonly-used polarizations are linear and circular. Ref.: IEEE Standard Definitions of Terms for Antennas | |
Coordinate System | A right-handed spherical coordinate system used. Usually the boresight of the telescope beam is aligned along the z axis. Reference |
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Cross-polarization | The polarization orthogonal to the co-polarization. | |
D3A | Deep Dish Demonstrator Array | |
D-plane | For a linearly polarized antenna, the plane at 45° to the E- and H-planes. Cross-polarization is usually largest in this plane. | |
Drift scan | A method for measuring a beam cut through a telescope beam by leaving the telescope stationary and allowing a radio source to pass through the beam. | |
E-plane | For a linearly polarized antenna, the plane containing the electric field vector and the direction of maximum radiation. Ref.: IEEE Standard Definitions of Terms for Antennas | |
FM3 | "Flux Monitor 3"; solar flux monitor telescope north of the Synthesis Telescope track. | |
GRASP | General Reflector Antenna Simulation Program. An electromagnetic simulation program designed for the analysis of multi-surface reflector antennas using Physical Optics and the Physical Theory of Diffraction. | |
HIRAX | ||
Holography | A process where the 2-dimensional complex radiation pattern of an antenna is measured and then Fourier transformed to obtain the field distribution across the aperture. This is often used to determine distortions of reflector surfaces. Ref.: Rahmat-Samii 1984 | |
H-plane | For a linearly polarized antenna, the plane containing the magnetic field vector and the direction of maximum radiation. Ref.: IEEE Standard Definitions of Terms for Antennas | |
Synthesis Telescope | ST | An East-West seven-element interferometer at DRAO which observes at 408 MHz and 1.42 GHz. |