Everything about Microwave Antenna totally explained
The
parabolic antenna is a high-gain reflector antenna used for radio, television and data communications, and also for radiolocation (
RADAR), on the
UHF and
SHF parts of the electromagnetic spectrum. The relatively short wavelength of electromagnetic (radio) energy at these frequencies allows reasonably sized reflectors to exhibit the very desirable highly directional response for both receiving and transmitting.
A typical parabolic antenna consists of a
parabolic reflector illuminated by a small
feed antenna.
The reflector is a metallic surface formed into a
paraboloid of revolution and (usually) truncated in a circular rim that forms the diameter of the antenna. This paraboloid possesses a distinct
focal point by virtue of having the
reflective property of parabolas in that a point light source at this focus produces a parallel light beam aligned with the axis of revolution.
The feed antenna is placed at the reflector focus. This antenna is typically a
low-gain type such as a
half-wave dipole or a small
waveguide horn. In more complex designs, such as the
Cassegrain antenna, a sub-reflector is used to direct the energy into the parabolic reflector from a feed antenna located away from the primary focal point. The feed antenna is connected to the associated radio-frequency (RF) transmitting or receiving equipment by means of a
coaxial cable transmission line or hollow
waveguide.
Considering the parabolic antenna as a circular
aperture gives the following approximation for the maximum gain:
»
or
»
where:
» is power gain over
isotropic
is reflector diameter in same units as wavelength
» is
wavelength
Practical considerations of
antenna effective area and
sidelobe suppression reduce the actual gain obtained to between 35 and 55 percent of this theoretical value. For theoretical considerations of mutual interference (at frequencies between 2 and c. 30 GHz - typically in the
Fixed Satellite Service) where specific antenna performance hasn't been defined, a
reference antenna based on Recommendation
ITU-R S.465 is used to calculate the interference, which will include the likely sidelobes for off-axis effects.
Applying the formula to just one of the 25-meter-diameter
VLA antennas shown in the illustration for a wavelength of 21 cm (1.42 GHz, a common
radio astronomy frequency) yields an approximate maximum gain of 140,000 times or about 50 dBi (
decibels above the
isotropic level).
With the advent of
TVRO and
DBS satellite television, the parabolic antenna became a ubiquitous feature of urban, suburban, and even rural, landscapes. Extensive terrestrial microwave links, such as those between cellphone
base stations, and wireless WAN/LAN applications have also proliferated this antenna type. Earlier applications included ground-based and airborne
radar and
radio astronomy. The largest "dish" antenna in the world is the
Arecibo Observatory's
radio telescope at
Arecibo, Puerto Rico, but, for beam-steering reasons, it's actually a
spherical, rather than parabolic, reflector.
Structure
The reflector dish can be solid, mesh or wire in construction and it can be either fully circular or somewhat rectangular depending on the radiation pattern of the feeding element. Solid antennas have more ideal characteristics but are troublesome because of weight and high wind load. Mesh and wire types weigh less, are easier to construct and have nearly ideal characteristics if the holes or gaps are kept under 1/10 of the wavelength.
More exotic types include the off-set parabolic antenna, Gregorian and Cassegrain types. In the off-set, the feed element is still located at the focal point, which because of the angles utilized, is usually located below the reflector so that the feed element and support don't interfere with the main beam. This also allows for easier maintenance of the feed, but is usually only found in smaller antennas.
The Gregorian and Cassegrain types, sometimes generically referred to as "dual optics" antennas, utilize a secondary reflector, or "sub-reflector", allowing for better control over the colimnated beam as well as allowing the antenna feed system to be more compact. These antennas are usually much larger where prime focus and off-set construction are not as practical. The feed element is usually located in a "feed horn" which protrudes out from the main reflector. This setup is used when the feed element is bulky or heavy such as when it contains a pre-amplifier or even the actual receiver or transmitter. Parabolic antenna theory closely follows optics theory. So a Gregorian antenna can be identified by the fact that it uses a concave sub-reflector, while a Cassegrain antenna uses a convex sub-reflector.
Feeding parabolic antennas.
The actual 'antenna' in a parabolic antenna, that is, the device that interfaces the transmission line or waveguide containing the radio-frequency energy to free space, is the feed element. The reflector surface is entirely passive. This feed element should usually be at the center of the reflector at the focal point of that dish. The focal point is the point where all reflected waves will be concentrated. The focal length
(distance of focal point from the center of the reflector) is calculated with the following equation:
»
where:
» is the focal length of the reflector
is reflector diameter in same units as wavelength
» is depth of the reflector
The radiation from the feed element induces a current flow in the conductive reflector surface which, in turn, re-radiates in the desired direction, perpendicular to the directrix plane of the paraboloid. The feed element can be any one of a multitude of antenna types. Whichever type is used, it must exhibit a directivity that efficiently illuminates the reflector and must have the correct polarization for the application -- the polarization of the feed determining the polarization of the entire antenna system. The simplest feed is a half-wave dipole which is commonly used at lower frequencies, sometimes in conjunction with a closely coupled parasitic reflector or "splash plate". At higher frequencies a
horn-type becomes more feasible and efficient. To adapt the horn to a coaxial antenna cable, a length of waveguide is used to effect the transition.
Further Information
Get more info on 'Microwave Antenna'.
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