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A parabolic antenna directs radio waves using a parabolic reflector, which is a curved surface having the cross-sectional form of a parabola. The most common design, which is shaped like a dish and is known as a dish antenna or parabolic dish, is the most frequent. A parabolic antenna’s primary benefit is its great directivity. It works in the same way as a searchlight or flashlight reflector in that it directs radio signals in a narrow beam or only receives radio waves from one direction. Parabolic antennas feature some of the greatest gains of any antenna type, allowing them to create the narrowest beamwidths. Because the parabolic reflector must be much larger than the wavelength of the radio waves used to achieve narrow beamwidths, parabolic antennas are used in the high frequency part of the radio spectrum, at UHF and microwave (SHF) frequencies, where the wavelengths are small enough to use conveniently-sized reflectors.
In applications such as microwave relay links that carry telephone and television signals between nearby cities, wireless WAN/LAN links for data communications, satellite communications, and spacecraft communication antennas, parabolic antennas are used as high-gain antennas for point-to-point communications. Radio telescopes also make use of them.
Another common application for parabolic antennas is radar antennas, which need the transmission of a narrow beam of radio waves to find things such as ships, airplanes, and guided missiles, as well as weather detection. With the introduction of home satellite television receivers, parabolic antennas have become a familiar sight in modern countries’ landscapes.
Heinrich Hertz, a German physicist, devised the parabolic antenna when he discovered radio waves in 1887. During his groundbreaking experiments, he employed cylindrical parabolic reflectors with spark-excited dipole antennas at their focal points for both transmitting and receiving.
A point source of radio waves at the focal point in front of a paraboloidal reflector of conductive material is reflected into a collimated plane wave beam along the reflector’s axis, which is how a parabolic antenna works. An entering plane wave parallel to the axis, on the other hand, will be concentrated on a point at the focal point.
A conventional parabolic antenna consists of a metal parabolic reflector with a tiny feed antenna hanging in front of it at its focus and pointing back toward it. The reflector is a metal surface that has been shaped into a paraboloid of revolution and is generally terminated in a circular rim that defines the antenna’s diameter. The feed antenna of a transmitting antenna receives radio frequency current from a transmitter through a transmission line wire and transforms it to radio waves. The feed antenna emits radio waves back toward the dish, which reflect off the dish creating a parallel beam. In a receiving antenna, incoming radio waves bounce off the dish and are focussed to a point at the feed antenna, which transforms them to electric currents that flow to the radio receiver over a transmission line.
At a frequency of 2.5-2.7 GHz, a wire grid-type parabolic antenna is employed for the MMDS data connection. It’s supplied by a vertical dipole hidden behind the boom’s modest metal reflector. Vertically polarized microwaves are emitted.
The reflector can be made of sheet metal, metal screen, or wire grill, and it can be shaped like a circular “dish” or any other form to generate multiple beam shapes. As long as the holes are less than one-tenth of a wavelength, a metal screen reflects radio waves as well as a solid metal surface, hence screen reflectors are frequently employed to minimize dish weight and wind loads. To obtain optimum gain, the shape of the dish must be correct to within a few hundredths of a wavelength, ensuring that waves from various regions of the antenna arrive to the focus in phase. To give the requisite rigidity, large dishes frequently require a supporting truss system behind them.