parabolic dish reflector

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    The Parabolic Reflector Antenna (Satellite Dish)

    Antennas List Antenna Theory(Home) Antenna Basics

    Dishes: Basic Properties Gain Calculations and

    Efficiency Radiation Patterns

    The most well-known reflector antenna is the parabolic reflector antenna, commonly known as a

    satellite dish antenna. Examples of this dish antenna are shown in the following Figures.

    Figure 1. The "big dish" antenna of Stanford University.

    DruckmessumformerDifferenzdruck- Messumformer 0-25 Pa bis 0-100 kPa

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    Figure 2. A random direcTV dish antenna on a roof.

    Parabolic reflectors typically have a very high gain(30-40 dB is common) and low cross

    polarization. They also have a reasonable bandwidth, with the fractional bandwidthbeing at least 5%

    on commercially available models, and can be very wideband in the case of huge dishes (like the

    Stanford "big dish" above, which can operate from 150 MHz to 1.5 GHz).

    The smaller dish antennas typically operate somewhere between 2 and 28 GHz. The large dishes can

    operate in the VHF region (30-300 MHz), but typically need to be extremely large at this operating

    band.

    The basic structure of a parabolic dish antenna is shown in Figure 3. It consists of a feed antenna

    pointed towards a parabolic reflector. The feed antenna is often a horn antennawith a circular

    aperture.

    Figure 3. Components of a dish antenna.

    http://www.antenna-theory.com/antennas/aperture/horn.phphttp://www.antenna-theory.com/definitions/fractionalBW.phphttp://www.antenna-theory.com/definitions/crosspolarization.phphttp://www.antenna-theory.com/basics/gain.php
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    Unlike resonant antennas like the dipole antennawhich are typically approximately a half-

    wavelength long at the frequency of operation, the reflecting dish must be much larger than a

    wavelength in size. The dish is at least several wavelengths in diameter, but the diameter can be on

    the order of 100 wavelengths for very high gain dishes (>50 dB gain). The distance between the feed

    antenna and the reflector is typically several wavelenghts as well. This is in contrast to the corner

    reflector, where the antenna is roughly a half-wavelength from the reflector.

    In the next section, we'll look at the parabolic dish geometry in detail and why a parabola is a desired

    shape.

    Geometry of Parabolic Dish Antenna

    Now we'll try to explain why a paraboloid makes a great reflector. To start, let the equation of aparabola with focal length Fcan be written in the (x,z) plane as:

    This is plotted in Figure 4.

    Figure 4. Illustration of parabola with defining parameters.

    The parabola is completely described by two parameters, the diameter Dand the focal lengthF. We

    also define two auxilliary parameters, the vertical height of the reflector (H) and the max angle

    between the focal point and the edge of the dish ( ). These parameters are related to each other bythe following equations:

    Horn Antenna-In stockStandard Gain Horn,10, 15, 20, 25dB up to 110GHz, Wideband horn, Lens

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    To analyze the reflector, we will use approximations from geometric optics. Since the reflector is

    large relative to a wavelength, this assumption is reasonable though not precisely accurate. We willanalyze the structure via straight line rays from the focal point, with each ray acting as a plane wave.

    Consider two transmitted rays from the focal point, arriving from two distinct angles as shown in

    Figure 5. The reflector is assumed to be perfectly conducting, so that the rays are completely

    reflected.

    Figure 5. Two rays leaving the focal point and reflected from the parabolic reflector.

    There are two observations that can be made from Figure 5. The first is that both rays end up

    travelling in the downward direction (which can be determined because the incident and reflected

    angles relative to the normal of the surface must be equal).

    The rays are said to be collimated. The second important observation is that the path lengths ADE

    and ABC are equal. This can be proved with a little bit of geometry, which I won't reproduce here.

    These facts can be proved for any set of angles chosen. Hence, it follows that:

    All rays emanating from the focal point (the source or feed antenna) will be reflected towards thesame direction.

    The distance each ray travels from the focal point to the reflector and then to the focal plane is

    constant.

    As a result of these observations, it follows the distribution of the field on the focal plane will be in

    phase and travelling in the same direction. This gives rise to the parabolic dish antennas highly

    directional radiation pattern. This is why the shape of the dish is parabolic.

    Finally, by revolving the parabola about the z-axis, a paraboloid is obtained, as shown below.

    http://www.antenna-theory.com/basics/radPattern.html
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    For design, the value of the diameter Dshould be increased to increase the gain of the antenna. The

    focal length Fis then the only free parameter typical values are commonly given as the ratio F/D,

    which usually range between 0.3 and 1.0. Factors affecting the choice of this ratio will be given in

    the following sections.

    In the next section, we'll look at gain calculations for a parabolic reflector antenna.

    Next: Parabolic Reflectors(Page 2)

    Antennas List

    Antennas(Home)

    This page on parabolic dish antennas (satellite dish) is copyrighted. No portion can be reproduced

    except by permission from the author. Copyright antenna-theory.com, 2009-2011, satellite dish,

    parabolic dish antena.

    Horn Antenna-In stockStandard Gain Horn,10, 15, 20, 25dB up to 110GHz, Wideband horn, Lens

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