Satellite Antenna

or Satellite Dish The reflective surface that gathers and concentrates the satellite's signal to the electronics located in the front-end.

LNB

The amplifier located in the front-end of the satellite system. C band is measured in degrees Kelvin and Ku band is measured in decibles. With a little fancy math, the measurements can be converted back and forth. Point of reference: whether C band or Ku band, the lower the measurement in decibles or Kelvin, the better the picture.

AUDIO SIGNAL-TO-NOISE

The subcarrier audio S/N ratio is a measure of audio signal power relative to noise power at the output of a satellite receiver. It depends upon factors such as the peak deviation of the subcarrier expressed in kHz, the maximum baseband audio frequency in kHz, the center frequency of the subcarrier in MHz, the de-emphasis improvement factor of the audio broadcast in dB as well as the peak deviation of the main carrier by the subcarrier in MHz, the intermediate frequency (IF) pre-detection or receiver bandwidth in MHz and the downlink C/N ratio. In this calculation, like that of the video S/N ratio, the receiver is assumed to be operating above the non-linear threshold region and that sufficient bandwidth is available to adequately accommodate the audio signal prior to its demodulation by the satellite receiver.

Feed Horn

The part between the dish and the LNB that gathers and channels the signal to the LNB.

Actuator or Positioner

The motorized assembly that positions the antenna to the selected satellite.

IRD

(Integrated Receiver Descrambler) The box on top of the TV that selects the channels, controls the dish movement and houses the VC descrambler.

Ribbon Cable

The cable needed to receive the signal from the dish, control the feed horn and control the dish position.

Coax Cable

The round wire used by the cable company to deliver their services to your TV set.

Servo Motor

The small motor that mounts to the feed horn to select the polarity of the satellite signal.

Polarity

Satellite signals are broadcast in a couple different ways. The most common signal is a horizontal polarity or a vertical polarity. The signal may also be broadcast in a clockwise or a counterclockwise format. For example: C band broadcasts 12 channels on vertical polarity and 12 channels on horizontal polarity totaling 24 channels.

C band

A 4 GHz frequency that satellites broadcast on. Most commonly used for broadcasting network programming and popular cable services.

Ku band

A 12 GHz frequency that satellites broadcast on. More commonly used for broadcasts that are live and unedited.

DBS

Ku band DBS frequency that Direct TV and USS Hubbard broadcast on to the RCA, SONY, Uniden and Toshebia satellite antennas. EchoStar will soon be broadcasting on this same frequency.

Inclinometer

Tool that measures the elevation of an object in degrees.

Infrared remote

The remote control that works the IRD if it is in the line of sight.

UHF remote

The remote control that works the IRD from up to 150' away and through walls. Example: if you have a second television located in the bedroom and it is connected to the IRD, then you can control the IRD from that bedroom.

VCRS

Descrambler The defacto standard descrambler for residential C band services available in the USA. This unit is exclusively manufactured by General Instruments.

Diplexer

The special signal combiner/spliter that brings together and separates the satellite signal and the local

Actuators

Actuators provide the mechanical drive to allow an antenna to scan the arc of satellites under remote control. In the early 1980s there were only a limited number of satellites in the geostationary orbit over North America so most antennas were either fixed on one target or hand-cranked between communication spacecraft. However, as more satellites began to relay television programming, antennas had to be moved from one satellite to another. Manually moving a three or four meter dish in, for example, cold and wet weather was not an attractive proposition. In addition, even when only one satellite is to be targeted, inclined orbit tracking systems must sometimes be used. Many systems feature either linear or horizon-to-horizon actuators. Linear actuators have a telescoping arm that moves within a fixed external tube. Horizon-to-horizon actuators are attached to the base of an antenna and are solidly constructed to generate the torque necessary to rotate a dish and to allow minimal movement in winds or under other loads such as heavy snows. When designing a system to receive satellites close to the horizon it is important to realize that linear actuators typically has a more limited range of motion than a horizon-to-horizon devices.

AUDIO SIGNAL-TO-NOISE

The subcarrier audio S/N ratio is a measure of audio signal power relative to noise power at the output of a satellite receiver. It depends upon factors such as the peak deviation of the subcarrier expressed in kHz, the maximum baseband audio frequency in kHz, the center frequency of the subcarrier in MHz, the de-emphasis improvement factor of the audio broadcast in dB as well as the peak deviation of the main carrier by the subcarrier in MHz, the intermediate frequency (IF) pre-detection or receiver bandwidth in MHz and the downlink C/N ratio. In this calculation, like that of the video S/N ratio, the receiver is assumed to be operating above the non-linear threshold region and that sufficient bandwidth is available to adequately accommodate the audio signal prior to its demodulation by the satellite receiver.

Azimuth angle

The azimuth angle is the compass bearing towards a communication satellite. In order to obtain a useful result, the calculated azimuth angle must be corrected for local magnetic deviation. This program incorporates the powerful and useful feature of calculating magnetic deviation for any site on the surface of the earth.

A/V Switching

Feature that allows users to connect one or more sources such as a VCR, camera and/or laser videodisc player and select which source will be monitored.

Antenna

Parabolic dish designed to collect electromagnetic signals from a satellite.

Aperture Beamwidth

Dish diameter. A 10-foot dish has an aperture of 10 feet. The beamwidth of a dish antenna is the angle of sky which can be illuminated (picked up or sent out) by the dish. Within that arc satellites can be seen from the TVRO dish. Large dishes have narrow beamwidths, which reduces noise form its sides. Samll dishes have wider beamwidths, meaning that they are noisier but easier to aim. Table of Contents

Audio Subcarrier

Carrier wave that transmits audio information.

Auto Tracking

IRD (integrated receiver-decoder) feature that automatically locates and stores all satellite positions into memory.

Auto Tuning

IRD feature that automatically adjusts the dish position and antenna polarity for best picture.

Automatic Frequency Control

Circuit that locks onto a frequency to eliminate drifting off channel.

Azimuth-Elevation (Az-El)

Antenna mount that allows dish movement in both a horizontal plane and vertically in elevation to locate satellites.

Backhaul

This is an uplink of live events such as baseball games, news links, special events, etc. It is usually a location where special feeds occur and most always are delivered without commercial breaks.

Beam Polarity

Signals are almost always transmitted from geosynchronous communication satellites in either linear or circular polarity formats. The use of beam polarities that can be distinguished by satellite reception systems allows for "frequency re-use" whereby the same frequency can be used on each beam. Similarly satellites that transmit more resticted spot beam footprints can re-use frequencies in widely dispersed geographical areas.

Beamwidth

A satellite receive dish is characterized by a half-power beamwidth. The signal is received with most power directly along the dish boresight. At increasing greater angles from the boresight, detected signal power drops. The half-power beamwidth is the angular separation between these -3 dB points on the main lobe. Larger antennas have more narrow beamwidths; likewise dishes that receive higher frequency signals have more narrow beamwidths.

Backhaul

Term applied to the satellite signal sent back to a TV station when a sports "home team" is playing a game on the road. Table of Contents

Barker Channel

A term used for an audio advertisement on a frequency that is automatically picked up when tuned to a scrambled channel. Table of Contents

Baseband

The basic direct 6 Mhz output signal from a television camera, satellite receiver or VCR.

Bird

Nickname for a satellite

Block Downconversion

A process of lowering the entire band of frequencies in one step to an intermediate range. Allows receivers in multiple receiver system to independently select channels on a satellite.

Bullet Amplifier

Small device used to increase signal power and offset signal loss caused by coaxial cable and splitting devices.

Buttonhook

A rod shaped like a question mark that supports the feedhorn and LNA. Feedhorns and LNAs also can be supported by three- or four-leg mounts affixed to the edges of the satellite dish.

C-Band

The microwave frequency band that ranges from 1 GHz to above 30 GHz includes the familiar C-band range of frequencies, 3.40 to 6.425 GHz.

Carson's Rule

Carson's Rule is an approximate method to calculate the "minimum" bandwidth in a frequency modulated satellite signal so a high-fidelity, sharp picture will be delivered. While reducing the bandwidth below that recommended by Carson's Rule is a common practice and does result in a higher video S/N ratio, this is at the expense of streaking in fast moving scenes and overall picture sharpness. A concurrent loss of audio fidelity also can occur. The greater the number of subcarriers, the greater the Carson's bandwidth required. This calculation of minimum bandwidth does not include the smaller effect of the deviation of a satellite signal caused by the energy dispersal waveform.

Cassegrain Dish

The Cassegrain or "back-fire" dish also has a parabolic surface but then redirects the incoming satellite signals via a second reflector, the hyperbolic subreflector, down a waveguide to an LNB mounted in a rear position. This type, often more expensive than more common prime-focus dishes, is usually installed in commercial earth stations. The Cassegrain geometry can be very useful in hot climates because the LNB is mounted behind the reflective surface where it is protected from the direct rays of the sun, remains relatively cool and functions more efficiently.

Channel Bandwidth

The channel bandwidth is the frequency range in which the energy of a communications signal is concentrated. The bandwidth is centered on the center frequency. For example, the bandwidth of a typical C-band transponder is 36 MHz, more than enough frequency space to transmit a high fidelity video signal via satellite. However, channel bandwidths as low as a half-transponder, 18 MHz, or less are also occasionally used. In addition, while many transponders have 54 and 72 MHz bandwidths, in particular on many Ku-band links, the bandwidth of each video signal may be centered on the upper or lower half of the transponder and occupy typically 27 to 36 MHz or less.

Circular Polarization

Signals downlinked from communications satellites often circularly polarized. The electric and magnetic fields rotate in a circular motion as they travel through space, analogous to movement along a spiral. The direction of rotation determines the type of circular polarization. A signal whose electric or magnetic fields rotate in a right-hand direction is termed right-hand circular polarized (RHCP); a signal rotating in the left-hand direction is termed left-hand circular polarized (LHCP). The use of circular polarization eliminates the need for skew adjustment in the reception equipment. In addition, circularly polarized signals are also not subject to Faraday Rotation, the rotation of polarity caused by the Earth's magnetic field and/or magnetic storms when a signal travels through the atmosphere. This resistance to Faraday rotation makes circular polarization eminently more suitable than linear polarization for voice and data relays via satellite. Adjacent high-powered direct broadcast Ku-band satellites in Europe have been configured to use opposite senses of circular polarization to decrease interference between satellites by virtue of cross-polarization discrimination built into the feed. Table of Contents

Circular Polarizer

Circular polarizer usually consist of two internal probes set at right angles to each other to detect the incoming signal. The output of one is delayed 1/4 wavelength relative to the other so the signals are added to detect one sense of polarization (LHCP or RHCP); reversing the delay detects the other polarity sense. A pin diode switch controlled by a small dc voltage can be used to select polarity. Such devices can be easily built into the throat of an LNB. Polarizers that combine this method with the mechanically rotated probe can switch at will between both linear and both circular formats. A scalar feed can be modified to receive circularly polarized signals, albeit with a 2 to 3 dB performance penalty. This is accomplished by inserting a dielectric slab, typically a small rectangular piece of teflon or similar material, into the circular waveguide at a 45° angle from the position of the probe. It acts by "delaying" the circularly polarized signal thus translating it into a linearly polarized signal. Standard scalar feed cannot distinguish between LHCP and RHCP transmissions but this simple retrofit permits detection and discrimination of both circular polarity senses.

Coaxial Cable

Coaxial cables connect the output of the LNB with the input of the satellite receiver. Both the signal and the switching voltage for electronically switched polarizers can be transmitted via coax. Coax is characterized by a characteristic impedance and signal losses per unit distance. 75-ohm cables are nearly always in satellite reception systems. Signal losses vary with the construction of the cable as well as the frequency. Higher frequencies are attenuated more strongly. For example, RG-6 coax has approximately 24.6 dB and 27.9 dB per 100 meters at a signal frequency of 950 and 1450 MHz, respectively.

Color Television Standards

The color television standards, NTSC, PAL and SECAM, were developed during the early days of color television. The NTSC-M and PAL-M formats both have 60 Hertz field frequencies and 525 line scanning. All other conventional standards use a 50 Hertz field frequency and 625 line scanning. Except for the SECAM-L format, all use negative video modulation and FM sound. The characteristics of these variety of systems used is outlined on the following page:

Color Television Standards

System Video Bandwidth Baseband Channel Primary Sound (MHz) Width (MHz) Carrier (MHz) NTSC-M 4.2 6.0 4.5 PAL-B 5.0 7.0 5.5 PAL-D1 6.0 8.0 6.5 PAL-G 5.0 8.0 5.5 PAL-H 5.0 8.0 5.5 PAL-I 5.5 8.0 6.0 PAL-I1 5.5 8.0 6.0 PAL-M 4.2 6.0 4.5 PAL-N 4.2 6.0 4.5 SECAM-B 5.0 7.0 5.5 SECAM-D 6.0 8.0 6.5 SECAM-G 5.0 8.0 5.5 SECAM-H 5.0 8.0 5.5 SECAM-K 6.0 8.0 6.5 SECAM-K1 6.0 8.0 5.5 SECAM-L 6.0 8.0 6.5

Dielectric Feed

The dielectric feed is a recently introduced innovation and a viable wideband alternative to a conventional scalar feed. It is essentially a microwave lens designed to have a radiation pattern with relatively sharp edges that inserts directly into the mouth of a waveguide at the entrance to the LNB. This improvement in dish illumination and a better balancing of the E and H-fields result in an increase in system efficiency from typically 60% to 80%. This translates into the need for a dish with 25 2.306125e-82ss surface area.

Dish Aperture

The diameter or aperture of a satellite receive dish determines the amount of signal collected from a communication satellite. The larger the aperture, the more signal is intercepted and therefore the higher the gain. The aperture of a prime focus dish can be partially blocked by the feed/LNB and its support structure. For this reason, offset fed antennas are more efficient at the lower end of dish apertures, less than about 1 meter.

Dish Beamwidth

Every dish and feed system has a "fingerprint," its beam pattern, that describes how signals are received from its surroundings. This pattern depends upon the aperture and accuracy of the dish as well as upon signal frequency. Surface imperfections generally tend to widen the main lobe and increase side lobes.

Dish Efficiency

Efficiency is a measure of the percentage of signal actually captured by the dish feed system. An ideal feed would capture all the signal that the dish intercepts. In the real world some signal is blocked by the feed structure and the reflective surface is never perfectly accurate. As a result, typical efficiencies range from lows of 40% for inferior products to 70% or even higher for excellent quality prime-focus antennas. Offset fed parabolic antennas can have efficiencies in excess of 80%.

Dish f/D Ratio and Depth

The depth of a parabolic dish is a measure of the distance from the dish to the feed/LNB structure. Deep dishes have an f/D, the ratio of focal length to diameter, of 0.25 to 0.31 while shallow dishes range from 0.37 to 0.45. When f/D equals 0.25 the feed sits along the line between the edges of the dish. In general, everything else being equal, deeper dishes have smaller side lobes because the feed and LNB are closer to the reflective surface and thus are better screened from the surrounding environment.

Dish Focal Distance

The focal distance of a parabolic dish is the distance from the center of the reflective surface to the focal point, the location where all signals arriving along the dish boresight are focused to a single point.

Dish Gain

Gain is the factor by which an incoming signal is concentrated when it reaches the focal point. A higher gain dish would be required to receive signals from a weaker satellite. Gain is measured in decibels relative to an "isotropic antenna," one that would receive signals from all directions equally well. An isotropic antenna has a gain of 0 dBi, equal to a concentration factor of 1. A dish, for example, with a gain of 30 dBi, concentrates incoming signals by a factor of 1,000. The gain calculations, accessible from the CALCULATIONS and subsequently RECEIVE SYSTEM and ANTENNA PARAMETERS menus is measured in dBi. Gain increases as dish size increases since more signal can be intercepted, just like a larger bucket can collect more rain. Higher gain dishes are often required to receive the very weak signals from Intelsat global or hemispheric beams or from areas far off the boresight of spot or zone beams. For example, if reflective surface area is doubled, so is its gain. Gain also increases with signal frequency, actually the square of the frequency. A dish would thus have 9 times more gain at Ku-band than at C-band since the frequency is three times higher. The gain of a dish also depends upon its surface accuracy. Small distortions in the reflective surface, can cause substantial decreases in gain. Therefore, a dish that has a large number of deep welts or ripples will behave more poorly than one that is smooth and more closely approximates its designed shape. Signals striking a dent would be reflected away from the focal point. This loss of gain with surface imperfections becomes even more important at higher frequencies. Ku-band dishes must be more accurate than those for C-band reception. A receive dish intercepts and concentrates signals from transponders with power outputs ranging from 6 to over 100 watts that have been attenuated by approximately 200 dB on their journey earthward. While system performance improves as dish gain increases, below a minimum gain, even the best LNB cannot compensate enough to adequately capture the signal essential to reconstruct a satellite broadcast. Table of Contents

Dish Noise Temperature

Satellite dishes not only detect the desired satellite broadcast but also noise from natural and man-made sources. Noise from the surrounding environment and electronic equipment works in the opposite direction to gain and must be avoided if at all possible. A portion of this noise enters via the dish side lobes; a smaller amount, predominantly that from outer space, enters via the main lobe. Dish noise temperature is a measure of how much noise is detected from the surrounding environment. The warm ground emits microwave radiation so noise temperature increases as a dish is pointed at increasingly lower elevation angles. Thus the reception from a satellite located closer to either horizon would be poorer than one from one located higher in the arc. Noise also decreases as dish size increases, since larger dishes have smaller side lobes and a more narrow main lobe.

db and dBW

dB (decibels) is the standard unit for expressing relative power, voltage or current. dBW indicates actual power of one signal compared to a reference of 1 watt. In satellite dishes, an increase of 3dBW equals a doubling of gain.

DBS

Direct Broadcast Satellite, a new method of program delivery by which signals are sent directly to small (18-inch to 3-feet diameter) home dishes form high-powered (120- to 200-watts per transponder) Ku-band satellites, as opposed to "over the air" broadcast, cable delivery or lower-powered C-band or Ku-band transmissions. PrimeStar is a quasi-DBS service, while USSB and DirecTV, planned for 1994, and ExpressVu, planned for 1995, will be true DBS services.

Decoder

A device that restores a signal to its original form after it has been encoded. Also called a descrambler or a decryption device. Table of Contents

Demodulator

A device that extracts signals from transmitted carrier waves.

Dig. Vid. Compression

(DVC) - Process by which multiple video services, or channels, are broadcast on one satellite transponder. Performed by turning analog audio and video into digital (computer) information for broadcasting.

Digital Audio

Method used to transmit audio on scrambled channels.

Dish

The part of the satellite dish antenna that collects, reflects, and focuses the satellite signal into the LNB.

DNR

Dynamic Noise Reduction is a filter circuit that reduces high audio frequencies such as hiss.

Dolby Surround Sound

Four-channel audio format, which is encoded in the two audio channels of virtually every motion picture, music video and movie on television.

Downconverter

A circuit that lowers the high-frequency signal to a lower, intermediate range. The three types of downcoversion are signal, dual and block downconversion.

Downlink

Term used to describe the retransmitting of signals from a satellite back to Earth.

Drip Loop

Several inches of slack in a cable that prevents water from collecting on the cable or running along the surface of the cable. A drip loop between the LNB and the entry point into the building also allows some free movement of the dish while adjusting it.

DSS

Digital Satellite System.

DSS Receiver

Receives, processes, and converts the satellite signal into picture and sound.

DTH

Direct-to-Home broadcasting of television signals using a satellite to reflect the program signal to a home-installed dish. Table of Contents

Dual Band Feedhorn

A feedhorn that can receive both C-band and Ku-band signals.

Dual Feedhorn

A feedhorn that can simultaneously receive both horizontally and vertically polarized signals.

Effective Isotropic Radiated Power - EIRP

The term effective isotropic radiated power (EIRP) is derived from the word isotropic which means equal in all directions. Effective isotropic radiated power means the power levels that would be received at any location if an antenna were radiating equally in all directions. Therefore, a 37 dBw EIRP reading means that a perfect antenna would direct 37 dBw or 5012 watts per square meter in all directions. The reason that a transponder having rather limited power, typically in the 8 to 150 watts range, can apparently have such a high EIRP stems from the fact that this power is not radiated equally in all directions but is concentrated in a narrow beam aimed at the earth below. Ku-band transponders having a total power of 50 watts have EIRPs as high as 48 or 49 dBw when this power is directed into a tightly aimed zone beam. EIRP levels refer to the power of signals measured at the satellite downlink antenna. In the example above, 5012 watts per square meter would be directed towards a selected location on earth below.

Elevation Angle

The angle at which a dish points above the local horizon is termed the elevation angle. For any site on the globe the largest elevation angle occurs when aiming at those satellites at the most southerly (in the northern hemisphere) or the most northerly locations. For a site at the equator, the elevation angles is a constant 90 degrees.

Earth Ground

Conducting connection to the earth for an electrical charge so that the electrical charge is at zero potential with respect to earth. Table of Contents

Earth Station

Term used to describe a system for receiving signals.

Elevation

Up and down adjustments of your dish. Technically, the vertical angle that is measured form the horizon up to the satellite. This information helps you locate the satellite and point the dish toward it.

Fade Margin

Signals from geosynchronous satellites spread out and weaken in power on their journey to a receive site below. While this free space path loss can be easily calculated there are other more unpredictable losses. These include losses due to scattering and absorption by water in various forms, by oxygen molecules and by particulates in the atmosphere. Furthermore, atmospheric turbulence, antenna pointing errors, waveguide losses and ionospheric refraction measurably reduce downlinked signal power. Atmospheric absorption and antenna depointing losses may each typically be in the 0.2 to 0.3 dB range. When skies are clear, a satellite dish detects noise from the warm ground solely through its side lobes and very low temperature galactic noise via its main lobe. However, when rain falls and to a lesser extent when fog, snow and clouds are present, the main lobe "sees" a higher sky temperature than normal via its main lobe. This increase in detected noise temperature is typically about 1.2 dB. The decrease in signal power and increase in noise power lowers the C/N ratio. A receive system that operates near threshold under ideal conditions may fall below threshold during, for example, a rain or wind storm. Ku-band systems are particularly sensitive to rain fading. During a severe storm signal power could fall by as much as 10 dB. System designer must build a fade margin into a satellite reception system that depends upon local atmospheric conditions as well as availability, determined by the minimum percentage of down time. For example, in a very rainy climate to obtain a 99.99% availability at Ku-band a fade margin of 10 dB or more may be required.

Feeds

A feed has the important function of funneling signals reflected from a dish into the LNB. It is tuned to the frequency of the downlink signal and must have minimal losses while ignoring noise and other unwanted signals coming from off-axis directions. A poorly matched feed that does not properly illuminate a dish can add as much as 20°K of noise to a receiving system. Feeds must also select the required circular or linear polarity to properly detect a broadcast. Use of an inappropriate feed can result in poor cross-polarization discrimination, namely the reception of a signal with not only the desired polarity but also an unacceptable amount of the opposite polarity signal. Five general types of feeds have been developed for use in receiving satellite broadcasts: scalar, circular, dielectric, conical and pyramidal. Scalar, dielectric and conical feeds are the most commonly employed; the conical feed is employed with offset dishes. The scalar feed, the most common type in use today, consists of a section of circular waveguide with a set of concentric "scalar" rings. The circular waveguide is designed to detect both senses of linear polarity and the scalar rings to minimize signal reflections. Typically about 1.5% of the energy entering a scalar feed, about 0.08 dB, is lost due to reflections. A fixed ring scalar feed generally operates in the 0.33 to 0.45 f/D range. In some brands the position of the rings can be adjusted to extend this range from 0.28 to as high as 0.5 to match the f/D ratio of a dish. In general, the additional expense of an adjustable ring version is justifiable. An improvement of as much as 0.5 dB in carrier-to-noise ratio can be gained by matching a feed to a dish.

Feed Illumination

The term feedhorn was originally derived from uplink antenna jargon. An uplink feedhorn "fed" microwaves onto and "illuminated" a reflective surface below. The terms feedhorn and illumination have persisted even when describing downlink components. A feed thus "illuminates" a dish even though it actually receives reflected microwaves. The detected illumination pattern describes its field of view. A perfectly illuminated feed would collect radiation coming from nowhere but the targeted satellite signal reflected from the dish surface; it would reject microwaves from all other sources. In practice, prime-focus feeds illuminate antenna central regions most strongly and are progressively less able to detect radiation at increasingly greater off-axis angles. Similarly, feeds employed with an offset fed reflector are designed to be most capable of collecting energy from its center. The illumination pattern is an important design criteria. A feed that illuminated just the central portions of a dish would introduce little noise into the system but would miss some of the signal originating from the reflector edges and hence result in lowered system gain. However, a feed which over-illuminated a dish would take advantage of all the available gain but would introduce too much ground noise. Over- illuminating a dish could be a serious problem, especially when receiving signals from spacecraft close to horizontal elevations, because the ground on a typical cool summer day emits noise at a "hot" 290°K. A feed must be properly matched to the f/D ratio of the dish so that illumination is optimized. Using an inappropriate feed results in detection of less signal and more noise. It will also result in poor side lobe performance and thus increased susceptibility to terrestrial interference. Dish efficiency can be altered by simply changing feed illumination pattern. An over-illuminated dish would have a very high efficiency but the additional ground noise detected would result in a lower signal-to- noise ratio, the final determinant of system performance. In contrast, under-illuminating would result in substantially lower antenna efficiency as well as detected noise. The end result would still be the same, an undesired reduced signal-to-noise ratio.

Ferrite Polarizer

A ferrite polarizer is a solid-state device with no moving parts. The sense of linear polarity is selected by use of a magnetic field produced by a ferrite rod held in the center of a circular waveguide by a plastic dielectric support. The current passing through a large coil wound around the outside of the waveguide produces a magnetic field whose orientation depends upon the direction of the flow of charges. The polarity of the detected signal, in turn, depends upon the orientation of the magnetic field. Such polarizers have no moving parts and are thus not subject to the problems that affect their mechanical counterparts. As a result, these are preferable to mechanical devices for systems installed in very cold climates where probes can seize up due to condensation and freezing of water. Ferrite feeds typically have insertion losses of about 0.3 dB. Satellite receivers that operate with this type of polarizer often have some degree of built-in fine skew adjustment that allows the device to line up with the plane of signal polarity since the polarity plane can vary with satellite/receive site longitude differences and can be affected by atmospheric conditions like rain.

Flat Plate Antennas

Flat plate antennas have not yet been widely used in home satellite systems. There are two basic types: passive and active. The active flat plate is based on microcircuit design techniques. It is rarely seen in home satellite systems but is not uncommon in military and civilian radar systems were system cost is not a serious constraint. Passive flat plate antennas, like more common dishes, reflect or redirect satellite signals. A series of concentric rings overlaid onto a transparent sheet creates a lens that redirects or reflects and focuses signals. If these concentric rings are elongated into a set of ellipses, signals arriving from off- boresight locations can be focused to a point either in front of or behind the pattern.

Free Space Path Loss

Path loss, the loss a satellite incurs in traveling from an orbiting satellite to a receive location, is composed of free space path loss and other losses. The reduction in signal power due to the spreading of a spherical wave front as the wave radiates to the earth below is the free space path loss. The greater the distance to the target, the slant range, and the higher the frequency, the greater the path losses. Other losses include absorption by water and other atmospheric constituents. Ku-band signals sustain more loss that do C-band signals because attenuation by water vapor increases with frequency in this range. At Ku-band frequencies, rainfall can attenuate the signal by as much as 15 dB above that at clear sky conditions. When designing a satellite reception system, adequate fade margin must be incorporated to prevent severe signal fading during rainstorms.

F Connector

A special type of connector used commonly to terminate coaxial cable.

Favorite Channel Memory

IRD feature that allows the storage of favorite satellite TV and radio stations in memory as "favorite channels" for easy recall. Table of Contents

Feedhorn

A device that gathers microwave signals reflected from the surface of the dish and feeds them to the LNB.

Footprint

The geographic area toward which a satellite directs its signal.

Frequency

The property of an alternating-current signal measured in cycles per second or hertz.

FSS

Fixed Satellite Service.

G/T Factor

The G/T factor is the "figure of merit" of a dish/feed/LNB combination. It is calculated by taking the difference in decibels between dish gain and system noise temperature, a shorthand for G-10logT which is expressed in decibels. The "bottom line" G/T defines the combination of minimum dish diameter and LNB noise temperature required so that the C/N ratio at the satellite receiver input is just at threshold.

Gain Loss versus Reflector Irregularities

A perfect parabolic reflector would direct all incoming signals towards its focal point. However, dishes suffer from both systematic and random surface errors. Systematic errors result from large scale distortions such as twisting of the entire dish surface or flat regions on a mesh dish. Random errors are a direct result of the accuracy of the manufacturing process. As either type of surface errors increase, dish gain falls.

Gain

Increase in power. In satellite dishes, the gain is measured in dBW. A 3dB increase in gain equals a doubling in power. Table of Contents

Geostationary

Fixed orbit, approximately 22,300 miles above the earth's equator. Satellites parked in this orbit travel at the same speed as the rotation of the earth.

Geosynchronous

Term applied to satellites pared in orbit in the Clarke Belt (named for Arthur C. Clarke, father of satellite TV) 22,300 miles above the equator. Geostationary means same thing; often used interchangeably with geosynchronous.

Gigahertz (Ghz)

One billion cycles per second. Signals above one gigahertz are known as microwaves.

Ground Rod

Metal pole eight feet long driven into the ground to connect an electrical current to earth.

Ground Wire (or Conductor)

Wire connecting an electrical circuit to a ground rod.

Grounding Block

Device that connects two coaxial cables and can be grounded to earth to prevent electrical surges through the coaxial cables. Table of Contents

Half-Transponder Video

Some satellites have transponder with 54 MHz, 72 MHz or other bandwidths. These as well as standard 36 MHz wide channels can be used to transmit two television signals in a half-transponder format. The bandwidth is divided into two 27 or 36 MHz regions with the video carriers are centered in either the upper or lower region. To receive half-transponder formats, a receiver must be capable of both tuning to a continuously variable center frequency and employing bandwidth narrowing filters. For example, to receive 23 MHz half- transponder broadcasts, the tuner is centered on either the upper or lower half of the transponder frequency and then bandpass filters reduce the detected bandwidth from the normal 28 to 32 MHz to a more narrow 23 MHz. Adjustable bandpass filters can be interfaced to the IF loopthrough connections available on the rear panels of most satellite receivers. This loopthrough in many brands is connected via a short jumper cable when not in use. Narrowing the bandwidth improves the input C/N ratio with an expense in picture quality that ranges from hardly detectable to unacceptable. The trade-off is between a loss of color fidelity and picture detail for reduction in impulse noise, sparklies, and increased clarity. Receiver bandwidths as low as 12 MHz may be acceptable in some cases. At bandwidths below 10 MHz the audio subcarriers fall above the upper frequency cutoff of the high frequency bandpass filters. In this extreme case, a separate receiver would have to be used to recover the audio information. At bandwidths below 7 MHz color subcarriers are also truncated and only black/white video would be visible. The reduced frequency response in the receiver causes an attenuation of both the sync pulses and the high frequency portions of the video signal itself. Some picture tearing might be observed and as noise begins to overpower the signal sparklies again begin to appear.

Hertz (Hz)

Cycles per second.

Horizon-to-Horizon

Type of antenna mount that permits 180 degrees of antenna movement. Very strong and reliable, it is the most accurate mount to use for tracking Ku-band satellites.

IRD

Abbreviation for integrated receiver-decoder. New satellite receivers feature a built-in decoder (VideoCipher II Plus or VideoCipher RS) and dish motor drive controller. In older models, these were separate components.

Ku-Band

The microwave frequency band that ranges from 1 GHz to above 30 GHz includes the familiar Ku-band range of frequencies, 10.95 to 14.5 GHz.

LNB

A low noise block downconverter (LNB), detects the signal relayed from the feed, converts it to an electrical current, amplifies it and lowers its frequency. The downconverted signal is relayed via coax to an indoor satellite receiver. LNBs designed to receive C-band satellite signals that usually detect signals in the 3.7 to 4.2 GHz range can be used in most locations around the globe (although some transmissions from the C.I.S. Raduga and Gorizont satellites and Intelsat VI spacecraft are broadcast at frequencies below 3.7 GHz). These have outputs of 950 to 1450 MHz. However, Ku-band LNBs must be mated to the particular frequency range in use. For example, while all or a portion of the 10.950 to 11.700 GHz range is the standard input frequency in Europe, Africa and the Middle East, LNBs used in the Americas must manage signals of 11.700 to 12.200 GHz. While the differences are small, units designed for one area will not function adequately when used in regions having different downlink signal frequencies.

LNB Noise Temperature

LNBs are described either in terms of noise temperature (degrees K) or noise figure (dB), two interchangeable yardsticks. LNB noise figure is a measure of the degree by which an LNB degrades the signal-to- noise ratio of the satellite signal as it passes through the device. Since an LNB is the "front end" of a satellite reception system the noise it adds to the incoming signal sets the noise floor and plays a large part in determining picture quality. LNBs operating in the Ku-band range are now available at reasonable prices with noise figures in the 1.8 to 0.6 dB range, equal to temperatures ranging from 149 to 43°K. C-band LNBs are available in noise temperatures as low as 20°K. The improving noise performance of LNBs has brought benefits to many in difficult reception areas. For example, in regions where temperatures regularly soar to above 100°F during the day, LNBs perform well enough to overcome associated performance degradation. In weak footprint regions of the world, ultra-low noise LNBs combined with large dishes can greatly enhance reception of signals.

Latitude

The distance, measured in degrees, between the location of the surface of the earth and the equator.

LLA

- Low Level Audio which can be tuned in on your satellite receiver (if it has this ability).

LNA

Low-noise amplifier that boosts the satellite signal picked up by the earth-station dish. It is installed at a particular spot on the dish and is directly connected to the feedhorn.

Longitude

The distance, measured in degrees, between a position on a surface of the earth and the prime meridian.

Look Angle

Angle above the horizon at your location from which the satellite signal arrives.

Low Noise Block Downconverter (LNB)

A device that amplifies and downconverts the whole 500 Mhz satellite bandwidth at once to an intermediate frequency range. Table of Contents

Magnetic Deviation

Magnetic deviation is defined as the difference between the north compass heading and the actual heading to true north. The difference arises because the earth is not a homogenous sphere but has a time- and space- varying magnetic core and field structure. The earth acts like a giant magnet with its source of magnetism not concentrated at specific magnetic poles but throughout a large volume within the earth. The geographic north pole and the numerous magnetic north pole are located in different positions. It is a common misconception that a compass points towards magnetic north. This is not the case since a compass will point along the local magnetic field line. The magnetic variation at any point on the earth reflects this pointing variation.

Main Lobe

The central portion of a dish beam pattern, the main lobe, shows how narrow a region of space can be targeted. This is a very important factor considering that some satellites separated by 2° appear to be very closely spaced together from a receive site on earth. A dish detects most power via its main lobe. The beamwidth is defined as the width of this main lobe between "half power" points where detected signal power has dropped by 501r 3 dB. The smaller the beamwidth, the more narrow the field of view. It beamwidth is too great and satellites are spaced too closely together, more than one signal might be detected via the main lobe. Beamwidth decreases as both signal frequency and dish diameter increase. For example, a dish will have a third of the beamwidth at Ku-band than at C-band because the frequency is three time higher.

Mechanical Polarizer

A mechanical polarizer discriminates among linear or circular polarization formats by virtue of a physical motion. The original method to select between linearly polarized C-band signals was simply rotating the entire feed and low noise amplifier assembly. While this method is still occasionally used, more efficient techniques are employed today. Polarity is usually selected by rotating a small, lightweight metal probe that is housed in the circular waveguide in the throat of a feed between horizontal and vertical polarity orientations. A servo or dc motor accurately controls its position. Most satellite receivers available today have built-in controls for interfacing with one or both types of mechanical polarizers. Such devices are commonly employed in North America but are becoming rare in Europe where V/H switched or ferrite polarizers are more common. Mechanical devices suffer from the limitations of having moving parts that wear out and potentially seize in wet climates where freezing occurs.

Microwave Bands

Satellite broadcasts are transmitted within or just slightly below the microwave frequency band for a number of reasons. First, higher frequency signals have the potential for relaying larger quantities of information because, as the frequency increases, any given bandwidth becomes a smaller fraction of the carrier frequency. Second, signals transmitted at microwave frequencies can be aim into a highly directional beam towards an extremely small target in space. Third, microwave transmissions to satellites or between earth-based, line-of-sight relay stations are not as susceptible to noise from atmospheric disturbances as are lower frequency transmissions. Fourth, microwaves are able to pass through the upper atmosphere into outer space. Below frequencies of approximately 30 MHz, a radio wave will be reflected back from the ionosphere layer in the atmosphere towards earth. Fifth, the microwave region within the electromagnetic spectrum was a virgin territory during the late 1950s and 60s when frequency spectrum was being allocated by the International Telecommunications Union. Lower frequency space was already occupied by many different communication media and users. The microwave frequency band extends from just about 1 GHz to 30 GHz and above. The nomenclature used is listed here:

Band Name Frequency Range (GHz) L 1.53 - 2.70 S 2.50 - 2.70 C 3.40 - 6.425 X 7.25 - 8.40 Ku 10.95 - 14.50 Ka 17.7 - 21.2 K 27.5 - 31.0

Multi-Focus Dish

Multi-focus dishes, developed originally for use with C-band systems, allow more than one satellite to be simultaneously detected. This is done by reflecting incoming signals to a series of feedhorns. In contrast, single-focus reflectors must be repositioned by actuators in order to receive signals from just one satellite at a time.

Modified Polar Mount

Even perfectly aligned true polar mounts always have a small tracking error in scanning across the entire belt of satellites. This inaccuracy can be important when using large dishes with relatively narrow beamwidths, especially for Ku-band dishes that have one third the beamwidth of equal diameter C-band systems. If a satellite in the center of its sweep is accurately targeted, then those at the far ends will be slightly above the sight of the receiving antenna. If the end satellites are down the antenna boresight, the center one will be slightly below its main axis. This error can be controlled at less than 0.1 degrees with a well-adjusted, true polar mount. It is comparable with the 0.1 degrees "stationkeeping" motion of a satellite and is more than adequate for aligning C-band receive dishes. The aiming accuracy of a polar mount can be improved from 0.1 to less than 0.01 degrees even at end-of-arc satellites. The "modified" polar mount geometry is achieved by fine tuning the polar axis and declination offset angles. Once this is accomplished the pointing error achieved is less than the tolerances of the best available az-el mount mechanisms. Once the true polar angles have been correctly adjusted in a "true" polar mount, polar axis is then tilted slightly forward towards the arc of satellites. The declination offset angle is then reduced by an equal amount. A satellite due south from the receive site would be unaffected by this net zero change. The slight decrease in declination causes a dish to point higher than normally would be the case except when aimed directly south (or north). In effect, the most southerly satellite is targeted perfectly, while the antenna's main axis is aimed below the easterly or westerly spacecraft less than would normally occur with the conventional polar mount adjustments.

Mounts

A mount must accurately and securely aim a dish towards any chosen satellite. Even slight movements might mean the difference between receiving a signal and its being off target, especially with small beamwidth, large dishes operating a Ku-band frequencies. A deviation of as little as one degree might cause a second satellite to be swept into view in some areas of the world. Pointing accuracy is not necessarily as important an issue when detecting DBS broadcast satellites that are spaced 6 degrees apart in Europe and 8 degrees apart in North American. Antennas as small as 30 cm with 3 dB beamwidths of 5.8 degrees can be successfully used. There are two principal classes of antenna mounts: azimuth-elevation (az-el) and "true" or "modified" polar mounts. While both az-el or polar mounts can be fitted with actuators to permit rapid and easy targeting of any satellite in the arc, tracking mechanisms for polar mounts are usually the most simple and inexpensive. Remote controlled movement of either type of mount should be considered if multiple satellites or if satellites in unstable orbits are to be received.

Mast

Metal pipe attached to the mounting foot. Supports the LNB support arm and dish. In a pole mounting system, the metal pole is the mast.

Megahertz (Mhz)

Millions of cycles per second.

Modulation

The process in which a message is added to a carrier wave.

Modulator

A device that modulates a carrier. In a satellite receiver or VCR, the modulator places the audio and video signals on a carrier, usually channel 3 or 4, so they can be tuned by a standard TV set.

MTS Stereo

Broadcast standard by which local stations transmit stereo programs to TVs and VCRs equipped with MTS tuners. Some new IRDs feature MTS output, permitting stereo programs to be delivered on a single cable to MTS TVs and VCRs throughout the house. Table of Contents

Noise Figure

The noise figure of an amplifier is defined as the ratio of the S/N ratio at the its input to the S/N ratio at its output. In other words, the noise figure is a measure of the degree by which an LNB degrades the signal-to-noise ratio of the satellite signal as it passes through the device. Noise temperature, is also expressed in degrees Kelvin. This scale is based on the fact that at a temperature known as absolute zero, 0°K (equal to minus 273.16°C or minus 459.72°F), molecular motion ceases and consequently noise disappears. Table of Contents

Noise Temperature

The noise is any communication system is directly proportional to the ambient temperature of the device and the bandwidth of the signal being processed. In short, Noise equals kTB where k is a number known as Boltzman's constant.

Orthomode Transducers (OMTs) and Dual-Band LNBs

Orthomode transducers (OMTs) can simultaneously detect both vertically and horizontally polarized signals. Such devices are commonly found in commercial C-band installations such as satellite master antenna and cable television headends because they allow reception of all satellite transponders at one time. Another variety of feed designed to simultaneously detect both polarities, a dual LNB/feed, has no waveguide section but instead has two independent probes and two LNBs built into one housing. It is designed so each probe/LNB detects signals of only one polarity.

Polarization Offset

Some satellites do not have the plane of their electric fields perfectly aligned with the equatorial plane. As a result of this polarization offset, polarizers must be capable of having some fine adjustment, known as skew adjustment, in the plane of detected linear polarity to achieve maximal signal reception. In addition, even if the plane of linear polarization is perfectly aligned with the equatorial plane, as the difference between the site and satellite longitude increases, this apparent plane is twisted as viewed from the receive dish. Table of Contents

Polarizer

Satellites most often broadcast signals with either one or two senses of linear or circular polarities. The polarizer built into a feed must be capable of discriminating between these two different signals. There are three basic types of linear polarizers, mechanical, V/H switched and ferrite or electromechanical devices as well as circular polarizers.

Pre-Emphasis and De-Emphasis

FM video signals are pre-emphasized at the uplink site and de-emphasized within the satellite receiver. At the uplink, the video signal is passed through a network that attenuates only the lower frequencies effectively boosting the high frequency portion of the signal. At the receiver, a de-emphasis network attenuates the upper frequencies to restore the original video waveform. The objective of this technique is to improve the signal-to-noise ratio by about 2 dB. This method is effective because the noise in an FM satellite transmission increases from the 0 MHz to the upper limits of the baseband signal, about 6 MHz (a triangular noise distribution). Pre- and de-emphasis reduces noise by lowering the higher power, higher frequency noise. Pre- and de-emphasis circuits are simple RC networks with time constants usually of 50 or 75 microseconds. Pre-emphasis and de-emphasis are also applied to audio signals, also typically with 50 (North America) and 75 (Europe) microsecond time constants. European broadcasts are also in J17 audio format.

Prime-Focus Parabolic Dish

The most familiar dish is the prime-focus parabola which has a feed/LNB mounted at its focal point, typically secured by three or four supporting arms or a buttonhook assembly. A perfect dish would detect nothing but satellite signals. However, this goal is never achieved since its surface is never perfectly accurate and even a perfect dish would "see" signals coming from off-boresight directions. In addition, the feed and LNB that are located in front of the dish inevitably block some of the incoming signal.

Receiver Bandwidth

e the bandwidth in order to extend receiver threshold. While reducing bandwidth does reduce impulse noise and thus sparklies, it does so at the expense of picture fidelity. Whenever half-transponder formats are received, receiver bandwidth must be reduced and center frequency adjusted to accommodate just the portion of the transponder bandwidth in use.

SCPC - Single Carrier per Channel Audio

Audio signals are transmitted via satellite either in conjunction with the video or as separate signals in a variety of formats including audio subcarriers, single channel per carrier and digital sound-in-sync audio. Hundreds of single channel per carrier (SCPC) audio signals with individually assigned center frequencies can be transmitted over each satellite transponder. In contrast, a single 36 MHz wide transponder can manage at very most 10 to 15 audio subcarriers because these are relayed at the expense of the associated video power and bandwidth. Each SCPC carrier may occupy from as little as 5 kHz of bandwidth for voice-grade messages to as much as 250 kHz for high fidelity audio. Some satellite services occasionally relay the audio portion of their television broadcast is independently of the video in a SCPC format. In a few instances, this SCPC signal may not even be relayed on the same transponder. In these cases, a separate audio FM scanner is required for reception of both the video and audio signals

Signal Frequency

The term signal frequency usually refers to center frequency of a carrier although it can also refer to the entire transponder or channel bandwidth.

Satellites

Satellite that broadcast audio, data and video to vast regions of the earth below are high power, complex switching and frequency translation relay devices. Modern communication satellites receive signals, typically in the 1 to 40 GHz range, amplify and process these signals, and then downconvert their frequency for broadcast to a target area on the earth below. Each transponder processes signals with a given center frequency that spans a specified frequency band and has a predetermined EIRP. Today satellites that relay L-band, S-band, C-band, Ku-band and Ka-band signals are common. C-band video satellites typically have 24 transponders, or separate channels, on-board. The channel structure of Ku-band spacecraft is generally more variable. Today numerous spacecraft have transponders designed to handle more than one frequency band. Each satellite can be defined by a number of parameters including the number of channels, downlink power, antenna coverage and frequency transmitted.

Satellite Dish

Satellite dishes receive microwave signals from orbiting communication satellites. A dish used to receive satellite signals is generally a parabolic surface that reflects microwaves to a feed. The small metal probe within this feed is, in reality, the microwave antenna. A satellite dish collects and concentrates the very weak signals downlinked from a broadcast satellite while ignoring as much of any unwanted signals and noise as possible. Most dishes in use today are parabolically shaped, although multi-focus dishes are combinations of circular or parabolic shapes. Flat plate antennas are also used for receiving broadcast signals from satellites. Signals are reflected from the dish surface and concentrated to a "focal point" or to a series of focal points.

Satellite Receivers

The function of a satellite receiver is to select a channel for viewing or listening from the available block of information and then to process this signal into a form acceptable by a television, monitor or stereo. Receivers that either continuously tune across the range of frequencies or that have programmable tuning sections can accommodate any of the various frequency schemes relayed via C-band and Ku-band spacecraft. Most of these brands are completely frequency agile, namely they can be tuned continuously across the range in question. The quality of a satellite receiver is judged by the clarity and fidelity of the television picture and crispness of the sound it produces. These subjective criteria can be partially estimated from the receiver IF bandwidth and threshold. These, in turn, are all determined by the care taken in designing and manufacturing as well as by the choice of circuit components. The audio section of a receiver designed for agile use in international or domestic reception must be capable of continuous tuning through the 5.0 to 8.5 MHz subcarrier band. Audio subcarrier deviations can also range from narrow such as employed on Intelsat spacecraft to wide for some high fidelity audio and data relays so receivers should, at the very least, have a wide/narrow audio bandwidth selection. Furthermore, receivers must be able to manage the audio processing employed on the broadcasts desired such as Panda I stereo or multiplex, discrete or narrow deviation Wegener stereo. De-emphasis and low-pass filters may also vary since 50 microsecond, 75 microsecond or J17 emphasis is used on satellite transmissions in various parts of the world.

Side Lobes

Signals are also received via side lobes, an inherent property of the wave-like character of microwaves and the resulting "spreading" in the vision of a dish. Side lobes must be at least 16 to 20 dB lower than the main lobe. This means that a signal intercepted along the side lobes would be detected at 16 to 20 dB below the power that it would have been if it entered along the dish boresight. Side lobes "see" off-target signals that consist of unwanted noise and interference from adjacent satellites and other communicators. For C-band and Ku-band dishes up to roughly 5 meters and 3 meters, respectively, experience shows that a prime focus feed system results in better efficiency and lower side lobes at dramatically lower costs. However, for larger dishes a Cassegrain configuration has the advantage that the feed is in a much more accessible and serviceable location.

Slant Distance

The slant distance is the distance from the geosynchronous satellite to the receive site.

Splitter

Split signal out of receiver to Multiple TV sets

Subcarrier Audio

Audio signals are typically transmitted as subcarriers modulated onto the main video carrier, a form of frequency division multiplexing. For example, NTSC subcarriers are inserted in the 5.0 to 8.5 MHz range. PAL and SECAM subcarriers often have 6.60 and 7.20 MHz center frequencies but, as is the case with NTSC transmissions, other frequencies are frequently selected. These audio subcarriers may be used to transmit monophonic or stereo sound. In North America one of four systems is typically used to transmit stereo sound over satellite circuits: multiplex, Warner Amex, discrete and processed narrow deviation stereo. The Wegener Panda stereo system is commonly used on European satellites.

System Noise Temperature

System noise temperature reflects how much noise is added to a satellite signal by a reception system. Sources include noise detected by the dish and produced in the LNB, cable runs and remaining electronic circuitry. Satellite reception systems are sensitive to very weak noise sources including both galactic noise and that introduced by radiation from the warm earth. Galactic noise detected by a dish pointed directly into deep space is typically about 6°K. However, noise from the warm earth that is at an average temperature of 290°K is much higher. This noise is detected via dish side lobes and depends upon its elevation. As a dish is lowered towards the horizon it detects more ground noise. Since elevation to satellites at the center of the geosynchronous arc is higher than that of those at the easterly and westerly portions, system noise is lower when the most southerly satellites (or most northerly in the southern hemisphere) are targeted. The noise performance of an antenna can be improved in a number of ways. A higher quality dish of a given aperture has lower side lobes and is therefore less susceptible to noise. A larger diameter dish also has a better side lobe pattern and a more narrow main lobe so it generally contributes lower amounts of noise. Similarly, a deeper antenna having a lower f/D ratio, all else being constant, would detect lower amounts of ground noise. The noise introduced by the LNB is simply expressed by its noise temperature or figure. Therefore, for example, a 25°K LNB adds 25°K of noise. The noise contributed by the cables and satellite receiver is low by comparison because the LNB amplifies both the noise and signal detected by the antenna/feed. Its output signal is substantially higher in power than the noise added by cables, connectors and the satellite receiver. Therefore, the balance of system components has only a small effect, typically at most 5°K, on system noise temperature. G/T, the figure of merit for an earth station, can therefore be closely approximated by replacing T, system noise temperature, with the noise contribution of just the antenna and low noise amplifier. The signal at the output of the LNB is thus the key determinant of overall performance quality of satellite reception system.

Skew

Term used to describe the fine-tuning adjustment of the feedhorn polarity probe.

Threshold Extension

Subjective tests of picture quality have documented the degradation in picture quality seen near threshold. Therefore receiver manufacturers have been motivated to develop methods to "extend" or lower threshold and thus make a weaker signal more watchable. There are a number of approaches to extending receiver threshold. Using the best possible circuit design and components that contribute the lowest amounts of noise to a signal being processed is the starting point. Another simple method underlying most of these techniques is to reduce video bandwidth. The effect of reducing bandwidth is to increase C/N ratio resulting in some loss of picture fidelity. The increase in C/N ratio can be calculated from the link equation. For example, decreasing the bandwidth from 30 to 15 MHz results in a 3 dB increase in C/N ratio. The same result can be obtained by doubling the surface area of the receive dish. This technique can be valuable in out-of-footprint or weak signal areas. For example, reducing the bandwidth from 28 to 18 MHz, a manageable amount, increases the C/N ratio by 1.92 dB. This would be equivalent to replacing a 5 meter dish with an equivalent one that is 6.3 meters in diameter.

Transponder Bandwidth

Transponder bandwidth typically varies from 36 MHz to, in some cases, higher than 120 MHz. Such wider band transponders are often used for data transmissions but may also be subdivided into segments used to relay multiple video signals. Thus channel bandwidth is often less than transponder bandwidth. In such "half-transponder" video formats, the center frequency does not lie in the middle of the transponder band.

Teletext

An "electronic newspaper" transmitted via satellite that can be received with a teletext decoder such as the InfoCipher. Table of Contents

Transponder

A combination receiver, transmitter and antenna package on a satellite. The signal is received from the uplink station and downlinked back to Earth on a different frequency. Most C-band satellites have 24 transponders (12 vertical, 12 horizontal polarization); most Ku-band satellites have 16, although the Canadian Anik birds have 32. Some satellites have a mix of C-band and Ku-band transponders.

Tuner

The portion of a receiver that selects a desired signal from a group of signals in a frequency band.

TVRO

Trade name often used for satellite receiving system, shorthand for television receive-only. Home dish owners receive signals while programmers send or uplink signals

Uplink

Antenna facility that transmits signals to a satellite.

V/H Switched Polarizer

Solid state selection is electronic switching between two probes that are mounted within circular waveguide. One probe detects horizontally and the other vertically polarized signals. A V/H switched polarizer is not as popular as other selection methods in situations where numerous satellites over the full extent of the geosynchronous arc will be detected. In that case fine fine tuning of polarity, skew control, is not possible since only two fixed directions of polarity, based on the orientation of two probes, can be selected. Such "solid state probe selection polarizers" also tend to somewhat more noisy than mechanical or ferrite methods. Switching between the two probes, vertical and horizontal, is effected by changing the supply voltage on the center conductor of the cable feeding the LNB. A pin diode may be switched by an LNB voltage of, for example, 13 volts for one direction of polarity and 17 volts for the other. Table of Contents

Video Carrier-to-Noise (C/N) Ratio

The video carrier-to-noise ratio is a measure of the ratio of carrier to noise power expressed in decibels. C/N ratio is determined from link analysis calculations. It depends directly upon satellite EIRP, dish gain, dish noise temperature, LNB noise temperature, signal bandwidth and path loss.

Video Noise Bandwidth Factor

The video noise bandwidth factor is a reflection of the bandwidth of the video filter within a satellite receiver. It is normally set equal to the same value as the baseband video frequency. 4.2 MHz and 5.5 MHz are used for NTSC and PAL formatted broadcasts. If the maximum baseband video filter is set at a value greater than the baseband video frequency, the S/N ratio would be reduced since additional noise would enter the system. If this factor is much below the baseband video frequency, the video signal is low-pass filtered resulting in poor resolution, streaking and smearing of colors, delays in the color signal and other related problems.

Video Signal-to-Noise (S/N) Ratio

In any communication system the ratio of the signal to noise power, the S/N ratio, available to drive the audio or video device is the central factor in determining whether a communication signal is usable. Even when the noise power is quite high, if the signal power is sufficient the S/N ratio and thus picture quality can be acceptable. Subjective experiments have shown that television picture quality is directly related to the S/N ratio. For example, in 1959, the FCC in the United States, authorized a task group, known as the Television Allocations Study Organization or TASO, to investigate the problems associated with television broadcasting and reception. When a standard television set was viewed by people who were then asked to rate picture quality results indicated that for an acceptable picture a S/N ratio of at least 35 dB was necessary. Other studies have confirmed these findings.

Video Compression

A new, soon to be used technology that permits the squeezing of multiple channels into the bandwidth of one satellite transponder. Table of Contents

Video Monitor

A television set that accepts direct video signals. Not all TV sets are also monitors, which are best suited to deliver the most optimal video and audio performance.

Video Signal

That portion of the transmitted signal containing the picture information.

Videocipher

An encryption (scrambling) and de-cryption system technology developed in the U.S. in the mid 1980's for signals broadcast via satellite. Adopted by U.S. premium cable services (ie. HBO, ESPN, etc.) to control distribution of their signal to cable operators and direct-to-home satellite dish owners.

Videocipher II+

Most recent updated VIDEOCIPHER technology with improved security necessitated by "PIRACY". Includes "RS - Renewable Security" access port for future software updates.

VSWR (Voltage Standing Wave Ratio)

A measure of the efficiency of a signal interface, especially the impedance match of the antenna to the LNA

1.Azimuth: The angle of horizontal rotation that a dish must be rotated to point at a specific satellite, 0 degree is North, 90 degree is East and 180 degrees is South.

2.Compass headings: The adjusted azimuth reading with the magnetic variation of the earth.

3.Elevation: The upward tilt of the dish measured in degrees required to aim the dish at a specific satellite.

4.Dish: Commonly used term for a satellite antenna.

5.Feedhorn: The focal point assembly on a dish that collects the signal and changes the polarity, and sends it to the LNB.

6.Ku Band: Microwave broadcast at 11.7-12.2 GHz. For reference, DSS satellites are broadcasted at 12.2-12.7 Ghz range.

7.L.O.: Local Oscillation Frequency. this is 10750Mhz for Normal Ku band LNBF, to convert from I.F. freq. to Downlink frequency, add 10750 MHz. For example, CTN on G4 is 1090 I.F., its downlink is 1090+10750=11840.

8.Wide Band: Band wider than normal Ku 11.7-12.2, say 10.95-11.7 GHz, for example,the Deutsche Welle is broadcasting at 12.605 Downlink frequency, you need a Wide-Band LNB to receive DW on Intelsat K. 9.Uplink: Signal transmission from ground station to satellite. 10.Downlink: Signal transmission from satellite to your dish and LNB.

11.LNB: Stands for Low Noise Block Downconverter. A device that pre-amplifies and converts a direct satellite signal that can be utilized by satellite receiver.

12.LNBF: Combining LNB and Feedhorn in one casing for best efficiency and minimum loss. Electronically switchable between horizontal and vertical polarities by voltages provided by the satellite receiver. Waterproof.

13.Look Angle: The angle at which an antenna must be aimed in order to see a particular satellite.

14.Satellite Receiver: A receiver that processes satellite signals and allows you to tune in different video and audio channels. It cannot descramble the scrambled channels.

15.I.F. BW: I.F. tuning for best picture quality. Some receivers have this button to narrow the video bandwidth.

16.Audio BW Audio tuning for best audio quality. Some receivers have this button to narrow the audio bandwidth to get rid of annoying noise.

17.Prime-focus Dish: The focus of the dish is at dish center, round dish.

18.Offset Dish: A newly designed dish for accumulating less snow and better efficiency. When looking at the same satellite, the offset dish is about 25 degree less tilted than the prime-focus dish(prime focus dish looking more up to the sky).

LNBF - The Low Noise Blockdown Feedhorn amplifies the signal collected on the parabolic antenna(dish). It works on 13V of power which is supplied by the satellite receiver. A single LNBF will feed one receiver, and a dual LNBF will feed two or more receivers.

LNB - The Low Noise Blockdown amplifier performs the same functions as the LNBF.

DTH Broadcast Satellite - Direct-to-Home Broadcast Satellite. DirecTV and USSB's satellites are manufactured by Hughes. Echostars' satellite are manufactured by Lockheed Martin. These satellites are in a geostationary orbit about 22,800 miles above the earth in various orbital slots within the Clarke Belt.

DBS - Direct Broadcast Satellite

DSS - Specific reference to the DBS system offered by DIRECTV/USSB

DST - Digital Satellite Television

DVB - Digital Video Broadcast - system offered by Echostar

MPEG-1 - Specific data transmission protocol (format) developed by the Moving Pictures Experts Group (MPEG). MPEG-1 protocol is not as advanced as MPEG-2 protocol

MPEG-2 - Latest specific data transmission protocol (format) developed by the Moving Pictures Experts Group (MPEG). It is a more advanced protocol than MPEG-1 due primarily its all-digital transmission of data at between 4 and 9 megabits/second (Mbit/sec). Several other enhancements over MPEG-1 are also realized. MPEG formating is the specific formating in which data is transmitted to satellites, transmitted back to earth, and interpreted by set-top units.

Satellite - Equipment in orbit that can transmit signals between (station and distributor) or (distributor and homeowner); the signals can be analog or digital; each satellite usually has the capacity to transmit a number of different signals simultaneously

Satellite Dish - Receives the transmissions being sent from satellites; Distributors have dishes to receive the transmissions from the broadcast stations; Howeowners have dishes to receive transmissions that have been retransmitted by the distributors

Set-Top Unit - Device that converts the digital signal received by the dish to whatever signals are required by the TV set; the name set-top implies that the device sits atop the television

A...

Amplitude Modulation (AM) The baseband signal is caused to vary the amplitude or height of the carrier wave to create the desired information content.

Amplifier A device used to boost the strength of an electronic signal.

Analog A form of transmitting information characterized by continuously variable quantities, as opposed to digital transmission, which is characterized by discrete bits of information in numerical steps. An analog signal is responsive to changes in light, sound, heat and pressure.

Analog-to-Digital Conversion (ADC) Process of converting analog signals to a digital representation. DAC represents the reverse translation.

ANIK The Canadian domestic satellite system that transmits Canadian Broadcasting Corporation's (CSC) network feeds throughout the country. This system also carries long distance voice and data services throughout Canada as well as some transborder service to the U.S. and Mexico.

Antenna A device for transmitting and receiving radio waves. Depending on their use and operating frequency, antennas can take the form of a single piece of wire, a di-pole a grid such as a yagi array, a horn, a helix, a sophisticated parabolic-shaped dish, or a phase array of active electronic elements of virtually any flat or convoluted surface.

Aperture A cross sectional area of the antenna which is exposed to the satellite signal.

Apogee The point in an elliptical satellite orbit which is farthest from the surface of the earth. Geosynchronous satellites which maintain circular orbits around the earth are first launched into highly elliptical orbits with apogees of 22,237 miles. When the communication satellite reaches the appropriate apogee, a rocket motor is fired to place the satellite into its permanent circular orbit of 22,237 miles.

Apogee Kick Motor (AKM) Rocket motor fired to circulate orbit and deploy satellite into geostationary orbit.

Attenuation The loss in power of electromagnetic signals between transmission and reception points.

Attitude Control The orientation of the satellite in relationship to the earth and the sun.

Audio Subcarrier The carrier between 5 MHz and 8 MHz containing audio (or voice) information inside of a video carrier.

Automatic Frequency Control (AFC) A circuit which automatically controls the frequency of a signal.

Automatic Gain Control (AGC) A circuit which automatically controls the gain of an amplifier so that the output signal level is virtually constant for varying input signal levels.

AZ/EL Mount Antenna mount that requires two separate adjustments to move from one satellite to another;

Azimuth The angle of rotation (horizontal) that a ground based parabolic antenna must be rotated through to point to a specific satellite in a geosynchronous orbit. The azimuth angle for any particular satellite can be determined for any point on the surface of the earth giver the latitude and longitude of that point. It is defined with respect to due north as a matter of easy convenience.

B...

B-Mac A method of transmitting and scrambling television signals. In such transmissions MAC (Multiplexed Analog Component) signals are time-multiplexed with a digital burst containing digitized sound, video synchronizing, authorization, and information.

Backhaul A terrestrial communications channel linking an earth station to a local switching network or population center.

Backoff The process of reducing the input and output power levels of a traveling wave tube to obtain more linear operation.

Band Pass Filter An active or passive circuit which allows signals within the desired frequency band to pass through but impedes signals outside this pass band from getting through.

Bandwidth A measure of spectrum (frequency) use or capacity. For instance, a voice transmission by telephone requires a bandwidth of about 3000 cycles per second (3KHz). A TV channel occupies a bandwidth of 6 million cycles per second (6 MHz) in terrestrial Systems. In satellite based systems a larger bandwidth of 17.5 to 72 MHz is used to spread or "dither" the television signal in order to prevent interference.

Baseband The basic direct output signal in an intermediate frequency based obtained directly from a television camera, satellite television receiver, or video tape recorder. Baseband signals can be viewed only on studio monitors. To display the baseband signal on a conventional television set a "modulator" is required to convert the baseband signal to one of the VHF or UHF television channels which the television set can be tuned to receive.

Baud The rate of data transmission based on the number of signal elements or symbols transmitted per second. Today most digital signals are characterized in bits per second.

Beacon Low-power carrier transmitted by a satellite which supplies the controlling engineers on the ground with a means of monitoring telemetry data, tracking the satellite, or conducting propagation experiments. This tracking beacon is usually a horn or omni antenna.

Beamwidth The angle or conical shape of the beam the antenna projects. Large antennas have narrower beamwidths and can pinpoint satellites in space or dense traffic areas on the earth more precisely. Tighter beamwidths thus deliver higher levels of power and thus greater communications performance.

Bird Slang for a communications satellite located in geosynchronous orbit.

Bit A single digital unit of information

Bit Error Rate The fraction of a sequence of message bits that are in error. A bit error rate of 10-6 means that there is an average of one error per million bits.

Bit Rate The speed of a digital transmission, measured in bits per second.

Blanking An ordinary television signal consists of 30 separate still pictures or frames sent every second. They occur so rapidly, the human eye blurs them together to form an illusion of moving pictures. This is the basis for television and motion picture systems. The blanking interval is that portion of the television signal which occurs after one picture frame is sent and before the next one is transmitted. During this period of time special data signals can be sent which will not be picked up on an ordinary television receiver.

Block Down Converter A device used to convert the 3.7 to 4.2 KHz signal down to UHF or lower frequencies (1 GHz and lower).

Business Television Corporate communications tool involving video transmissions of information via satellite. Common uses of business television are for meetings, product introductions and training.

C...

C Band This is the band between 4 and 8 GHz with the 6 and 4 GHz band being used for satellite communications. Specifically, the 3.7 to 4.2 GHz satellite communication band is used as the down link frequencies in tandem with the 5.925 to 6,425 GHz band that serves as the uplink.

Carrier to Noise Ratio (C/N) The ratio of the received carrier power and the noise power in a given bandwidth, expressed in dB. This figure is directly related to G/T and S/N; and in a video signal the higher the C/N, the better the received picture.

Carrier The basic radio, television, or telephony center of frequency transmit signal. The carrier in an analog signal. is modulated by manipulating its amplitude (making it louder or softer) or its frequency (shifting it up or down) in relation to the incoming signal. Satellite carriers operating in the analog mode are usually frequency modulated.

Carrier Frequency The main frequency on which a voice, data, or video signal is sent. Microwave and satellite communications transmitters operate in the band from 1 to 14 GHz (a GHz is one billion cycles per second).

Cassegrain Antenna The antenna principle that utilizes a subreflector at the focal point which reflects energy to or from a feed located at the apex of the main reflector.

CDMA Code division multiple access. Refers to a multiple-access scheme where stations use spread-spectrum modulations and orthogonal codes to avoid interfering with one another.

Channel A frequency band in which a specific broadcast signal is transmitted. Channel frequencies are specified in the United States by the Federal Communications Commission. Television signals require a 6 MHz frequency band to carry all the necessary picture detail.

Circular Polarization Unlike many domestic satellites which utilize vertical or horizontal polarization, the international Intelsat satellites transmit their signals in a rotating corkscrew-like pattern as they are down-linked to earth. On some satellites, both right-hand rotating and left-hand rotating signals can be transmitted simultaneously on the same frequency; thereby doubling the capacity of the satellite to carry communications channels.

Clamp A video processing circuit that removes the energy dispersal signal component from the video waveform.

Clarke Orbit That circular orbit in space 22,237 miles from the surface of the earth at which geosynchronous satellites are placed. This orbit was first postulated by the science fiction writer Arthur C. Clarke in Wireless World magazine in 1945. Satellites placed in these orbits, although traveling around the earth at thousands of miles an hour, appear to be stationary when viewed from a point on the earth, since the earth is rotating upon its axis at the same angular rate that the satellite is traveling around the earth.

C/No Carrier-to-noise ratio measured either at the Radio Frequency (RF) or Intermediate Frequency (IF)

Codec Coder/decoder system for digital transmission.

Co-Location Ability of multiple satellites to share the same approximate geostationary orbital assignment frequently due to the fact that different frequency bands are used.

Color Subcarrler A subcarrier that is added to the main video signal to convey the color information. In NTSC systems, the color subcarrier is centered on a frequency of 3.579545 MHz, referenced to the main video carrier.

Common Carrier Any organization which operates communications circuits used by other people. Common carriers include the telephone companies as well as the owners of the communications satellites, RCA, Comsat, Direct Net Telecommunications, AT&T and others. Common carriers are required to file fixed tariffs for specific services.

Companding A noise-reduction technique that applies single compression at the transmitter and complementary expansion at the receiver.

Composite Baseband The unclamped and unfiltered output of the satellite receiver's demodulator circuit, containg the video information as well as all transmitted subcarriers.

Conus Contiguous United States. In short, all the states in the U.S. except Hawaii and Alaska.

Cross Modulation A form of signal distortion in which modulation from one or more RF carrier(s) is imposed on another carrier.

C/T Carrier-to-noise-temperature ratio.

D...

DAMA Demand-Assigned Multiple Access - A highly efficient means of instantaneously assigning telephony channels in a transponder according to immediate traffic demands.

DBS Direct broadcast satellite. Refers to service that uses satellites to broadcast multiple channels of television programming directly to home mounted small-dish antennas.

dBi The dB power relative to an isotropic source.

dBW The ratio of the power to one Watt expressed in decibels.

Decibel (dB) The standard unit used to express the ratio of two power levels. It is used in communications to express either a gain or loss in power between the input and output devices.

Declination The offset angle of an antenna from the axis of its polar mount as measured in the meridian plane between the equatorial plane and the antenna main beam.

Decoder A television set-top device which enables the home subscriber to convert an electronically scrambled television picture into a viewable signal. This should not be confused with a digital coder/decoder known as a CODEC which is used in conjunction with digital transmissions.

Deemphasis Reinstatement of a uniform baseband frequency response following demodulation.

Delay The time it takes for a signal to go from the sending station through the satellite to the receiving station. This transmission delay for a single hop satellite connection is very close on one-quarter of a second.

Demodulator A satellite receiver circuit which extracts or "demodulates" the "wanted "signals from the received carrier.

Deviation The modulation level of an FM signal determined by the amount of frequency shift from the frequency of the main carrier.

Digital Conversion of information into bits of data for transmission through wire, fiber optic cable, satellite, or over air techniques. Method allows simultaneous transmission of voice, data or video.

Digital Speech Interpolation DSI - A means of transmitting telephony. Two and One half to three times more efficiently based on the principle that people are talking only about 40% of the time.

Dual Spin Spacecraft design whereby the main body of the satellite is spun to provide altitude stabilization, and the antenna assembly is despun by means of a motor and bearing system in order to continually direct the antenna earthward. This dual-spin configuration thus serves to create a spin stabilized satellite.

E...

Earth Station The term used to describe the combination or antenna, low-noise amplifier (LNA), down-converter, and receiver electronics. used to receive a signal transmitted by a satellite. Earth Station antennas vary in size from the.2 foot to 12 foot (65 centimeters to 3.7 meters) diameter size used for TV reception to as large as 100 feet (30 meters) in diameter sometimes used for international communications. The typical antenna used for INTELSAT communication is today 13 to 18 meters or 40 to 60 feet.

Echo Canceller An electronic circuit which attenuates or eliminates the echo effect on satellite telephony links. Echo cancellers are largely replacing obsolete echo suppressors.

Echo Effect A time-delayed electronic reflection of a speaker's voice. This is largely eliminated by modern digital echo cancellers.

Edge of Coverage Limit of a satellite's defined service area. In many cases, the EOC is defined as being 3 dB down from the signal level at beam center. However, reception may still be possible beyond the -3dB point.

EIRP Effective Isotropic Radiated Power - This term describes the strength of the signal leaving the satellite antenna or the transmitting earth station antenna, and is used in determining the C/N and S/N. The transmit power value in units of dBW is expressed by the product of the transponder output power and the gain of the satellite transmit antenna.

Elevation The upward tilt to a satellite antenna measured in degrees required to aim the antenna at the communications satellite. When. aimed at the horizon, the elevation angle is zero. If it were tilted to a point directly overhead, the satellite antenna would have an elevation of 90 degrees.

Encoder A device used to electronically alter a signal so that it can only be viewed on a receiver equipped with a special decoder.

EOL End of Life of a satellite.

Equatorial Orbit An orbit with a plane parallel to the earth's equator.

ESC Engineering Service Circuit - The 300-3,400 Hertz voice plus teletype (S+DX) channel used for earth station-to-earth station and earth station-to-operations center communications for the purpose of system maintenance, coordination and general system information dissemination. In analog (FDM/FM) systems there are two S+DX channels available for this purpose in the 4,000-12,000 Hertz portion of the baseband. In digital systems there are one or two channels available which are usually convened to a 32 or 64 Kbps digital signal and combined with the earth station traffic digital bit stream. Modern ESC equipment interfaces with any mix of analog and digital satellite carriers, as well as backhaul terrestrial links to the local switching center.

F...

F/D Ratio of antenna focal length to antenna diameter. A higher ratio means a shallower dish.

FDMA Frequency division multiple access. Refers to the use of multiple carriers within the same transponder where each uplink has been assigned frequency slot and bandwidth. This is usually employed in conjunction with Frequency Modulation.

Feed This term has at least two key meanings within the field of satellite communications. It is used to describe the transmission of video programming from a distribution center. It is also used to describe the feed system of an antenna. The feed system may consist of a subreflector plus a feedhorn or a feedhorn only.

Feedhorn A satellite TV receiving antenna component that collects the signal reflected from the main surface reflector and channels this signal into the low-noise amplifier (LNA)

FM Frequency Modulation - A modulation method whereby the baseband signal varies the frequency of the carrier wave.

FM Threshold That point at which the input signal power is just strong enough to enable the receiver demodulator circuitry successfully to detect and recover a good quality television picture from the incoming video carrier. Using threshold extension techniques, a typical satellite TV receiver will successfully provide good pictures with an incoming carrier noise ratio of 7db. Below the threshold a type of random noise called "sparkles" begins to appear in the video picture. In a digital transmission, however, signal is sudden and dramatically lost when performance drops under the threshold.

Focal Length Distance from the center feed to the center of the dish.

Focal Point The area toward which the primary reflector directs and concentrates the signal received.

Footprint A map of the signal strength showing the EIRP contours of equal signal strengths as they cover the earth's surface. Different satellite transponders on the same satellite will often have different footprints of the signal strength. The accuracy of EIRP footprints or contour data can improve with the operational age of the satellite. The actual EIRP levels of the satellite, however, tends to decrease slowly as the spacecraft ages.

Forward Error Correction (FEC) Adds unique codes to the digital signal at the source so errors can be detected and corrected at the receiver.

Frequency The number of times that an alternating current goes through its complete cycle in one second of time. One cycle per second is also referred to as one hertz; 1000 cycles per second, one kilohertz; 1,000,000 cycles per second, one megahertz: and 1,000,000,000 cycles per second, one gigahertz.

Frequency Coordination A process to eliminate frequency interference between different satellite systems or between terrestrial microwave systems and satellites. In the U.S. this activity relies upon a computerized service utilizing an extensive database to analyze potential microwave interference problems that arise between organizations using the same microwave band. As the same C-band frequency spectrum is used by telephone networks and CATV companies when they are contemplating the installation of an earth station, they will often obtain a frequency coordination study to determine if any problems will exist.

G...

Gain A measure of amplification expressed in dB.

Geostationary Refers to a geosynchronous satellite angle with zero inclination. so the satellite appears to hover over one spot on the earth's equator.

Geosynchronous The Clarke circular orbit above the equator. For a planet the size and mass of the earth, this point is 22,237 miles above the surface.

Gigahertz (GHz) One billion cycles per second. Signals operating above 3 Gigahertz are known as microwaves. above 30 GHz they are know as millimeter waves. As one moves above the millimeter waves signals begin to take on the characteristics of Iightwaves.

Global Beam An antenna down-link pattern used by the Intelsat satellites, which effectively covers one-third of the globe. Global beams are aimed at the center of the Atlantic, Pacific and Indian Oceans by the respective Intelsat satellites, enabling all nations on each side of the ocean to receive the signal. Because they transmit to such a wide area, global beam transponders have significantly lower EIRP outputs at the surface of the Earth as compared to a US domestic satellite system which covers just the continental United States. Therefore, earth stations receiving global beam signals need antennas much larger in size (typically 10 meters and above (i.e.30 feet and up).

Gregorian Dual-reflector antenna system employing a paraboloidal main reflector and a concave ellipsoidal subreflector.

G/T A figure of merit of an antenna and low noise amplifier combination expressed in dB. "G" is the net gain of the system and "T" is the noise temperature of the system. The higher the number, the better the system.

Guard Channel Television channels are separated in the frequency spectrum by spacing them several megahertz apart. This unused space serves to prevent the adjacent television channels from interfering with each other.

H...

Half Transponder A method of transmitting two TV signals through a single transponder through the reduction of each TV signal's deviation and power level. Half-transponder TV carriers each operate typically 4 dB to 7 dB below single-carrier saturation power.

Headend Electronic control center - generally located at the antenna site of a CATV system - usually including antennas, preamplifiers, frequency converters, demodulators and other related equipment which amplify, filter and convert incoming broadcast TV signals to cable system channels.

Hertz (Hz) The name given to the basic measure of radio frequency characteristics. An electromagnetic wave completes a full oscillation from its positive to its negative pole and back again in what is known as a cycle. A single Hertz is thus equal to one cycle per second.

Hub The master station through which all communications to, from and between micro terminals must flow. in the future satellites with on-board processing will allow hubs to be eliminated as MESH networks are able to connect all points in a network together.

I...

IBS INTELSAT Business Services.

Inclination The angle between the orbital plane of a satellite and the equatorial plane of the earth.

INMARSAT The International Maritime Satellite Organization operates a network of satellites for international transmissions for all types of international mobile services including maritime, aeronautical, and land mobile.

INTELSAT The International Telecommunications Satellite Organization operates a network of satellites for international transmissions.

Interference Energy which tends to interfere with the reception of the desired signals, such as fading from airline flights, RF interference from adjacent channels, or ghosting from reflecting objects such as mountains and buildings.

ISDN - Integrated Services Digital Network. A CCITT standard for integrated transmission of voice, video and data. Bandwidths include: Basic Rate Interface - BR (144 Kbps - 2 B & 1 D channel) and Primary Rate - PRI (1.544 and 2.048 Mbps).

Isotropic Antenna A hypothetical omnidirectional point-source antenna that serves as an engineering reference for the measurement of antenna gain.

ITU International Telecommunication Union.

J...

JPEG ISO Joint Picture Expert Group standard for the compression of still pictures.

K...

Ka Band The frequency range from 18 to 31 GHz.

Kbps Kilobits per second. Refers to transmission speed of 1,000 bits per second.

Kelvin (K) The temperature measurement scale used in the scientific community. Zero K represents absolute zero, and corresponds to minus 459 degrees Fahrenheit or minus 273 Celsius. Thermal noise characteristics of LNA are measured in Kelvins.

Kilohertz (kHz) Refers to a unit of frequency equal to 1,000 Hertz.

Klystron A type of high-power amplifier which uses a special beam tube.

Ku Band The frequency range from 10.9 to 17 GHz.

L...

L-Band The frequency range from 0.5 to 1.5 GHz. Also used to refer to the 950 to 1450MHz used for mobile communications.

Leased Line A dedicated circuit typically supplied by the telephone company.

Low Noise Amplifier (LNA) This is the preamplifier between the antenna and the earth station receiver. For maximum effectiveness, it must be located as near the antenna as possible, and is usually attached directly to the antenna receive port. The LNA is especially designed to contribute the least amount of thermal noise to the received signal.

Low Noise Block Downconverter (LNB) A combination Low Noise Amplifier and downconverter built into one device attached to the feed.

M...

MAC (A, B, C, D2) Multiplexed analog component color video transmission system. Subtypes refer to the various methods used to transmit audio and data signals.

Margin The amount of signal in dB by which the satellite system exceeds the minimum levels required for operation.

Master Antenna Television (MATV) An antenna system that serves a concentration of television sets such as in apartment buildings, hotels or motels.

Megahertz (MHz) Refers to a frequency equal to one million Hertz, or cycles per second.

Microwave Line-of sight, point-to-point transmission of signals at high frequency. Many CATV systems receive some television signals from a distant antenna location with the antenna and the system connected by microwave relay. Microwaves are also used for data, voice, and indeed all types of information transmission. The growth of fiber optic networks have tended to curtail the growth and use of microwave relays.

Microwave Interference Interference which occurs when an earth station aimed at a distant satellite picks up a second, often stronger signal, from a local telephone terrestrial microwave relay transmitter. Microwave interference can also be produced by nearby radar transmitters as well as the sun itself. Relocating the antenna by only several feet will often completely eliminate the microwave interference.

Modulation The process of manipulating the frequency or amplitude of a carrier in relation to an incoming video, voice or data signal.

Modulator A device which modulates a carrier. Modulators are found as components in broadcasting transmitters and in satellite transponders. Modulators are also used by CATV companies to place a baseband video television signal onto a desired VHF or UHF channel. Home video tape recorders also have built-in modulators which enable the recorded video information to be played back using a television receiver tuned to VHF channel 3 or 4.

Multiplexing Techniques that allow a number of simultaneous transmissions over a single circuit.

N...

Noise Any unwanted and unmodulated energy that is always present to some extent within any signal.

Noise Figure (NF) A term which is a figure of merit of a device, such as an LNA or receiver, expressed in dB, which compares the device with a perfect device.

NTSC - National Television Standards Committee A video standard established by the United States (RCA/NBC} and adopted by numerous other countries. This is a 525-line video with 3.58-MHz chroma subcarrier and 60 cycles per second.

O...

Orbital Period The time that it takes a satellite to complete one circumnavigation of its orbit.

P...

Packet Switching Data transmission method that divides messages into standard-sized packets for greater efficiency of routing and transport through a network.

PAL - Phase Alternation System The German developed TV standard based upon 50 cycles.per second and 625 lines.

Parabolic Antenna The most frequently found satellite TV antenna, it takes its name from the shape of the dish described mathematically as a parabola. The function of the parabolic shape is to focus the weak microwave signal hitting the surface of the dish into a single focal point in front of the dish. It is at this point that the feedhorn is usually located.

Phase-Locked Loop (PLL) A type of electronic circuit used to demodulate satellite signals.

Polarization A technique used by the satellite designer to increase the capacity of the satellite transmission channels by reusing the satellite transponder frequencies. In linear cross polarization schemes, half of the transponders beam their signals to earth in a vertically polarized mode; the other half horizontally polarize their down links. Although the two sets of frequencies overlap, they are 90 degree out of phase, and will not interfere with each other. To successfully receive and decode these signals on earth, the earth station must be outfitted with a properly polarized feedhorn to select the vertically or horizontally polarized signals as desired.

In some installations, the feedhorn has the capability of receiving the vertical and horizontal transponder signals simultaneously, and routing them into separate LNAs for delivery to two or more satellite television receivers. Unlike most domestic satellites, the Intelsat series use a technique known as left-hand and right-hand circular polarization.

Polarization Rotator A device that can be manually or automatically adjusted to select one of two orthogonal polarizations.

Polar Mount Antenna mechanism permitting steering in both elevation and azimuth through rotation about a single axis. While an astronomer's polar mount has its axis parallel to that of the earth, satellite earth stations utilize a modified polar mount geometry that incorporates a declination offset.

Polar Orbit An orbit with its plane aligned in parallel with the polar axis of the earth

PTT - Post Telephone and Telegraph Administration Refers to operating agencies directly or indirectly controlled by governments in charge of telecommunications services in most countries of the world.

Pulse Code Modulation A time division modulation technique in which analog signals are sampled and quantized at periodic intervals into digital signals. The values observed are typically represented by a coded arrangement of 8 bits of which one may be for parity.

Q...

QPSK - Quadrature Phase Shift Keying System of modulating a satellite signal.

R...

Rain Outage Loss of signal at Ku or Ka Band frequencies due to absorption and increased sky-noise temperature caused by heavy rainfall.

Receiver (Rx) An electronic device which enables a particular satellite signal to be separated from all others being received by an earth station, and converts the signal format into a format for video, voice or data.

Receiver Sensitivity Expressed in dBm this tells how much power the detector must receive to achieve a specific baseband performance, such as a specified bit error rate or signal to noise ratio.

S...

Satellite A sophisticated electronic communications relay station orbiting 22,237 miles above the equator moving in a fixed orbit at the same speed and direction of the earth (about 7,000 mph east to west).

Scalar Feed A type of horn antenna feed which uses a series of concentric rings to capture signals that have been reflected toward the focal point of a parabolic antenna.

Scrambler A device used to electronically alter a signal so that it can only be viewed or heard on a receiver equipped with a special decoder.

Secam A color television. system developed by the French and used in the USSR. Secam operates with 625 lines per picture frame and 50 cycles per second, but is incompatible in operation with the European PAL system or the U.S. NTSC system.

Sidelobe Off-axis response of an antenna.

Signal to Noise Ratio (S/N) The ratio of the signal power and noise power. A video S/N of 54 to 56 dB is considered to be an excellent S/N, that is, of broadcast quality. A video S/N of 48 to 52 dB is considered to be a good S/N at the headend for Cable TV.

Single-Channel-Per-Carrier (SCPC) A method used to transmit a large number of signals over a single satellite transponder.

Skew An adjustment that compensates for slight variance in angle between identical senses of polarity generated by two or more satellites.

Slant Range The length of the path between a communications satellite and an associated earth station.

Slot That longitudinal position in the geosynchronous orbit into which a communications satellite is "parked". Above the United States, communications satellites are typically positioned in slots which are based at two to three degree intervals.

Snow A form of noise picked up by a television receiver caused by a weak signal. Snow is characterized by alternate dark and light dots appearing randomly on the picture tube. To eliminate snow, a more sensitive receive antenna must be used, or better amplification must be provided in the receiver (or both).

Solar Outage Solar outages occur when an antenna is looking at a satellite, and the sun passes behind or near the satellite and within the field of view of the antenna. This field of view is usually wider than the beamwidth. Solar outages can be exactly predicted as to the timing for each site.

Spectrum The range of electromagnetic radio frequencies used in transmission of voice, data and television.

Spillover Satellite signal that falls on locations outside the beam pattern's defined edge of coverage.

Spin Stabilization A form of satellite stabilization and attitude control which is achieved through spinning the exterior of the spacecraft about its axis at a fixed rate.

Splitter A passive device (one with no active electronic components) which distributes a television signal carried on a cable in two or more paths and sends it to a number of receivers simultaneously.

Spot Beam A focused antenna pattern sent to a limited geographical area. Spot beams are used by domestic satellites to deliver certain transponder signals to geographically well defined areas such as Hawaii, Alaska and Puerto Rico.

Spread Spectrum The transmission of a signal using a much wider bandwidth and power than would normally be required. Spread spectrum also involves the use of narrower signals that are frequency hopped through various parts of the transponder. Both techniques produce low levels of interference Between the users. They also provide security in that the signals appear as though they were random noise to unauthorized earth stations. Both military and civil satellite applications have developed for spread spectrum transmissions.

SSPA Solid state power amplifier. A VSLI solid state device that is gradually replacing Traveling Wave Tubes in satellite communications systems because they are lighter weight and are more reliable.

Stationkeeping Minor orbital adjustments that are conducted to maintain the satellite's orbital assignment within the allocated "box" within the geostationary arc.

Subcarrier A second signal "piggybacked" onto a main signal to carry additional information. In satellite television transmission, the video picture is transmitted over the main carrier. The corresponding audio is sent via an FM subcarrier. Some satellite transponders carry as many as four special audio or data subcarriers whose signals may or may not be related to the main programming.

Synchronization (Sync) The process of orienting the transmitter and receiver circuits in the proper manner in order that they can be synchronized . Home television sets are synchronized by an incoming sync signal with the television cameras in the studios 60 times per second. The horizontal and vertical hold controls on the television set are used to set the receiver circuits to the approximate sync frequencies of incoming television picture and the sync pulses in the signal then fine tune the circuits to the exact frequency and phase.

T...

T1 The transmission bit rate of 1.544 millions bits per second. This is also equivalent to the ISDN Primary Rate Interface for the U.S. The European T1 or E1 transmission rate is 2.048 million bits per second.

T3 Channel (DS-3) In North America, a digital channel which communicates at 45.304 Mbps.

TDMA Time division multiple access. Refers to a form of multiple access where a single carrier is the shared by many users. Signals from earth stations reaching the satellite consecutively are processed in time segments without overlapping.

TI - Terrestrial Interference Interference to satellite reception caused by ground based microwave transmitting stations.

Transmitter An electronic device consisting of oscillator, modulator and other circuits which produce a radio or television electromagnetic wave signal for radiation into the atmosphere by an antenna.

Transponder A combination receiver, frequency converter, and transmitter package, physically part of a communications satellite. Transponders have a typical output of five to ten watts, operate over a frequency band with a 36 to 72 megahertz bandwidth in the L, C, Ku, and sometimes Ka Bands or in effect typically in the microwave spectrum, except for mobile satellite communications. Communications satellites typically have between 12 and 24 onboard transponders although the INTELSAT VI at the extreme end has 50.

TVRO Television Receive Only terminals that use antenna reflectors and associated electronic equipment to receive and process television and audio communications via satellite. Typically small home systems.

Tweeking The process of adjusting an electronic receiver circuit to optimize its performance.

TWTA Traveling wave tube amplifier.

U...

Uplink The earth station used to transmit signals to a satellite

V...

VSWR Voltage Standing Wave Ratio. A measurement of mismatch in a cable, waveguide, or antenna system.

VSAT Very small aperture terminal. Refers to small earth stations, usually in the 1.2 to 2.4 meter range. Small aperture terminals under 0.5 meters are sometimes referred to Ultra Small Aperture Terminals (USAT's)

W...

Waveguide A metallic microwave conductor, typically rectangular in shape, used to carry microwave signals into and out of microwave antennas.

X...

X.25 A set of packet switching standards published by the CCITT. < P>

Y...

Z...

The definitions found here are from the 1995 International Satellite Directory, published by Design Publishers.

For more information on this and other Design Publishers services, see the Design Publishers Catalog