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| [[Image:Toshiba Vacuum tube Radio .jpg|thumb|A 5-tube superheterodyne receiver made in Japan around 1955]]
| | Hello, I'm Deangelo, a 23 year old from Aix-En-Provence, France.<br>My hobbies include (but are not limited to) Auto audiophilia, Geocaching and watching Doctor Who.<br><br>Feel free to surf to my website ... cell phone tracking [[http://df3D831-manager.appspot.com/ Visit Homepage]] |
| [[File:Superheterod radio.JPG|thumb|right|250px|Superheterodyne [[transistor radio]] circuit around 1975]]
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| In [[electronics]], a '''superheterodyne receiver''' (often shortened to '''superhet'''), invented by US engineer [[Edwin Armstrong]] in 1918 during [[World War 1]],<ref name="Armstrong">{{cite journal
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| | last = Armstrong
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| | first = Edwin H.
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| | title = A new system of short wave amplification
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| | journal = Proc. of the IRE
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| | volume = 9
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| | issue = 1
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| | pages = 3-11
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| | publisher = Institute of Radio Engineers
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| | location = New York
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| | date = February 1921
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| | url = http://books.google.com/books?id=REISAAAAIAAJ&pg=PA3
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| | issn =
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| | doi =
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| | id =
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| | accessdate = 22 October 2013}}</ref> uses [[frequency mixer|frequency mixing]] or [[heterodyne|heterodyning]] to convert a received signal to a fixed [[intermediate frequency]] (IF), which can be more conveniently processed than the original [[radio]] carrier frequency. Virtually all modern radio receivers use the superheterodyne principle.
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| ==History==
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| [[Image:Prototype Armstrong superheterodyne receiver 1920.jpg|thumb|upright=1.5|One of the prototype superheterodyne receivers built at Armstrong's Signal Corps laboratory in Paris during World War 1. It is constructed in two sections, the [[frequency mixer|mixer]] and [[local oscillator]] ''(left)'' and three IF amplification stages and a detector stage ''(right)''. The IF frequency was 75 kHz. ]]
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| ===Background===
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| "Superheterodyne" is a contraction of "supersonic heterodyne", where "supersonic" indicates frequencies above the range of human hearing. The word ''[[heterodyne]]'' is derived from the Greek roots ''hetero-'' "different", and ''-dyne'' "power". In radio applications the term derives from the "heterodyne detector" pioneered by Canadian inventor [[Reginald Fessenden]] in 1905, describing his proposed method of producing an audible signal from the [[Morse code]] transmissions of the new [[continuous wave]] transmitters. With the older [[spark gap transmitter]]s then in use, the Morse code signal consisted of short bursts of a heavily modulated carrier wave which could be clearly heard as a series of short chirps or buzzes in the receiver's headphones. However, the signal from a continuous wave transmitter did not have any such inherent modulation and Morse Code from one of those would only be heard as a series of clicks or thumps. Fessenden's idea was to run two Alexanderson alternators, one producing a carrier frequency 3 kHz higher than the other. In the receiver's detector the two carriers would [[Beat_%28acoustics%29#Mathematics_and_physics_of_beat_tones|beat]] together to produce a 3 kHz tone thus in the headphones the Morse signals would then be heard as a series of 3 kHz beeps. For this he coined the term "heterodyne" meaning "generated by a difference" (in frequency).
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| ===Invention===
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| The superheterodyne principle was devised in 1918 by [[U.S. Army]] [[Major]] [[Edwin Armstrong]] in [[France]] during [[World War I]].<ref name="luxor">{{Cite web|url=http://www.astrosurf.com/luxorion/qsl-ham-history-landmarks.htm|title=The History of Amateur Radio|publisher=Luxorion date unknown|accessdate=19 January 2011}}</ref><ref>{{Citation |first=Tapan K. |last=Sarkar |first2=Robert J. |last2=Mailloux |first3=Arthur A. |last3=Oliner |first4=Magdalena |last4=Salazar-Palma |first5=Dipak L. |last5=Sengupta |title=History of Wireless |publisher=John Wiley and Sons |year=2006 |isbn=0-471-71814-9 |doi= }}, p 110?</ref> He invented this receiver as a means of overcoming the deficiencies of early vacuum tube [[triode]]s used as high-frequency amplifiers in radio [[direction finding]] equipment. Unlike simple radio communication, which only needs to make transmitted signals audible, direction-finders measure the received signal strength, which necessitates linear amplification of the actual [[carrier wave]].
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| [[Image:Homemade superheterodyne receiver 1920.jpg|thumb|One of the first amateur superheterodyne receivers, built in 1920 even before Armstrong published his paper. Due to the low gain of early triodes it required 9 tubes, with 5 IF amplification stages, and used an IF of around 50 kHz. ]]
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| In a triode radio-frequency (RF) amplifier, if both the plate (anode) and grid are connected to resonant circuits tuned to the same frequency, stray [[capacitive coupling]] between the grid and the plate will cause the amplifier to go into oscillation if the stage gain is much more than [[unity (mathematics)|unity]]. In early designs, dozens (in some cases over 100) low-gain triode stages had to be connected in cascade to make workable equipment, which drew enormous amounts of power in operation and required a team of maintenance engineers. The strategic value was so high, however, that the [[British Admiralty]] felt the high cost was justified.
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| Armstrong realized that if radio direction-finding (RDF) receivers could be operated at a higher frequency, this would allow better detection of enemy shipping. However, at that time, no practical "short wave" (defined then as any frequency above 500 kHz) amplifier existed, due to the limitations of existing triodes.
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| It had been noticed some time before that if a [[Regenerative circuit|regenerative]] receiver was allowed to go into oscillation, other receivers nearby would suddenly start picking up stations on frequencies different from those that the stations were actually transmitted on. Armstrong (and others) eventually deduced that this was caused by a "supersonic heterodyne" between the station's carrier frequency and the oscillator frequency. Thus if a station was transmitting on 300 kHz and the oscillating receiver was set to 400 kHz, the station would be heard not only at the original 300 kHz, but also at 100 kHz and 700 kHz.
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| Armstrong realized that this was a potential solution to the "short wave" amplification problem, since the beat frequency still retained its original modulation, but on a lower carrier frequency. To monitor a frequency of 1500 kHz for example, he could set up an oscillator at, for example, 1560 kHz, which would produce a heterodyne difference frequency of 60 kHz, a frequency that could then be more conveniently amplified by the triodes of the day. He termed this the "[[Intermediate Frequency]]" often abbreviated to "IF".
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| <blockquote>In December 1919, Major E. H. Armstrong gave publicity to an indirect method of obtaining short-wave amplification, called the super-heterodyne. The idea is to reduce the incoming frequency which may be, say 1,500,000 cycles (200 meters), to some suitable super-audible frequency which can be amplified efficiently, then passing this current through a radio frequency amplifier and finally rectifying and carrying on to one or two stages of audio frequency amplification.<ref>(page 11 of December 1922 [[QST|QST magazine]])</ref></blockquote>
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| ===Development===
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| Armstrong was able to rapidly put his ideas into practice, and the technique was rapidly adopted by the military. However, it was less popular when commercial [[radio broadcasting]] began in the 1920s, mostly due to the need for an extra tube (for the oscillator), the generally higher cost of the receiver, and the level of technical skill required to operate it. For early domestic radios, [[tuned radio frequency receiver]]s ("TRF"), also called the [[Neutrodyne]], were more popular because they were cheaper, easier for a non-technical owner to use, and less costly to operate. Armstrong eventually sold his superheterodyne patent to [[Westinghouse Electric (1886)|Westinghouse]], who then sold it to [[RCA]], the latter monopolizing the market for superheterodyne receivers until 1930.<ref>{{cite web|last=Katz|first=Eugenii|title=Edwin Howard Armstrong|work=History of electrochemistry, electricity, and electronics|publisher=[http://www.geocities.com/neveyaakov/ Eugenii Katz homepage, Hebrew Univ. of Jerusalem]|url=http://www.geocities.com/neveyaakov/electro_science/armstrong.html|accessdate=2008-05-10|archiveurl=http://web.archive.org/web/20091022120609/http://geocities.com/neveyaakov/electro_science/armstrong.html|archivedate=2009-10-22}}</ref>
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| Early superheterodyne receivers used IFs as low as 20 kHz, often based on the self-resonance of iron-cored [[transformer]]s. This made them extremely susceptible to [[Superheterodyne_receiver#Image_frequency_.28fimg.29|image frequency]] interference, but at the time, the main objective was sensitivity rather than selectivity. Using this technique, a small number of triodes could be made to do the work that formerly required dozens of triodes.
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| In the 1920s, commercial IF filters looked very similar to 1920s audio interstage coupling transformers, had very similar construction and were wired up in an almost identical manner, and so they were referred to as "IF Transformers". By the mid-1930s however, superheterodynes were using much higher intermediate frequencies, (typically around 440–470 kHz), with tuned coils similar in construction to the aerial and oscillator coils. However, the name "IF Transformer" was retained and is still used today. Modern receivers typically use a mixture of [[ceramic resonator]] or [[Electronic filter#SAW filters|SAW]] (surface-acoustic wave) resonators as well as traditional tuned-inductor IF transformers.
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| {{multiple image
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| | image1 = Philco radio model PT44 front.jpg
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| | image2 = Philco radio model PT44 chassis back.jpg
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| | footer = By the 1940s the vacuum-tube superheterodyne AM broadcast receiver was refined into a cheap-to-manufacture design called the "[[All American Five]]", because it only used five vacuum tubes: usually a converter (mixer/local oscillator), an IF amplifier, a detector/audio amp, audio power amp, and a rectifier.
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| }}
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| By the 1930s, improvements in vacuum tube technology rapidly eroded the TRF receiver's cost advantages, and the explosion in the number of broadcasting stations created a demand for cheaper, higher-performance receivers.
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| The development of the [[tetrode]] vacuum tube containing a [[screen grid]] led to a multi-element tube in which the mixer and oscillator functions could be combined, first used in the so-called [[autodyne]] mixer. This was rapidly followed by the introduction of tubes specifically designed for superheterodyne operation, most notably the [[pentagrid converter]]. By reducing the tube count, this further reduced the advantage of preceding receiver designs.
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| By the mid-1930s, commercial production of TRF receivers was largely replaced by superheterodyne receivers. The superheterodyne principle was eventually taken up for virtually all commercial radio and TV designs.
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| ==Design and principle of operation==
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| The principle of operation of the superheterodyne receiver depends on the use of [[heterodyning]] or [[frequency mixer|frequency mixing]]. The signal from the antenna is filtered sufficiently at least to reject the ''[[Superheterodyne_receiver#Image_frequency_.28fimg.29|image frequency]]'' (see below) and possibly amplified. A [[local oscillator]] in the receiver produces a sine wave which [[frequency mixer|mixes]] with that signal, shifting it to a specific [[intermediate frequency]] (IF), usually a lower frequency. The IF signal is itself filtered and amplified and possibly processed in additional ways. The [[demodulator]] uses the IF signal rather than the original radio frequency to recreate a copy of the original information (such as audio).
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| [[Image:Superhet2.svg|frame|right|Block diagram of a typical superheterodyne receiver]]
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| The diagram at right shows the minimum requirements for a single-conversion superheterodyne receiver design. The following essential elements are common to all superheterodyne circuits:<ref name=Carr02>Joseph J. Carr ''RF Components and Circuits'' Newnes, 2002 ISBN 978-0-7506-4844-8 , Chapter 3</ref> a receiving [[Antenna (radio)|antenna]], a tuned stage which may optionally contain amplification (RF amplifier), a variable frequency [[local oscillator]], a [[frequency mixer]], a band pass filter and [[intermediate frequency]] (IF) amplifier, and a demodulator plus additional circuitry to amplify or process the original audio signal (or other transmitted information).
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| ===Circuit description===
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| To receive a radio signal, a suitable [[Antenna (radio)|antenna]] is required. This is often built into a receiver, especially in the case of AM broadcast band radios. The output of the antenna may be very small, often only a few [[microvolt]]s. The signal from the antenna is tuned and may be amplified in a so-called radio frequency (RF) amplifier, although this stage is often omitted. One or more [[tuned circuit]]s at this stage block frequencies which are far removed from the intended reception frequency. In order to tune the receiver to a particular station, the frequency of the local oscillator is controlled by the tuning knob (for instance). Tuning of the local oscillator and the RF stage may use a [[variable capacitor]], or [[varicap diode]].<ref>{{Cite book|url=http://books.google.co.uk/books?id=QtJ5tNdlyYAC&pg=PA58&dq=radio+local+oscillator+tuning+varicap#v=onepage&q&f=false|title=Radio-frequency electronics: circuits and applications By Jon B. Hagen -p.58 l. 12|publisher=Cambridge University Press, 1996 - Technology & Engineering|accessdate=17 January 2011}}</ref> The tuning of one (or more) tuned circuits in the RF stage must track the tuning of the local oscillator.
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| Notice that the accompanying diagram shows a fixed-frequency local oscillator, as the symbol is for a fixed-frequency crystal frequency-determining device. A tuneable receiver would show a variable-frequency oscillator with operational connection to the tuned circuits of the antenna and radio-frequency amplifier stages.
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| ===Local oscillator and mixer===
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| The signal is then fed into a circuit where it is mixed with a sine wave from a variable frequency oscillator known as the [[local oscillator]] (LO). The mixer uses a non-linear component to produce both sum and difference [[Beat (acoustics)#Mathematics and physics of beat tones|beat frequencies]] signals,<ref>{{Cite book |url=http://books.google.co.uk/books?id=bkOMDgwFA28C&pg=PA886&f=false |title=The art of electronics |pages=886 |publisher=Cambridge University Press |year=2006 |accessdate=17 January 2011 }}</ref> each one containing the [[modulation]] contained in the desired signal. The output of the mixer may include the original RF signal at ''f''<sub>RF</sub>, the local oscillator signal at ''f''<sub>LO</sub>, and the two new heterodyne frequencies ''f''<sub>RF</sub> + ''f''<sub>LO</sub> and ''f''<sub>RF</sub> − ''f''<sub>LO</sub>. The mixer may inadvertently produce additional frequencies such as third- and higher-order intermodulation products. Ideally, the IF [[bandpass filter]] removes all but the desired IF signal at ''f''<sub>IF</sub>. The IF signal contains the original modulation (transmitted information) that the received radio signal had at ''f''<sub>RF</sub>.
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| Historically, vacuum tubes were expensive, so broadcast AM receivers would save costs by employing a single tube as both a mixer and also as the local oscillator. The [[pentagrid converter]] tube would oscillate and also provide signal amplification as well as frequency shifting.<ref>{{Cite patent |inventor-last= |inventor-first= |inventorlink= |country-code=GB |patent-number=426802 |title=Improvements in or relating to superheterodyne radio receivers |publication-date=12 October 1933 |issue-date= }}</ref>
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| The frequency of the local oscillator ''f''<sub>LO</sub> is set so the desired reception radio frequency ''f''<sub>RF</sub> mixes to ''f''<sub>IF</sub>. There are two choices for the local oscillator frequency because the dominant mixer products are at ''f''<sub>RF</sub> ± ''f''<sub>LO</sub>. If the local oscillator frequency is less than the desired reception frequency, it is called '''low-side injection''' (''f''<sub>IF</sub> = ''f''<sub>RF</sub> - ''f''<sub>LO</sub>); if the local oscillator is higher, then it is called '''high-side injection''' (''f''<sub>IF</sub> = ''f''<sub>LO</sub> - ''f''<sub>RF</sub>).<!-- only cases for difference mixing given -->
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| The mixer will process not only the desired input signal at f<sub>RF</sub>, but also all signals present at its inputs. There will be many mixer products (heterodynes).<!-- ignoring higher order products --> Most other signals produced by the mixer (such as due to stations at nearby frequencies) can be [[Filter (signal processing)|filtered]] out in the IF amplifier;<!-- dynamic range issues --> that gives the superheterodyne receiver its superior performance. However, if ''f''<sub>LO</sub> is set to ''f''<sub>RF</sub> + ''f''<sub>IF</sub>, then an incoming radio signal at ''f''<sub>LO</sub> + ''f''<sub>IF</sub> will ''also'' produce a heterodyne at ''f''<sub>IF</sub>; this is called the ''image frequency'' and must be rejected by the tuned circuits in the RF stage. The image frequency is 2 ''f''<sub>IF</sub> higher (or lower) than ''f''<sub>RF</sub>, so employing a higher IF frequency ''f''<sub>IF</sub> increases the receiver's ''image rejection'' without requiring additional selectivity in the RF stage.
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| To suppress the unwanted image, the tuning of the RF stage and the LO may need to "track" each other. In some cases, a narrow-band receiver can have a fixed tuned RF amplifier. In that case, only the local oscillator frequency is changed. In most cases, a receiver's input band is wider than its IF center frequency. For example, a typical AM broadcast band receiver covers 510 kHz to 1655 kHz (a roughly 1160 kHz input band) with a 455 kHz IF frequency; an FM broadcast band receiver covers 88 MHz to 108 MHz band with a 10.7 MHz IF frequency. In that situation, the RF amplifier must be tuned so the IF amplifier does not see two stations at the same time. If the AM broadcast band receiver LO were set at 1200 kHz, it would see stations at both 745 kHz (1200−455 kHz) and 1655 kHz. Consequently, the RF stage must be designed so that any stations that are twice the IF frequency away are significantly attenuated.. The tracking can be done with a multi-section variable capacitor or some [[varactor]]s driven by a common control voltage. An RF amplifier may have tuned circuits at both its input and its output, so three or more tuned circuits may be tracked. In practice, the RF and LO frequencies need to track closely but not perfectly.<ref>{{Citation |first=Frederick Emmons |last=Terman |title=Radio Engineers' Handbook |year=1943 |publisher=McGraw-Hill |location=New York }}. Pages 649–652 describes design procedure for tracking with a pad capacitor in the Chebyshev sense.</ref><ref>{{Citation |first=Ulrich L. |last=Rohde |first2=T. T. N. |last2=Bucher |title=Communications Receivers: Principles & Design |year=1988 |location=New York |publisher=McGraw-Hill |isbn=0-07-053570-1}}. Pages 155–160 discuss frequency tracking. Pages 160–164 discuss image rejection and include an RF filter design that puts transmission zeros at both the local oscillator frequency and the unwanted image frequency.</ref>
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| ===Intermediate frequency amplifier===
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| The stages of an intermediate frequency amplifier ("IF amplifier" or "IF strip") are tuned to a fixed frequency that does not change as the receiving frequency changes. The fixed frequency simplifies optimization of the IF amplifier.<ref name=Carr02/> The IF amplifier is selective around its center frequency ''f''<sub>IF</sub>. The fixed center frequency allows the stages of the IF amplifier to be carefully tuned for best performance (this tuning is called "aligning" the IF amplifier). If the center frequency changed with the receiving frequency, then the IF stages would have had to track their tuning. That is not the case with the superheterodyne.
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| Typically, the IF center frequency ''f''<sub>IF</sub> is chosen to be less than the desired reception frequency ''f''<sub>RF</sub>. The choice has some performance advantages. First, it is easier and less expensive to get high selectivity at a lower frequency. For the same bandwidth, a tuned circuit at a lower frequency needs a lower Q. Stated another way, for the same filter technology, a higher center frequency will take more IF filter stages to achieve the same selectivity bandwidth. Second, it is easier and less expensive to get high gain at a lower frequency. When used at high frequencies, many amplifiers show a constant [[gain–bandwidth product]] (dominant pole) characteristic. If an amplifier has a gain–bandwidth product of 100 MHz, then it would have a voltage gain of 100 at 1 MHz but only 10 at 10 MHz. If the IF amplifier needed a voltage gain of 10,000, then it would need only two stages with an IF at 1 MHz but four stages at 10 MHz.
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| Usually the intermediate frequency is lower than the reception frequency ''f''<sub>RF</sub>, but in some modern receivers (e.g. scanners and spectrum analyzers) a higher IF frequency is used to minimize problems with image rejection or gain the benefits of fixed-tuned stages. The Rohde & Schwarz EK-070 VLF/HF receiver covers 10 kHz to 30 MHz.<ref>{{Harvnb|Rohde|Bucher|1988|pp=44–55}}</ref> It has a band switched RF filter and mixes the input to a first IF of 81.4 MHz. The first LO frequency is 81.4 to 111.4 MHz, so the primary images are far away. The first IF stage uses a crystal filter with a 12 kHz bandwidth. There is a second frequency conversion (making a triple-conversion receiver) that mixes the 81.4 MHz first IF with 80 MHz to create a 1.4 MHz second IF. Image rejection for the second IF is not a major problem because the first IF provides adequate image rejection and the second mixer is fixed tuned.<!-- easy to place zero at image frequency. -->
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| In order to avoid interference to receivers, licensing authorities will avoid assigning common IF frequencies to transmitting stations. Standard intermediate frequencies used are 455 kHz for [[medium-wave]] AM radio, 10.7 MHz for broadcast FM receivers, 38.9 MHz (Europe) or 45 MHz (US) for television, and 70 MHz for satellite and terrestrial microwave equipment. To avoid [[Machine tool|tooling costs]] associated with these components, most manufacturers then tended to design their receivers around a fixed range of frequencies offered which resulted in a worldwide ''de facto'' standardization of intermediate frequencies.
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| In early superhets, the IF stage was often a regenerative stage providing the sensitivity and selectivity with fewer components. Such superhets were called super-gainers or regenerodynes.{{Citation needed|date=October 2011}}
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| ===Bandpass filter===
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| The IF stage includes a filter and/or multiple tuned circuits in order to achieve the desired [[selectivity (electronic)|selectivity]]. This filtering must therefore have a band pass equal to or less than the frequency spacing between adjacent broadcast channels. Ideally a filter would have a high attenuation to adjacent channels, but maintain a flat response across the desired signal spectrum in order to retain the quality of the received signal. This may be obtained using one or more dual tuned IF transformers, a quartz [[crystal filter]], or a multipole [[ceramic resonator | ceramic crystal filter]].<ref>{{Cite web|url=http://www.qsl.net/va3iul/Homebrew_RF_Circuit_Design_Ideas/Crystal_Filter_Types.gif|title=Crystal filer types|publisher=QSL RF Circuit Design Ideas Date unknown|accessdate=17 January 2011}}</ref>
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| ===Demodulation===
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| The received signal is now processed by the [[demodulator]] stage where the audio signal (or other [[baseband]] signal) is recovered and then further amplified. AM demodulation requires the simple [[rectification (electricity)|rectification]] of the RF signal (so-called [[envelope detector|envelope detection]]), and a simple RC low pass filter to remove remnants of the intermediate frequency.<ref>{{Cite web |url=http://bc.inter.edu/facultad/rflores/ELEN4360/Labs/Com1_Lab3.pdf |title=Reception of Amplitude Modulated Signals - AM Demodulation |publisher=BC Internet education 6/14/2007 |accessdate=17 January 2011}}</ref> FM signals may be detected using a discriminator, [[Detector (radio)#Ratio detector|ratio detector]], or [[phase-locked loop]]. [[Continuous wave]] ([[Morse code]]) and [[single sideband]] signals require a [[product detector]] using a so-called [[beat frequency oscillator]], and there are other techniques used for different types of [[modulation]].<ref>{{Cite web |url=http://www.dbugman.com/handbook/tscmh5.html |title=Basic Radio Theory |publisher=TSCM Handbook Ch.5 date unknown |accessdate=17 January 2011}}</ref> The resulting audio signal (for instance) is then amplified and drives a loudspeaker.
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| When so-called '''high-side injection''' has been used, where the local oscillator is at a ''higher'' frequency than the received signal (as is common), then the frequency spectrum of the original signal will be reversed. This must be taken into account by the demodulator (and in the IF filtering) in the case of certain types of modulation such as [[single sideband]].
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| ==Advanced designs==
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| To overcome obstacles such as [[image response]], in some cases multiple stages with two or more IFs of different values are used. For example, for a receiver that can tune from 500kHz to 30MHz, three frequency converters might be used, and the radio would be referred to as a ''triple conversion superheterodyne'';<ref name=Carr02/>
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| The reason that this is done is the difficulty in obtaining sufficient selectivity in the front-end tuning with higher shortwave frequencies.
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| With a 455kHz IF it is easy to get adequate front end selectivity with broadcast band (under 1600kHz) signals. For example, if the station being received is on 600kHz, the local oscillator will be set to 600 + 455 = 1055kHz. But a station on 1510kHz could also potentially produce an IF of 455kHz and so cause image interference. However because 600kHz and 1510kHz are so far apart, it is easy to design the front end tuning to reject the 1510kHz frequency.
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| However at 30MHz, things are different. The oscillator would be set to 30.455MHz to produce a 455kHz IF, but a station on 30.910 would also produce a 455kHz beat, so both stations would be heard at the same time. But it is virtually impossible to design an RF tuned circuit that can adequately discriminate between 30MHz and 30.91MHz, so one approach is to "bulk downconvert" whole sections of the shortwave bands to a lower frequency, where adequate front-end tuning is easier to arrange.
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| For example the ranges 29MHz to 30MHz; 28MHz to 29MHz etc. might be converted down to 2MHz to 3 MHz, there they can be tuned more conveniently. This is often done by first converting each "block" up to a higher frequency (typically 40MHz) and then using a second mixed to convert it down to the 2MHz to 3 MHz range. The 2MHz to 3 MHz "IF" is basically another self-contained superheterodyne receiver, most likely with a standard IF of 455kHz.
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| ===Other uses===
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| In the case of modern television receivers, no other technique was able to produce the precise [[bandpass]] characteristic needed for [[vestigial sideband]] reception, similar to that used in the [[NTSC]] system first approved by the U.S. in 1941. By the 1980s these had been replaced with precision electromechanical [[surface acoustic wave]] (SAW) [[Electronic filter|filters]]. Fabricated by precision laser milling techniques, SAW filters are cheaper to produce, can be made to extremely close tolerances, and are very stable in operation.
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| ===Modern designs===
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| Microprocessor technology allows replacing the superheterodyne receiver design by a [[software defined radio]] architecture, where the IF processing after the initial IF filter is implemented in software. This technique is already in use in certain designs, such as very low-cost FM radios incorporated into mobile phones, since the system already has the necessary [[microprocessor]].
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| [[Radio transmitter]]s may also use a mixer stage to produce an output frequency, working more or less as the reverse of a superheterodyne receiver.
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| ==Advantages and drawbacks of the superheterodyne design==
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| Superheterodyne receivers have essentially replaced all previous receiver designs. The development of modern [[semiconductor]] electronics negated the advantages of designs (such as the [[regenerative receiver]]) which used fewer vacuum tubes. The superheterodyne receiver offers superior sensitivity, frequency stability and selectivity. Compared with the [[tuned radio frequency receiver]] (TRF) design, superhets offer better stability because a tuneable oscillator is more easily realized than a tuneable amplifier. Operating at a lower frequency, IF filters can give narrower passbands at the same [[Q factor]] than an equivalent RF filter. A fixed IF also allows the use of a [[crystal filter]]<ref name=Carr02/> or similar technologies which cannot be tuned. [[Regenerative circuit|Regenerative]] and super-regenerative receivers offered a high sensitivity, but often suffer from stability problems making them difficult to operate.
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| Although the advantages of the superhet design are overwhelming, we note a few drawbacks which need to be tackled in practice.
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| ===Image frequency (''f''<sub>img</sub>)===
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| One major disadvantage to the superheterodyne receiver is the problem of image frequency. In heterodyne receivers, an image frequency is an undesired input frequency equal to the station frequency plus twice the intermediate frequency. The image frequency results in two stations being received at the same time, thus producing interference. Image frequencies can be eliminated by sufficient [[attenuation]] on the incoming signal by the RF amplifier filter of the superheterodyne receiver.
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| :<math>f_\mathrm{img} = \begin{cases} f + 2f_\mathrm{IF} , & \mbox{if } f_\mathrm{LO} > f \mbox{ (high side injection)}\\ f- 2f_\mathrm{IF}, & \mbox{if } f_\mathrm{LO} < f \mbox{ (low side injection)} \end{cases} </math>
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| For example, an AM broadcast station at 580 kHz is tuned on a receiver with a 455 kHz IF. The local oscillator is tuned to {{nowrap|580 + 455 {{=}}}} 1035 kHz. But a signal at {{nowrap|580 + 455 + 455 {{=}}}} 1490 kHz is also 455 kHz away from the local oscillator; so both the desired signal and the image, when mixed with the local oscillator, will also appear at the intermediate frequency. This image frequency is within the AM broadcast band. Practical receivers have a tuning stage before the converter, to greatly reduce the amplitude of image frequency signals; additionally, broadcasting stations in the same area have their frequencies assigned to avoid such images.
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| The unwanted frequency is called the ''image'' of the wanted frequency, because it is the "mirror image" of the desired frequency reflected <math>f_{o}\!</math>. A receiver with inadequate filtering at its input will pick up signals at two different frequencies simultaneously: the desired frequency and the image frequency. Any noise or random radio station at the image frequency can interfere with reception of the desired signal.
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| Early [[Autodyne]] receivers typically used IFs of only 150 kHz or so, as it was difficult to maintain reliable oscillation if higher frequencies were used. As a consequence, most Autodyne receivers needed quite elaborate antenna tuning networks, often involving double-tuned coils, to avoid image interference. Later superhets used tubes especially designed for oscillator/mixer use, which were able to work reliably with much higher IFs, reducing the problem of image interference and so allowing simpler and cheaper aerial tuning circuitry.
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| Sensitivity to the image frequency can be minimised only by (1) a filter that precedes the mixer or (2) a more complex mixer circuit [http://www.freepatentsonline.com/7227912.html] that suppresses the image. In most receivers this is accomplished by a [[bandpass filter]] in the [[RF front end]]. In many tunable receivers, the bandpass filter is tuned in tandem with the local oscillator.
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| Image rejection is an important factor in choosing the intermediate frequency of a receiver. The farther apart the bandpass frequency and the image frequency are, the more the bandpass filter will attenuate any interfering image signal. Since the frequency separation between the bandpass and the image frequency is <math>2f_\mathrm{IF}\!</math>, a higher intermediate frequency improves image rejection. It may be possible to use a high enough first IF that a fixed-tuned RF stage can reject any image signals.
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| The ability of a receiver to reject interfering signals at the image frequency is measured by the [[image rejection ratio]]. This is the ratio (in [[decibel]]s) of the output of the receiver from a signal at the received frequency, to its output for an equal-strength signal at the image frequency.
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| ===Local oscillator radiation===
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| {{further2|[[Electromagnetic compatibility]]}}
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| It is difficult to keep stray radiation from the local oscillator below the level that a nearby receiver can detect. The receiver's local oscillator can act like a low-power [[Continuous wave|CW]] transmitter. Consequently, there can be mutual interference in the operation of two or more superheterodyne receivers in close proximity.
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| In intelligence operations, local oscillator radiation gives a means to detect a covert receiver and its operating frequency. The method was used by MI-5 during [[Operation RAFTER]].<ref>Peter Wright: ''Spycatcher: The Autobiography of a Senior Intelligence Officer'', by Peter Wright, 1987.</ref>
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| A method of significantly reducing the local oscillator radiation from the receiver's antenna is to use an RF amplifier between the receiver's antenna and its mixer stage.
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| ===Local oscillator sideband noise===
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| Local oscillators typically generate a single frequency signal that has negligible [[amplitude modulation]] but some random [[phase modulation]]. Either of these impurities spreads some of the signal's energy into sideband frequencies. That causes a corresponding widening of the receiver's frequency response, which would defeat the aim to make a very narrow bandwidth receiver such as to receive low-rate digital signals. Care needs to be taken to minimize oscillator phase noise, usually by ensuring that the oscillator never enters a [[non-linear]] mode.
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| ==See also==
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| *[[H2X radar]]
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| *[[Automatic gain control]]
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| *[[Demodulator]]
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| *[[Direct conversion receiver]]
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| *[[VFO]]
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| *[[Single sideband#Demodulation|Single sideband modulation (demodulation)]]
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| *[[Tuned radio frequency receiver]]
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| *[[Reflectional receiver]]
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| *[[Beat frequency]]
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| *[[Heterodyne]]
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| *[[Optical heterodyne detection]]
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| *[[Infradyne]] - superheterodyne with IF higher than signal frequency
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| *[[Superheterodyne transmitter]]
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| ==References==
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| {{reflist|30em}}
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| ==Further reading==
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| *{{cite book |title=The Electronics Handbook |last=Whitaker |first=Jerry |authorlink= |year=1996 |publisher=CRC Press |location= |isbn=0-8493-8345-5 |pages=1172 }}
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| *{{Citation |inventor-last=Fessenden |inventor-first=Reginald A. |inventorlink=Reginald Fessenden |title=Wireless Signaling |country-code=US |patent-number= 706740 |issue-date=August 12, 1902 |publication-date= September 28, 1901 }}
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| *{{Citation |inventor-last=Fessenden |inventor-first=Reginald A. |inventorlink=Reginald Fessenden |title=Electric Signaling Apparatus |country-code=US |patent-number=1050441 |issue-date=January 14, 1913 |publication-date=July 27, 1905 }}
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| *{{Citation |inventor-last=Fessenden |inventor-first=Reginald A. |inventorlink=Reginald Fessenden |title=Method of Signaling |country-code=US |patent-number=1050728 |issue-date=January 14, 1913 |publication-date=August 21, 1906 }}
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| == External links ==
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| {{Commons category|Superheterodyne circuits}}
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| *[http://antiqueradios.com/superhet/ Who Invented the Superheterodyne?] An article giving the history of the various inventors working on the superheterodyne method.
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| *[http://www.qsl.net/vu2msy/receiver.htm An in-depth introduction to superheterodyne receivers]
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| *[http://www.microwaves101.com/encyclopedia/receivers_superhet.cfm Superheterodyne receivers from microwaves101.com]
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| {{Telecommunications}}
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| {{DEFAULTSORT:Superheterodyne Receiver}}
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| [[Category:Radio electronics]]
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| [[Category:Communication circuits]]
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| [[Category:Electronic design]]
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| [[Category:History of radio]]
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| [[Category:Receiver (radio)]]
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