SAT Infrared seekers for Matra R 530 and Magic AAMs

overscan (PaulMM)

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SAT (infrared activity)

We indicated above that, during the first period, the bases of infrared detection, in particular the laws of atmospheric transmission, had been explained. Infrared technology (detector cells, filters, grid for determining the deviation) relating to the first spectral band had been developed and had enabled Turck to produce initial equipment: prototype goniometer for the SS 11 and homing device for the R 511 (not mass-produced).
During the second period, the study areas and equipment developed were infrared components and measurement of aircraft radiation, homing devices for Matra air-to-air missiles in band 2 [3-5 microns], goniometers for the firing stations of Nord-Aviation guided missiles, in band 1 [1.8-3 microns], and the single-line infrared analyzer for aircraft or reconnaissance missiles. We will discuss them successively.

In 1958, the STAé/ES directed studies towards the development of spectral band 2 technology. The objective was to produce an IR seeker detecting in this band for the equipment of the Matra R 530, which was to be launched in development in September 1958. The operational interest was considerable, since this band allowed for “all-sector” detection of aircraft, unlike band 1, which limited detection to the rear area of aircraft. It was a gamble, because the American Sidewinder 9 B missile, revealed in 1957, used band 1; it was only from 1978 that the 9 L version was operational in band 2.

The SAT succeeded in this difficult gamble in a record time of two years. The technology was complex: InSb detector cell (binary compound of indium antimonide with photovoltaic effect); cooler at the operating temperature of the cell, i.e. 77° K (by liquid nitrogen tank), produced in cooperation with the Air Liquide company; hemispherical-shaped irdome made of resistant and transparent material (lead germanate), designed in cooperation with Paramontois (later Sovirel). On the other hand, from 1957 to 1962, the STAé had the CEV carry out a major program of ground and in-flight measurements of the radiation from the jet of the reactors. For the measurement of the spectra, suitable spectroscopes were necessary; they were produced by the SAT according to the indications provided by Professor Barchewitz.

All these studies of infrared components and these measurements of the radiation were financed by the STAé/ES, until 1970, by annual contracts under general studies. The support of the STAé was constant.

The homing devices (AD) for the Matra air-to-air missiles in band 2 concerned the R 530 and the Magic 1 and 2.

The one for the R 530 was a modern homing device adapted to proportional navigation (see Appendix No. 3). With its spectral band, it allowed firing "all sectors" day and night, except in a cone of ± 5° relative to the direction of the sun; the gyroscopic head was made by SAGEM. The electronics initially included miniaturized tubes; it was transistorized in 1961.

The schedule was as follows:
- first firing of the missile (without charge) in September 1961, with a CT 20 target, destroyed by a very spectacular impact;
- during development and evaluation, numerous firings with impact took place;
- in mid-1964, start of series delivery: approximately 800 units were produced.

The progress since 1957 was considerable.
Liquid nitrogen production facilities were installed by Air Liquide on air bases; they used existing facilities for oxygen. The only defect that appeared for the AD was the filling of its nitrogen canister: it was a simple operation, but not always appreciated by the track mechanics.

The Magic 1 is the first combat missile with only an infrared AD; the Magic 2 is the more efficient version, especially for the AD. Compared to the R 530, the Magic 1's homing system was more modern and lighter (10 kg with the gyroscope for stabilization, instead of 20 kg). In particular, the liquid nitrogen tank was replaced by a Joule-Thomson cooler using the expansion of dry nitrogen under pressure (400 bars), stored in a bottle installed in the missile launcher (British design for the cooler); this solution was deemed operationally satisfactory.

The Magic 2's AD differed from the Magic 1 primarily in the use of a multi-element detector, which allowed the range to be increased. The “single cell and modulator” solution was dead: it was a first step towards the solution of the 1980s strip. The electronics were modernized: 1980 technology and improved anti-decoy control. For the irdome, a new material (sintered magnesium fluoride), more resistant to erosion when passing through clouds, was adopted; it was produced by the ceramicist, the Desmarquet company. The developments took place, respectively, for Magic1 and 2, from 1969 to 1975 and from 1978 to 1986. 12,000 seekers were produced.

Translated from https://eurosae.com/wp-content/uploads/2025/05/R_Carpentier_Missiles_tactiques.pdf
 
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So R.530 was all aspect against non supersonic targets?
 
So R.530 was all aspect against non supersonic targets?
Doubt it. Contemporary Red Top had side on capability but headon was only indicated for supersonic targets in afterburner.

I assume early indium antimonide seekers were less sensitive than mid 1970s ones, so head-on range was very short for subsonic non-afterburning targets.
 
SAT (infrared activity)

We indicated above that, during the first period, the bases of infrared detection, in particular the laws of atmospheric transmission, had been explained. Infrared technology (detector cells, filters, grid for determining the deviation) relating to the first spectral band had been developed and had enabled Turck to produce initial equipment: prototype goniometer for the SS 11 and homing device for the R 511 (not mass-produced).
Thanks for the extract on SAT infrared activity, which contains a lot of useful information and appears to be authoritative. It would be very helpful if you could identify the reference for the source you have quoted from?
 
https://eurosae.com/comaero/

This specific document has a lot of information about the -530 family of AAMs, also Magic 1 and 2.
https://eurosae.com/wp-content/uploads/2025/05/R_Carpentier_Missiles_tactiques.pdf
Merci beaucoup. The COMAERO work on "Tactical Missiles", written by René Carpentier, gives a great overview of air-to-air missile development in France. My main research is into the parallel British development of Firestreak and Red Top, and it is very interesting to compare the timelines of the French, British and American IR missile developments.

The English version of a more recent book by Patrick Mercillion, "European Tactical Missiles, the First Hundred Years", sponsored by MBDA and published in 2017, confuses the IR seeker standard by giving the following apparently contradictory statements in the section on the R.530:

page 174; "SAT even managed to develop an entirely new missile seeker using a lead sulphide detector and a gyroscopic head". I wonder if this refers to an early prototype with a PbS detector that was superseded in the final design standard by one with a cooled indium antimonide (InSb) detector? Can anyone offer an explanation?
page 175; "The R.530 IR also had the edge over the Sidewinder in terms of range, and an infrared seeker operating in band 2 (supporting head-on attack) rather than band 1 (attack only in pursuit mode, from the rear)." Note that the Sidewinder version is not explicit, but another Sidewinder mention in the R.530 section refer to the AIM-9B, which had an uncooled PbS detector. Note that the upgrade to a cooled PbS IR detector in the AIM-9D gave it increased sensitivity and, together with the increase in cut-off wavelength from 3.0 to around 3.8µ, some increase in angle-off-tail capability, but the AIM-9D was still limited to rear attacks.

I will need to check whether the text posted by PaulMM, on "SAT (infrared activity)", is all lifted from the René Carpentier document, or if it goes into additional detail. Hopefully, PaulMM will clarify his source.
 
Thanks for the link to your source. This is the same as one if the links identified by Archibald, so the source information will be the same.

I am not surprised that there could have been some confusion in unclassified secondary sources on the design standard of the R.530 IR seeker at different stages of its development.

In the UK, the research into different IR detectors at RRE (PbS, PbTe and InSb) overlapped the development of successive IR homing heads for Blue Jay Mark 1 (uncooled PbS to cooled PbS), Mark 2 (cooled PbTe), Mark 3 (cooled PbTe) and Mark 4 (cooled PbTe to cooled InSb); Mark 1 became Firestreak, Marks 2 and 3 were cancelled, and Mark 4 eventually became Red Top. As most of the work was classified as Secret, a statement of a particular design standard that was correct at a point in time could subsequently change, but secondary sources could remain uncorrected. This was certainly true for Red Top which was initially intended to have a cooled PbTe detector, which became the standard recorded in most secondary sources for many years, but the actual design standard had moved on to InSb during Red Top development and InSb was always the production standard. It would be interesting to know if something similar happened on the R.530.
 
@JEngO-23 There’s also an excellent website on the SAT company’s history and products, with articles written by engineers who worked there.

Some of these articles have been compiled in a book « A half century of infrared optronics in France », but the website also has a lot of unpublished content and technical details which your browser can translate to English.

https://www.satsouvenir.fr/index.php?p=4-3&contrib=91
 
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Posting here some relevant paragraphs from the SAT website (link above).

An interesting anecdote is that in 1940 SAT’s founder Jean Turck was part of the team that created the world’s first guided air launched weapon, a radio controlled glide torpedo, 20 of which were delivered before the fall of France.

He used this experience to help the allies come up with countermeasures to jam German Fritz glide bombs in 1943. After the war, while working on the first Franco-German antitank missiles, he found himself on the very same team with the German engineers who had designed the Fritz glide bombs that he had been jamming!

The first missile guidance systems
As early as 1948-1949, the Jean Turck company had been contacted by Matra to participate in a study of the guidance system for two surface-to-air interceptors. This project was not pursued because, in the meantime, France had decided to acquire American Hawk anti-aircraft missiles.

But at Matra, Yves Hebel was beginning the study of air-to-air missiles and asked the Jean Turck company to design an infrared seeker. Thus began a long collaboration with Matra under the auspices of the STAé (French Aeronautical Technical Service).

The first seekers operating in the 2µm band, such as those on the American Sidewinder missiles used during the Korean War, underwent flight testing. It quickly became apparent that this band was unsuitable because it was too disturbed by sunlight for an air-to-air missile (unlike surface-to-surface missiles). A change of wavelength was necessary, requiring a complete overhaul of the basic cryogenic technology, interference filters, optical materials, and the original detectors. Fortunately, the advent of binary semiconductor alloys made it possible to create the first InSb photodiodes operating in the 3-5µm infrared range.

The design of the infrared seeker for the R530 air-to-air missile was a major technical adventure for both manufacturers and State Technical Services, as it began without all the basic technologies being available: neither qualified detectors in the 3-5µm infrared, nor transparent materials for the window and optical system, nor operational means of cooling at 77 °K.

Therefore, to carry out the development requiring significant research potential and consequently substantial self-financing, Jean Turck was forced to approach the SAT. In 1957, these establishments were integrated into the SAT, thus increasing their research and development potential in infrared activities.

The success of the R530, the world's first infrared-guided air-to-air missile in the 3-5 µm band, would lead to the family of equally prestigious air-to-air missiles: the R550 Magic 1, the Magic 2, then the Mica which would equip the Rafale, as well as the Mistral surface-to-air missile.

Detectors
Two categories of detectors can be used in the infrared spectral range: thermal and quantum.

In thermal detectors, we find bolometric and pyroelectric detectors in which the heating caused by infrared radiation modifies the resistance of the detector or the surface electrical charges.

In quantum semiconductor detectors, we find photoconductors (PC) and photovoltaics (PV) for which infrared radiation creates charges that modify electrical conductivity or generate a current. Unlike the previous ones, they derive their sensitivity from operating at very low temperatures (typically 77 °K, or about -200 °C)

The first photon detectors produced by SAT were quantum detectors using evaporated PbS. They enabled the production of the rangefinders for the MILAN, HOT, and ROLAND programs, as well as those for the MINILIR and K 400 turrets. The same detectors are now used in prototypes of guided projectiles and other smart munitions, as well as on the PHOBOS space probe.


To go further in wavelength, it was necessary to change the material and, after tests on PbSe and PbTe, the InSb route became established as early as 1950. With the development of a special MESA technology came the first single-element InSb photovoltaic detectors, perfectly suited for generating programs for the AD530 and MAGIC I seekers and the Super Cyclope single-line analyzer.

Then, in the late 1960s, the first arrays were developed for the VAMPIR, PIRANA, and DDM search and tracking equipment. The second generation soon followed, and from 1979 onward, the planar InSb detector appeared, used in MAGIC II, Mistral, DDM, VAMPIR, PIRANA, and several space applications.

To extend photon detection to longer wavelengths, other materials were needed. Studies conducted at the CNRS as early as 1958 suggested the possibility of detecting a ternary compound based on HgTe and CdTe. The first HgCdTe photodiodes (*) obtained by Christian Vérié attracted the attention of the SAT, which found the ideal material for manufacturing detectors for 10.6-micron laser applications.

Following extensive research conducted in collaboration with the CNRS (French National Centre for Scientific Research), and numerous trials to refine the metallurgy, HgCdTe wafers are now widely used in SAT production.
 

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@H_K I spotted an error in he article you quoted concerning the Sidewinder:

The first seekers operating in the 2µm band, such as those on the American Sidewinder missiles used during the Korean War, underwent flight testing.

The Sidewinder never saw combat use during the Korean War as it was far from with it still flight-testing when the Korean armistice was signed in 1953. The sidewinder's initial IOC was in 1956 with the rather limited AIM-9A followed by a definitive IOC in 1958 with the AIM-9B (It first saw combat use in the 1958 Taiwan strait crisis when Taiwanese F-86Fs wired to carry to AIM-9Bs each shot down a number of PLA:AF MiG-17s).
 
So the AAMs with early InSb detectors were not sensitive enough for head-on engagements.

Its not a clear win over PbS in this era. PbS gives superior range for rear aspect engagement high temperature targets. InSb seeker is always less sensitive by comparison, but less affected by sun and with greater range of angles to engage the target.

Magic I is similar to Red Top and R530 while Magic II is more like AIM-9L.Seems the key change was the move from single element detector to array.
 
So perhaps equivalent to the AIM-9H in terms of seeker performance?
The PbS detector in AIM-9D/G was cooled to around 77K. Firestreak also had a similar cooled PbS detector. My understanding is that the AIM-9H introduced solid state electronics, improving the reliability of Sidewinder, but did not change the IR detector.

Comparing sensitivity of IR detectors is complex, but an indication of relative sensitivity is given in Figure 7.5 of Richard D Hudson's book "Infrared Systems Engineering", attached below. As indicated by PaulMM in Post # 16, a photoconductive (PC) InSb detector at 77K has lower peak sensitivity than PbS cooled to the same temperature. However, the InSb cut-off wavelength is significantly longer at around 5.9µ as opposed to the lower cut-off at around 3.8µ for the cooled PbS. This gives a detection performance advantage over AIM-9D/G/H to the longer wavelength InSb detector, such as in Red Top, R.530 and Magic 1, once the angle-off-tail increases beyond the point where the shorter wavelength emissions of the hot-jet-pipe are no longer detectable.

So any detailed performance comparison depends on target signature and angle-off-tail of the engagement, as well as several very specific IR detector characteristics which may not be generally available.
 

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My understanding is that the AIM-9H introduced solid state electronics, improving the reliability of Sidewinder, but did not change the IR detector.

Yes, the AIM-9H introduced both transistor circuitry along first-generation op-amp ICs (I suspect that the Fairchild μA709 op-amp IC was used, it was the precursor to the groundbreaking μA741 which is still in production) and this probably enabled it ho have basic IRCCM.
 
Yes, the AIM-9H introduced both transistor circuitry along first-generation op-amp ICs (I suspect that the Fairchild μA709 op-amp IC was used, it was the precursor to the groundbreaking μA741 which is still in production) and this probably enabled it ho have basic IRCCM.
Your mention of the Fairchild μA709 op-amp IC prompted me to pull a text-book of the shelf from my course at Edinburgh University in 1968-72, "Discrete and Integrated Semiconductor Circuitry" by L.J. Herbst, published in 1969. Sure enough, the chapter on Integrated Circuit Amplifiers starts, "One of the earliest and best known operational amplifiers is the μA702 monolithic IC element originated by Fairchild and now made by many manufacturers." The chapter describes both the μA702 and the developments incorporated in the μA709 amplifier. There was a major revision to the Electronics and Electrical Engineering course that started at Edinburgh in 1968; it was the first year the university stopped teaching about valves and focused instead on solid state electronics.
 
So I suppose that the groundbreaking Fairchild μA741 (Still in production by many different semiconductor manufacturers) appeared around 1972?
 
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