H2S was the first airborne, ground scanning radar system. It was developed for the Royal Air Force's Bomber Command during World War II to identify targets on the ground for night and all-weather bombing. This allowed attacks outside the range of the various radio navigation aids like Gee or Oboe, which were limited to about 350 kilometres (220 mi). It was also widely used as a general navigation system, allowing landmarks to be identified at long range.
In March 1941, experiments with an early Airborne Interception radar based on the 9.1 cm S band cavity magnetron revealed that different objects have very different radar signatures; water, open land and built-up areas of cities and towns all produced distinct returns. In January 1942, a new team was set up to combine the magnetron with a new scanning antenna and plan-position indicator display. The prototype's first use in April confirmed that a map of the area below the aircraft could be produced using radar. The first systems went into service in early 1943 as the H2S Mk. I (and ASV VIB) and H2S Mk. II.
On its second operational mission on 2/3 February 1943, an H2S was captured almost intact by German forces, and a second unit a week later. Combined with intelligence gathered from the surviving crew, they learned it was a mapping system and were able to determine its method of operation. When they pieced one together from parts and saw the display of Berlin, near panic broke out in the Luftwaffe. This led to the introduction of the FuG 350 Naxos radar detector in late 1943, which enabled Luftwaffe night fighters to home on the transmissions of H2S. The British learned of Naxos and a great debate ensued over the use of H2S. However, calculations showed that losses during this period were actually less than before.
After it was found the resolution of the early sets was too low to be useful over large cities like Berlin, in 1943 work started on a version operating in the X band at 3 cm (10 GHz). A wide variety of these H2S Mk. III versions were produced before the Mk. IIIG was selected as the late-war standard. Development continued through the late-war Mk. IV to the 1950s era Mk. IX that equipped the V bomber fleet and the English Electric Canberra. In the V-force, Mk. IXA was tied into both the bombsight and navigation system to provide a complete long-range Navigation and Bombing System (NBS). In this form, H2S was last used in anger during the Falklands War in 1982 on the Avro Vulcan. Some H2S Mk. IX units remained in service on the Handley Page Victor aircraft until 1993, providing fifty years of service.
Etymology of "H2S"Edit
The targeting radar was originally designated "BN" (Blind Navigation), but it quickly became "H2S". The genesis of this designation remains somewhat contentious, with different sources claiming it meant "Height to Slope"; or "Home Sweet Home". The "S" was already being used by the Airborne interception radar team as a deliberately confusing acronym for its operating wavelength in the "sentimetric [sic]" range, which ultimately gave name to the S band.[a]
It is also widely reported that it was named after hydrogen sulphide (chemical formula H2S, in connection with its rotten smell), because the inventor realised that had he simply pointed the radar downward instead of towards the sky, he would have a new use for radar, ground tracking instead of for identifying air targets and that it was simply "rotten" that he hadn't thought of it sooner.
The "rotten" connection, with a twist, is propounded by R.V. Jones, who relates the tale that, due to a misunderstanding between the original developers and Lord Cherwell, development of the technology was delayed, the engineers thinking that Lord Cherwell wasn't keen on the idea. Later, when Cherwell asked how the project was progressing, he was most upset to hear that it had been put on hold, and repeatedly declared about the delay that "it stinks". The engineers therefore christened the restarted project "H2S" and later, when Cherwell inquired as to what H2S stood for, no one dared tell Cherwell that it was named after his phrase—instead they pretended, on the spot, that it meant "Home Sweet Home"—which was the meaning that Cherwell related to others (including R.V. Jones).
After the Battle of Britain, RAF Bomber Command began night attacks against German cities. Although Bomber Command had reported good results from the raids, the Butt Report showed only one bomb in ten hit the target, half the bombs fell on open country and in some cases the bombing was seen to fall as far as 50 kilometres (31 mi) from the target.
Radio electronics promised some improvement. The British developed a radio navigation system called "Gee" and then a second known as "Oboe". Both were based on transmitter stations in the UK which sent out synchronized signals. In the case of Gee, an oscilloscope in the aircraft measured the time difference between two signals to determine location. Oboe used a transponder in the aircraft to reflect the signals back to the UK where operators carried out the same measurements on much larger displays to produce more accurate values. In both cases, the ground-based portion of the system limited range to a line-of-sight, about 350 kilometres (220 mi) for aircraft flying at typical mission altitudes. This was useful against targets in the Ruhr, but not the heart of Germany.
Taffy Bowen had noticed during his early Airborne Interception radar (AI) experiments before the war that the radar returns from fields, cities and other areas were different. This was due to geometry; objects with vertical sides like buildings or ships produced much stronger returns than flat objects like the ground or sea. During early tests of the AI system, the operator would often see coastlines at very long distances, and the development team used this as an ad hoc navigation system on several occasions. Bowen had suggested development of targeting radar based on this principle, but the matter had been forgotten.
The idea resurfaced in March 1941 when Philip Dee's group was developing a microwave frequency AI radar, christened "AIS" in reference to its "sentimetric" wavelength. During tests in a Blenheim, the team noticed the same sort of effects Bowen had earlier. However, the set's wavelength, over ten times shorter than the original 1.5 m AI sets, provided much greater resolution.
In October 1941, Dee attended a meeting of the RAF Bomber Command where the night targeting issue was discussed. Dee mentioned the recent discoveries using AIS. On 1 November, Dee performed an experiment in which he used an AIS radar mounted on a Blenheim to scan the ground. Using this display he was able to pick up the outline of a town 35 miles (56 km) away while flying at 8,000 feet (2,400 m) altitude.
The commanders were impressed and, on 1 January 1942, the Telecommunications Research Establishment (TRE) set up a team under Bernard Lovell to develop an S-band airborne targeting radar based on AIS. An initial order for 1,500 sets was placed. It was clear even at this point that a Plan Position Indicator (PPI) display would be desirable, but this would require a complex scanning parabolic antenna, compared to the very simple set of fixed antennas used in the A-scope system. It was decided to test both systems. In March, it was decided that both H2S and a new centimetric Air-Surface-Vessel radar (ASV) radar, ASV Mk. III, would be built using the same components, simplifying production.
In early tests in April, the superiority of the scanning PPI system was evident, and all work on the older A-scope version ended. H2S performed its first experimental flight on 23 April 1942, with the radar mounted in a Halifax bomber, V9977. The scanning unit was installed in the aircraft's belly using the position previously occupied by the mid-under turret, which was by that time seldom installed. The rotating scanner mounting was designed and manufactured by Nash & Thompson. The scanning aerial was covered by a distinctive streamlined radome.
One problem was that the returns from closer objects were much stronger than more distant objects, due to the radar equation. This made the area directly under the bomber much brighter than the surroundings if the signal was not adjusted to account for this. The solution was to adjust the broadcast power according to the cosecant-squared rule, so called after the mathematical function that defined the effective change in gain. The change was originally produced by fixing an angled metal plate on part of the parabolic reflector of the aerial, as may be seen in the picture of the aerial on a Halifax bomber. Later reflectors were actually shaped with a cosecant-squared curvature, no longer a perfect parabolic section.
Then disaster occurred; on 7 June 1942, the Halifax performing H2S tests crashed, killing everyone on board and destroying the prototype H2S. One of the dead was Alan Blumlein, and his loss was a huge blow to the programme. Also killed in the crash were Blumlein's colleagues Cecil Oswald Browne and Frank Blythen; a TRE scientist Geoffrey S. Hensby, and seven RAF personnel.
As development continued, a great debate broke out in the Air Ministry and RAF about the relative merits of the H2S system. While the ability to bomb in all weather at great distances was obviously useful to Bomber Command, the loss of an H2S aircraft would potentially reveal the secret of the magnetron to the Germans. Churchill's science advisor, Frederick Lindemann, wanted the design team to build H2S around the klystron rather than the magnetron.
Unlike a klystron, which is made mostly of glass and fragile metal parts, the magnetron was built out of a single block of copper that would be extremely difficult to destroy with any reasonable demolition charge. If a magnetron was recovered by the Germans, they would immediately understand its operation and potentially develop countermeasures. Since the magnetron was also being designed for use in night fighters and Coastal Command, the loss of the secret would not only provide the Germans with ample early warning to build detectors, but also allow them to develop their own effective airborne radars.
The H2S design team did not believe the klystron could do the job, and tests of an H2S built with klystrons showed a drop in output power by a factor of 20 to 30. At the same altitude, the klystron powered versions were able to detect a town at 10 miles (16 km) while the magnetron version was capable of 35 miles (56 km). There appeared to be no way to improve this, so it would have to be the magnetron, or nothing. The H2S team also protested that it would take the Germans two years to develop a centimetric radar once the cavity magnetron fell into their hands, and that there was no reason to believe they weren't working on the technology already. The first concern would prove correct; the second would be proven wrong.
In the midst of the debate, Isidor Isaac Rabi of the American Radiation Laboratory visited the TRE offices on 5 and 6 July 1942. He stated that the H2S device provided to them during the Tizard Mission was "unscientific and unworkable" and expressed his feelings that the only use of it would be to hand the magnetron to the Germans. The US was, at this time, deep into the development of an ASV set using a magnetron, so work on H2S continued as there appeared to be no reason to continue their own ASV when the US would soon provide one. Years later, Lovell attempted to discover the reasons for this negative report, but he found that no one recalled Rabi being so negative. The only explanation that anyone had was that problems getting the sets working were taken out of context. Taffy Bowen had noted that he had significant trouble getting the sets to do anything in the US; in testing against Springfield, Hartford and Boston, the display simply didn't show anything.
By September, a prototype version suitable for operational use was ready. In spite of all the concerns, on 15 September Churchill personally released the magnetron for use by Bomber Command. While the debate raged, it had been noticed that German submarines had been fitted with a new radar detector, later known to be the FuMB 1 Metox 600A, which allowed them to detect Coastal Command's ASV sets operating on the older 1.5 m band. In September the decision was made to prioritize construction for the ASV Mk. III. It was felt the chance that a magnetron falling into German hands from a patrol aircraft was vanishingly small.
The Air Ministry radar groups had originally formed up at Bawdsey Manor on the eastern coast of England. When the war began in 1939, this location was considered too exposed to potential German attack, and a pre-arranged move to the University of Dundee was carried out almost overnight. On arrival it was found nothing was prepared and there was little room for the teams to work in. Worse, the team working on airborne radars ended up at a tiny private airstrip in Perth, Scotland that was entirely unsuitable for development.
It took some time before the nature of the problem was finally accepted by management and a search began for a new location. The Airborne team moved to RAF St Athan, about 15 miles (24 km) from Cardiff. Although this location should have been ideal, they found themselves in a disused hangar with no heating, and work became almost impossible as the weather turned cold. The main research teams remained in Dundee during this period.
Meanwhile, the ongoing search for a more suitable location for all the teams led to the selection of Swanage on the southern coast of the UK. In retrospect, this decision seems particularly odd given that it was even more exposed to the enemy than their original location at Bawdsey Manor. The AI group, located in shacks located on the shoreline near Worth Matravers, was particularly exposed and only a short distance from Cherbourg. While the move was taking place, A.P. Rowe took the opportunity to set up a second airborne group working with magnetrons, sidelining Bowen's group in St Athan. Bowen was soon forced out of the TRE and sent on the Tizard Mission that summer.
On 25 May 1942, commandos carried out Operation Biting to capture a Würzburg radar that had been photographed near the French coast. This led to concerns that the Germans might repay the favour in kind. When reports were received that a company of paratroopers had been stationed near Cherbourg, directly across the English Channel from Christchurch, near panic broke out in the Air Ministry and yet another emergency move was made. The team ended up at Malvern College about 160 kilometers (99 mi) to the north. This provided ample office space but little in the way of housing, and introduced yet more delays in the development program.
Despite all the problems, on 3 July 1942 Churchill held a meeting with his military commanders and the H2S group, where he surprised the radar designers by demanding the delivery of 200 H2S sets by 15 October 1942. The H2S design team was under great pressure, but they were given priority on resources. The pressure also gave them an excellent argument to convince Lord Cherwell that the klystron-based H2S program be finally dropped.
TRE failed to meet the 15 October deadline; by 1 January 1943, only twelve Stirling and twelve Halifax bombers had been fitted with H2S. On the night of 30 January 1943, thirteen Stirlings and Halifaxs of the "Pathfinder" force used H2S to drop incendiaries or flares on a target in Hamburg. One hundred Lancasters following the Pathfinders used the flares as the target for their bombsights. Seven of the Pathfinders had to turn back, but six marked the target, and the results were considered "satisfactory". Similar raids were carried out against Turin the next night, and Cologne on the night of 2/3 February.
On 21 February, the decision was made to equip all Bomber Command aircraft with H2S, not only as a bombing aid, but a navigation aid as well. In early operations, H2S had proved able to detect coastlines at such a great distance that it could be used as a long-range navigation system, allowing the aircraft to fly in all weather. To aid the navigator, the bomb aimer had the task of operating the H2S during these periods. To further improve operations, on 12 March it was decided that Bomber Command would receive more of the available spares, as it was believed that they would need to make up for higher casualty rates. Previously every equipped squadron was required to hold 100% spares for all parts, and there simply weren't enough to go around.
H2S Mk. II, production versionEdit
The original H2S sets were essentially prototype units that were hand-built to equip the Pathfinder Force with all possible speed. Among the many problems with the rushed service entry was that the developers were forced to use existing plug-and-socket designs to connect the various units of the complete set together. There were no bulkhead mounting male connectors available at this time, and consequently many of the male free connectors at the ends of cable runs carried exposed lethal voltages. While installations of the prototypes progressed, work was underway on a true production version, the Mk. II, which would go on to be the most numerous version built. This was largely identical to the Mk. I's with the exception of various packaging and electronics details intended to make them easier to build.
Bomber Command didn't use H2S generally until summer 1943. On the night of 24 July, the RAF began Operation Gomorrah, a large attack on Hamburg. By that time, H2S had been fitted to Lancasters, which became a backbone of Bomber Command. With the target marked by Pathfinders using H2S, RAF bombers hit the city with high explosive and incendiary bombs. They returned on 25 and 27 July, with the USAAF performing two daylight attacks in between the three RAF raids. Large parts of the city were burned to the ground by a cyclone of fire. About 45,000 people, mostly civilians, were killed.
The Mk. II was soon upgraded to the Mk. IIA versions, which differed from the Mk. II only in the detail of the scanner antenna; IIA replaced the original dipole antenna at the scanner's focal point with a feed horn that sent the signal back to the receiver in a waveguide, eliminating the lossy coaxial cable of the earlier model.
It was noted on even the earliest flights of V9977 that a number of basic features of the H2S made it difficult to use. Attempts to fix these began even before H2S entered service, but a number of problems greatly delayed their entry. Added as they became available, this produced a profusion of different Marks, detailed below.
Late in April 1942, during a test flight of V9977, the prototype unit was shown to Flight Lieutenant E. Dickie, a navigator. Dickie pointed out that navigational charts were always produced with north at the top, while the PPI display of H2S had the top of the display representing whatever direction the aircraft was flying. He suggested that this would cause significant problems during navigation. This had not been considered before because H2S had been developed as a bombing aid. Now that it was also used as an important navigation aid, this was a major issue. This led to a crash program at EMI to modify the prototype sets with a system to correct for this problem. This was solved with the introduction of a selsyn connected to the aircraft's gyrocompass, whose output modified the scan rotation. A further addition produced a bright line on the display indicating the direction of travel.
A later modification allowed the heading indicator display to be manually controlled by the operator. This was used in concert with the Mark XIV bomb sight to accurately correct for any wind blowing the aircraft off the bomb line. The indicator was set to an initial angle provided by the bomb aimer, and from then the navigator could see any residual drift on his display and call out corrections to the pilot, and to the bomb aimer who would update his settings in the bombsight. This basic idea was later expanded to allow the navigator's measurements to be automatically sent back to the bombsight, meaning the bomb aimer no longer had to do this during the approach. Since the other settings, like altitude and airspeed, were already automatically fed in from the aircraft instruments, this left only the selection of the elevation of the target over sea level to be set manually, which could be done before the mission.
The other problem was that when the aircraft rolled, the signal hit the ground only on the lower side of the aircraft, filling one side of the display with a solid signal while the other side was blank. This was particularly annoying because it was during the last minute of the approach to the target that the navigator would be giving course corrections to the pilot, rendering the display unusable every time the pilot responded. This problem was solved through the introduction of a mechanical stabilizer that kept the scanning system level with respect to the ground. A preliminary version was ready by September 1943, but several problems were noted, and it was not until 5 November that the decision was made to move it into production. By this time development of the 3 cm version of H2S was underway, and Nash & Thompson promised to have versions of the stabilizer for both 10 and 3 cm units available by 15 December 1943.
A final problem related to the geometry of the signals returned by the radar. As the scanning angle increased, the time taken for the signal to return did not increase linearly, but hyperbolically. As a result, returns close to the aircraft were fairly similar to what would be seen on a map, but those further from the aircraft were increasingly compressed in range. At the shortest range setting, 10 miles (16 km), this was not a serious problem, but at the longest, 100 miles (160 km), this made the display very difficult to understand. This led F. C. Williams to develop a new time base generator that also output a hyperbolic signal, fixing this problem. This was called the "scan corrected indicator", or display Type 184.
All of these concepts were being worked on largely in parallel, and at a meeting in March 1944, it was learned that only low rates of production could be expected through the end of the year. By that time the new 3 cm sets were being introduced as well, and this led to a profusion of various Marks featuring one or more of these additional corrections. These delays had not been expected, and Lovell later noted:
|“||We were aghast at these delayed dates, but worse was to follow in the months ahead - we had overloaded the firms, people's brains and probably ourselves. The delays were appalling - it seemed that the whole country had stopped working... Matters steadily got worse and worse.||”|
Radar operates by sending out very short pulses of a radio signal from a transmitter, then turning the transmitter off and listening for echoes in a receiver. The output of the receiver is sent to an oscilloscope's brightness input, so strong echoes cause a spot on the screen to light up. To make the spots correspond to locations in space, the oscilloscope quickly scans from the centre to the outside of the display; echoes that return later in time are produced further out on the display, indicating further distance from the aircraft. The times are synchronized by using the transmission pulse to trigger the scan.
In the case of H2S, the echoes are returned from the ground and objects on it. That means the very first signal that would normally be received would be from the ground directly beneath the aircraft, as this is the closest to the aircraft. Since the echo from this location took some time to return to the aircraft, the time needed to travel to the ground and back at the aircraft's current altitude, the H2S display naturally had an empty area around the centre of the display, with its radius representing the altitude of the aircraft. This was known as the centre-zero. Normally the operator used a dial that delayed the start of the sweep in order to reduce the size of this centre-zero, and thereby increase the amount of the screen used for the ground display.
Operators noticed that sometimes fleeting echoes were visible within this circle, and quickly concluded these were from other aircraft. This presented a simple way to see enemy night fighters as long as they were below the bomber and not far enough away that they would be hidden in the ground return. German night fighters normally approached from below as it helped silhouette the target aircraft against the Moon, and the lack of a gun position in that location made it safe to approach from that direction. This left them ideally positioned for detection by H2S. However, the display was very small, and this blank area on the screen only a small portion of that, so seeing these returns was difficult even if the centre-zero had not been dialled out entirely.
In early 1943 German night fighter operations were improving. Between January and April 1943 Bomber Command lost a total of 584 aircraft to the defences. Although this represented only 4% of the sorties, this was nevertheless worrying because the increasing daylight length during the summer meant that the defences would inevitably be more effective. Several systems were already under development to help the bombers defend themselves, including the Monica radar (a simple adaptation of the original AI Mk. IV radar from the RAF's own night fighters) and the Automatic Gun-Laying Turret (AGLT), which was intended to automate defensive fire. However, the former proved almost useless in practice, and it was already clear the latter would not be available at least until 1944.
Dudley Saward visited the Malvern site on 18 April to view progress on the microwave radars and mentioned the problem to Lovell. He was particularly frustrated by a raid carried out the night before on 16/17 April on the Škoda works, where 11.3% of the attacking force was lost due to enemy action and all other issues. Mentioning the problems with the Monica and especially the AGLT, Saward told Lovell:
|“||What on earth are we going to do for a stop-gap? [Then I added that...] H2S gave us a good picture of the ground below us, and it was a pity it couldn't give us a good picture of the aeroplanes around us.||”|
Lovell was aware that this was indeed possible. The team promised they could build a sample of a special display that would increase the size of the centre-zero until it filled the display, thus making the returns from other aircraft easier to see. They only asked that the "whole affair was to be kept quiet to avoid difficulties".
Seward supplied an electronics technician, Sgt. Walker, and two mechanics, all of whom arrived the next day and immediately set about building a display in Halifax BB360. The basic idea was to use the delay timer that reduced the size of the centre-zero as a switch; the existing display would receive returns exactly as it had before, with everything before that timer being suppressed, while a new display would receive everything before that time, and could be adjusted so the centre-zero filled the display. This would result in one display showing everything in the air, and a second providing a ground map exactly as before. The first experimental system flew on 27 May with a Mosquito providing a target. The Mosquito clearly appeared on the display, and photographs of the display caused much excitement.
When the photos reached the desk of Robert Saundby, he immediately sent a message to the Air Ministry demanding that they be installed with all possible speed. The new display, given the official title Type 182 and nicknamed "Mousetrap", was on the assembly line by August 1943. At this point, the team received a message demanding they immediately stop using the name Mousetrap as that was the name of an upcoming secret mission.[b] They were officially allocated the new name "Fishpond", a choice that was made official by a telegram from Churchill on 9 July. The first operational units went into service in October 1943, and by the spring of 1944 most of Bomber Command's aircraft carried it. Two hundred of the prototype model were produced before a slightly modified version was introduced, the Type 182A. This version had the range fixed at 26,000 feet (7,900 m), with the side-effect that if the aircraft flew below this altitude the ground appeared as a ring of noise on the display.
The Type 182 display was normally located at the radio operator's station, not the navigator's. This reduced the navigator's workload while also simplifying communications when a target was seen; the radio operator could easily communicate with the crew or send messages to other aircraft. Normally a number of blips would be seen, as other aircraft in the bomber stream made excellent returns. However, these remained largely stationary on the display as they were all flying roughly the same path, so enemy fighters were easy to see as dots moving around within the pattern of returns. If it was suspected a blip was approaching the bomber, the bomber would change heading and see if the blip followed; if it did, immediate defensive manoeuvring started.
The resolution of any radar is a function of the wavelength used and the size of the antenna. In the case of H2S, the antenna size was a function of the bomber's turret opening, and when combined with the 10 cm wavelength, this led to a resolution of 8 degrees in arc. This was much coarser than desired, both for mapping purposes and for Coastal Command's desires to easily detect submarine conning towers. On 6 February 1943, work began on an X band version of the electronics, operating at 3 cm. This would improve resolution to 3 degrees when used with the same antenna. When priority was given to Bomber Command, Coastal Command responded by producing specifications for a far more advanced ASV system operating at 1.25 cm, but this was not completed by the end of the war.
Work on 3 cm magnetrons had been ongoing for some time, and an AIS unit with such a device had been fitted to the nose of RAF Defford's Boeing 247-D, DZ203 as early as 1942. This aircraft had originally been supplied by the Canadian Defense Research Board to test US models of AI radar, and since then had been widely used in the development of several versions of AI, ASV and H2S. George Beeching had been assigned the task of fitting H2S to the Stirling, and in early 1943 he managed to obtain a single 3 cm magnetron from Herbert Skinner's AI group working on the Boeing. He had it working in the H2S electronics in a bench top set on 7 March 1943, and then quickly fit it to Stirling N3724 to make its first flight on 11 March. Testing showed the unit had very short range, and could not be used effectively over 10,000 feet (3,000 m) altitude. Further work was delayed by the need to fit the existing 10 cm sets to operational aircraft.
Bomber Command began a series of large-scale raids on Berlin on the nights of 23/24 August, 31 August/1 September and 3/4 September 1943. H2S was found to be largely useless on these missions; the city was so large that picking out features proved very difficult. On 5 September, Saward, in charge of Bomber Command's radar efforts, visited the H2S team and showed them photographs of the PPI displays from H2S over Berlin. On the 10 miles (16 km) range setting, used during the bomb run, returns covered the entire display and there were no clear outlines of large objects on which to navigate. This was a surprise given the excellent results over Hamburg. After much argument among teams within the TRE on how to address this problem, on 14 September the team began working on an official version of H2S working in the X band.
By this time the US Radiation Laboratory was also entering the fray. They had decided to move directly to using a 10 GHz frequency, 3 cm wavelength design, calling their unit H2X. By June there was an ongoing debate in the UK whether to continue development of their own 3 cm H2S sets or simply use the American units when they became available. The suggestion was made that the existing H2S Mk. II units should be converted to X band, and the Americans should work on 3 cm ASV instead. This was followed by a 7 June meeting in which TRE management decided to press for three squadrons of 3 cm H2S by the end of the year. Lovell's team considered this to be basically impossible. Instead, they hatched a private plan to build and install a total of six sets which would equip Pathfinder Force Lancasters by the end of October.
Work continued on what was now known as H2S Mk. III, and an experimental set was first used over Berlin on the night of 18/19 November 1943. In comparison to the first mission with the Mk. I sets, the results using Mk. III were described as "most outstanding". Mk. III was rushed into production and saw its first real operational use on 2 December.
From this point until the end of the war, the Mk. III became the backbone of the Bomber Command fleet, and a large variety of versions were introduced. The first modification was the out-of-sequence Mk. IIIB, which added the range corrected Type 184 display unit from the IIC models, but lacked roll stabilization. Stabilization was added in the next version to see service, the Mk. IIIA. The new 6-foot (1.8 m) "whirligig" scanner was added to the Mk. IIIA to produce Mk. IIIC, while the original scanner with a higher power magnetron produced the Mk. IIID. The Type 216 display, using magnetic deflection, which was much easier to mass-produce, was added to the original IIIA to produce the Mk. IIIE, while the whirligig was added to the same unit to make the Mk. IIIF.
By the middle of 1944, the war in Europe was clearly entering its final stages, and the RAF began making plans to begin attacks on Japan with the Tiger Force group. In order to equip these aircraft, which would need both targeting and long-range navigation, a conversion system for the earlier Mk. II units was introduced. Based on non-stabilized IIC units, the Mk. IIIG used a new magnetron and receiver for 3 cm operation like the other Mk. III systems. The primary goal was to use it for long-range navigation, as opposed to bomb aiming. The final Mk. IIIH was IIIG with the Type 216 display.
Before H2S was deployed in 1943, there was an intense debate over whether to use it due to the possibility of it being lost to the Germans. As it turned out, this occurred almost immediately. On its second combat mission, during the raid on Cologne on the night of 2/3 February 1943, shortly after crossing the coast one of the Stirlings carrying H2S was shot down near Rotterdam. The device immediately attracted the attention of Wolfgang Martini's technicians, who managed to salvage everything except for the PPI display.
Giving it the name Rotterdam Gerät (Rotterdam apparatus), a group formed to exploit the device and met for the first time on 23 February 1943 at Telefunken's offices in Berlin.[c] A second example, also with a destroyed PPI, was captured on 1 March, ironically from a bomber that was part of a group attacking and greatly damaging Telefunken's offices, destroying the first example in the process.
Interrogation of surviving members of the second crew revealed that:
|“||The sets which have fallen into our hands have so far lacked their display unit... but the interrogation of the prisoners has revealed that the device is certainly used to find targets, inasmuch as it scans the territory over which it flies...||”|
Combined with their own display, a set was reassembled on the Humboldthain flak tower in Berlin. When it was activated clear images of the city appeared on the display, causing considerable consternation for Hermann Göring. A quickly adopted countermeasure was put in place by installing small corner reflectors around the city, producing bright spots on the display in areas that would otherwise be empty, like lakes and rivers. Producing the reflectors with the required angular accuracy proved to be a difficult problem, as did keeping them in the right positions in order to produce the right image.
Although the basic concept of the magnetron was immediately understood, a number of details of the system as a whole remained a mystery, and it was also realised that building a complete radar system using it would take some time. So for the short term, they gave "panic priority" to a ground-based jammer and a detector that would allow their night fighters to home in on the microwave signals. This development was slowed by the German electronic industry's decision to stop researching microwaves shortly before Rotterdam Gerät literally fell from the sky. Another serious problem was a lack of suitable crystal detectors that were key to the British receiver designs.
Several jammer systems were trialled. The first, known as Roderich, was developed by Siemens. These used a transmitter mounted on a tower pointed at the ground, the reflections off the ground spreading the signal out in space where they were picked up by the H2S receivers. Roderich transmissions were timed roughly with the scanning speed of the H2S antenna, causing a pattern to appear similar to a pinwheel that made it difficult to see the ground between its pulses. However, their magnetron was only capable of 5 W of power, giving it very short range. They were so ineffective that they were abandoned in 1944. Another system, Roland, used a 50 W klystron, but it was also considered unsuccessful and abandoned around March 1945. Another klystron-based system, Postklystron, was designed by the Reichspost and deployed around Leuna.
Two detector systems were ordered: a simple passive system that was essentially just a high-frequency receiver, which became Naxos, and a much more sensitive system using its own magnetron as a local oscillator known as Korfu. Both required crystal detectors in their receivers, and a crash program to develop them began. These began delivery in a few months, but proved difficult to mass-produce and extremely fragile in the field. This limited the availability of the Funkgerät (FuG) 350 Naxos radar detector to a handful of operational examples, which enabled Luftwaffe night fighters to home on the transmissions of H2S. A U version of the same equipment was used to allow U-boats to detect microwave-frequency ASVs.
The RAF remained unaware of the Naxos until the spring of 1944 when a number of intelligence reports suggested the Germans had developed an H2S detector. By this time, the Germans had only a few dozen such detectors in service, but the reports reopened the longstanding debate between the supporters of H2S and those of UK-based navigation systems like Oboe. This corresponded with a period of increased losses among Bomber Command, and there were calls for the system to be abandoned. The matter was debated for months.
The issue was finally settled by a study by Saward. He noted that losses during the Naxos period were actually lower, down from 4% to 2% of the sorties. The drop corresponded with the introduction of Fishpond. Saward concluded that:
|“||The chief value of Naxos to the Germans may be as a propaganda weapon in an endeavour to stop, or at least limit, our use of H2S.||”|
In July 1944, Ju 88G-1, of 7 Staffel/NJG 2, flew the wrong way on a landing beacon and landed at RAF Woodbridge by accident. The crew were arrested before they could destroy their equipment, providing the British researchers with the latest version of the Lichtenstein SN-2 VHF-band radar, the Flensburg radar detector, and the FuG 25a Erstling IFF gear. Interrogation of the crew revealed that the Flensburg system detected the RAF bombers' Monica tail warning radar emissions, and that it was used as a homing system. Naxos was not fitted, and the crew stated that it was only used for initial warning, not as a homing system.. This was all to the great relief of everyone involved; Monica was already being replaced by Fishpond systems on most aircraft, and any still equipped with Monica was told to turn it off. H2S remained in use for the rest of the war.
As the British engineers had predicted, it took the Germans two years to complete development of magnetron based radars. The first to reach operation in early 1945 was the FuG 240 Berlin, an Airborne Interception radar very similar to the British AI Mk. VIII. By this time the country was already in a shambles, and Berlin never entered service. A small number were fit experimentally, one of which was captured by the RAF in a shot-down Ju 88. Several other units developed from the same basic systems were also introduced but saw limited or no service. One advancement made by the Germans during this period was a new type of antenna using a dielectric to shape the output, known in the UK as a polyrod.
In a separate line of development, the RAF was working on a pair of mechanical computers known as the Air Milage Unit (AMU) and Air Position Indicator (API), which continually performed dead reckoning calculations, greatly reducing navigator workload. This was fed by inputs similar to those for the Mk. XIV bomb sight, namely the estimated wind direction and speed, with the aircraft heading and speed fed in automatically from the aircraft instruments. The system output was a varying voltage that could be used to drive the Mk. XIV bomb sight.
In a development known as Mark IV, H2S was modified to also read these voltages, which offset the center of the display by an amount proportional to the signals. This would counteract the motion of the aircraft, and "freeze" the display. When initially set up these calculations were never perfect, so some residual drift on the display was normally encountered. The navigator could then fine tune these settings with controls on the display, adjusting them until the image was perfectly still. These values then fed back into the AMU and API, producing highly accurate measurements of the winds aloft. The Mk. IVA used the larger whirligig scanner. None were available by the time the war ended.
Further improvements in magnetron and receiver design during the war led to the ability to use even shorter wavelengths, and in the summer of 1943 the decision was made to begin development of versions operating in the K band at 1.25 cm. This would improve the resolution by more than a factor of two over the X band versions, and was especially interesting as a system for low-level bombing where the short local horizon would require guidance on smaller objects like particular buildings.
The corollary of this improved resolution was that a K-band system would offer the same resolution as the X-band system with an antenna half the size. Such an antenna would fit on the Mosquito, and development of a 28 inches (710 mm) scanner began. The Mosquito was already widely used for pinpoint target indicator operations, and fitting them with H2S would further increase their abilities. On 22 February 1944, the development group proposed rapidly fitting Mark IV to all Lancasters, and for higher-accuracy needs, developing either an X-band Whirligig, or a K-band with a smaller antenna. Instead, they were ordered to do both.
The K-band work was given the name "Lion Tamer". The first test of the basic equipment took place on a Vickers Wellington on 8 May 1944, and Lancaster ND823 was equipped with the prototype Mark VI and flew on 25 June. However, a meeting on 16 June noted that the range of the K-band sets was not good, with tests in the US reaching only 10 miles (16 km) from 10,000 feet (3,000 m) altitude. Further, production was not ready for large-scale deliveries, and as Dee put it, "the present programme of 100 H2S Mark VI equipments should be regarded as an expression of faith."
Several new features became part of the Lion Tamer effort. Due to the much higher resolution of the K-band signals, a new display was needed because the dot produced on the older display was too large and overlapped details on either side. This led to the Type 216 display, which was magnetically deflected instead of electrostatic. However, this led to a new problem; in the older displays a bias voltage was sent to the deflection plates to create a rotating signal to produce the PPI, but a new method had to be developed for the Type 216. Modifications for this feature led to another being added, sector scan, which allowed the operator to select one of the eight compass rose points and the display expanded to show only that quarter. Meanwhile, work on the new mechanical computers for air navigation was progressing well. It was decided that the Mark VI should be able to connect to these systems. Eventually, all of these changes were rolled up into the proposed Mark VIII.
During the late summer of 1944, as the post-D-Day operations bogged down, there was renewed interest in using the K-band system to detect tactical targets like tanks. Lancaster JB558 was fit with a 6-foot scanner and a K-band set and began tests at low altitudes between 1,000 and 2,000 feet (300 and 610 m) beginning in December 1944. The results were "immediately staggering", with the displays showing high-quality images of individual buildings, roads, railways and even small streams.
Similar experiments with the smaller 3-foot scanner were not so successful in this role. At a meeting on 16 December, it was decided to move ahead with Lancasters with 6-foot scanners and Mosquitos with 3-foot scanners. This meant the K-band equipment originally planned to be installed on the Pathfinder Force would be used on these aircraft. Pathfinder Force received the Mark IIIF X-band equipment instead.
Ultimately, only the Mosquitoes were ready before the war ended, and carried out a total of three target marking operations for Pathfinder Force. When the war ended and the lend-lease ended with it, the availability of the K-band magnetrons disappeared. Additionally, in high-aititude tests it was noticed that the signal disappeared in clouds, an observation that would later give rise of weather radar systems, but in the meantime made the system less than useful. The Director of Radar in the Air Ministry decided to embargo all work on the K-band systems for security reasons.
Looking to further improve the navigational aspects of the system, some work was carried out on a system known as H2D, the D for "doppler". The idea was that the doppler shift of the signals due to the motion over the ground could be used to determine the ground speed. In still air, the maximum doppler shift would be seen dead ahead, but in the presence of any winds aloft, the sideways component would cause the maximum point to shift to an angle, while the head or tail component would make the measured doppler speed differ from the airspeed indicator. By comparing these measurements to the aircraft's airspeed and heading, the windspeed and direction could be accurately calculated.
Testing began at RAF Defford on Vickers Wellington NB822 in early 1944. It became apparent that the sensitivity of the unit was enough that ground traffic like trucks and trains became visible on the display. This is the first example of what is today known as moving target indication, which would theoretically allow an aircraft to scan for targets across a wide area. A second aircraft, NB823, joined the effort in June 1944, and then a third (unknown ID).
Unfortunately, more rigorous testing demonstrated that the experimental set was only really useful when the aircraft was flying under 3,000 feet (910 m) and had a maximum effective detection range on the order of 3 to 4 miles (4.8–6.4 km). Work to improve these numbers was slow going, and was eventually relegated to the status of purely experimental.
After VE day, all models earlier than the Mk. IIIG were declared obsolete, and ongoing work on many of the newer versions ended. In place of the entire series from Mk. VI to VIII came the Mark IX, which was essentially a version of the 3 cm Mk. VIII designed specifically for use on the E3/45 jet bomber, which after becoming B3/45, would finally emerge as the English Electric Canberra.
In contrast to the earlier designs that were added to existing bombers in an external fairing, for E3/45 the radar was designed as an integral part of the aircraft. It was otherwise an upgrade to the existing Mk. VIII with a 200 kW magnetron and numerous other upgrades. A contract was awarded to EMI in 1946 as the Mark IX, but during development it was amended to equip the much larger B14/46 bomber designs, the V-force. These were essentially identical to the original concept, but used the larger "whirligig" reflector and became the Mk. IXA. Using the larger "whirligig" reflector and a slotted waveguide allowed the angular beamwidth to hit 1.5 degrees, a great improvement over the WWII models.
The Mk. IX allowed the scanning rate to be set at 8, 16 or 32 RPM. Additionally, the IX included the ability to perform a sector scan, limiting the movement of the scanner so instead of performing complete circles it scanned back and forth across a smaller angle. This provided much more rapid updates of the selected area, which was needed in order to account for the much higher speed of the aircraft. This was especially useful on the v-force, where the radar's location in the nose made it difficult to scan to the rear anyway, and at best some 60 to 90 degrees was always blocked.
The system also added the ability to perform offset bombing, a relatively common addition to post-war bombing systems. It was found during operations that the target itself might not appear on the radar. In these cases, the navigator would select a nearby feature that would visible on the radar, a bend in a river or a radio tower for instance, and measure the angle and distance between it and the target. They would then attempt to guide the aircraft so that the selected aiming feature was in the proper location relative to the center of the display, by no means a simple task. Offset bombing allowed the navigator to dial these offsets into the display, which caused the entire display to move by that amount. The navigator then guided the aircraft so that the selected feature passed through the center of the display, which was much easier to arrange.
During this period, the API was replaced by the more advanced Navigation and Bombing Computer (NBC), which, when combined with Mk. IX and Green Satin radar, formed the Navigation and Bombing System (NBS). Green Satin made highly accurate and completely automatic measurements of wind speed and direction, allowing the NBC to perform dead reckoning calculations with a very high degree of accuracy. This further automated the navigation process to the point where separate navigators and bomb aimers were no longer needed, and some aircraft were designed with a crew of only two.
Development proceeded at a slower rate due to post-war realities. Flight testing of the smaller Mk. IX began in 1950 on a Avro Lincoln, followed by the Mk. IXA in 1951 on Handley Page Hastings or Avro Ashton aircraft. As this was too late for the Canberra, which entered service in 1951, early models had to be modified with a conventional glass nose for optical bombing. The Mk. IVA remained in service until 1956 when the Mk. IX finally entered service on the V-force.
The first use of NBS in combat was in 1956, when Vickers Valiants performed long-range strikes on the Egyptian Air Force at Cairo Airport. The system remained in service with the V bomber force (Valiant, Avro Vulcan and Handley Page Victor) throughout their lifetime. The last use in combat was made by the Vulcans of the Operation Black Buck flights in 1982, which used the system as the primary navigation and bombing aid throughout the 7,000 miles (11,000 km) round trips to and from Ascension Island.
In 1950 a further requirement for more accurate conventional bombing was raised, demanding 200 yards (180 m) accuracy from an aircraft flying at 50,000 feet (15,000 m) and 500 knots (930 km/h; 580 mph). This led to the early consideration of a version operating in the Q-band at 8 mm wavelength. An experimental version was constructed in 1951, but in practice the Mk. IX proved useful enough on its own and development was dropped.
- Mark I - prototype versions fit to Pathfinder Force (TR3159)
- Mark II - main production version with standard 3 foot (0.91 m) scanner (TR3191)
- Mark IIA - replaced the scanner's dipole antenna with a horn and waveguide
- Mark IIB - IIA with Fishpond displays
- Mark IIC - IIB with Type 184 scan-corrected display, roll stabilized scanner, and improved antenna reflector that eliminated the metal fillet
- Mark III - prototype 3 cm versions, six produced by December 1943
- Mark IIIA - III with Type 184 display and roll stabilized scanner
- Mark IIIB - III with Type 184 display (introduced as an interim model before IIIA while stabilizer production improved)
- Mark IIIC - IIIA with the 6-foot whirligig scanner
- Mark IIID - IIIA with a more powerful magnetron
- Mark IIIE - IIIA with the Type 216 display, new scanner and using a shorter pulse length
- Mark IIIF - IIIE with whirligig scanner
- Mark IIIG - IIC systems converted to 3 cm, lacking the stabilizer. Intended primarily for long-range navigation by Tiger Force
- Mark IIIH - IIIG with Type 216 display
- Mark IV - IIIA with altitude correction, links to AMU computer and Mk. XIV bomb sight. Passed over in favour of Mk. IVA
- Mark IVA - IV with whirligig scanner, standard model on Avro Lincoln bombers
- Mark V - set aside for H2X but not used
- Mark VI - IIIF operating at 1.25 cm wavelength, also with 28 inch scanner for Mosquitos. Also known as Lion Tamer.
- Mark VII - updated Mark VI with links to the navigation system, cancelled with the ending of the war
- Mark VIII - Mark IVA operating in the X-band, replacement for Mk. VII. Four produced.
- Mark IX, IXA - Mk. VIII with 200 kW magnetron and many other improvements. Used on the V bombers.
- As it was in the case of the US H2X, where the X did refer to the X band.
- This likely refers to the Canadian Mousetrap operation of 1942/43, which involved tapping telegraph lines in the USA to decode diplomatic signals being transmitted through US networks. See "Cautious Beginnings: Canadian Foreign Intelligence, 1939-51" by Kurt Jensen, page 91.
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|Wikimedia Commons has media related to H2S radar.|
- Bournemouth University Radar Recollections site
- Picture of an installed H2S unit
- A working H2S Mk 9 and NBS as used in the Vulcan, Victor, and Valiant
- Bomber's Radar - General Survey of the Three Primary Systems Used by Bomber Command - Flight article of September 1945
- Picture of a Lancaster's Fishpond display and R1154/T1154 receiver/transmitter