Early bombsights Prior to the introduction of the CSBS, bombsights were generally very simple systems of limited accuracy suitable only for low-level use. The primary pre-war device in RNAS service was the Lever Sight, which the pilot had to hold out of the cockpit in one hand while flying the aircraft with the other. The Central Flying School Sight replaced this in 1915, but was difficult to install in the cockpit. The CFS was in turn replaced by the
Equal Distance Sight (EDS) designed in 1916 by F. W. Scarff, better known for the development of the
Scarff ring. The EDS allowed the bomb-run parameters to be entered once and then left the pilot free to fly the plane. None of these sights had a way to calculate
drift, the sideways motion of the bombs due to wind. This meant the aircraft had to attack their targets directly along the wind line. Even in this direction, the wind would cause the bombs to fall long or short. To correct for this, the bomb aimer would first measure their speed over the ground using a
stopwatch. They would next look up the time it would take the bombs to reach the ground from their current altitude using a pre-computed table. Then, using both values, they would look up the proper angle for the sights, the so-called
range angle, and set the sights to that angle. This solution was far from practical, and prone to error. In 1916, Harry Wimperis started the design of a new bombsight, working in collaboration with Scarff. This new
Drift Sight included a simple system that greatly eased the measurement of the wind. By observing their movement over the ground, the aircraft would first determine the direction of the wind. The aircraft would then turn to fly at right angles to this wind direction so that the wind was pushing the aircraft sideways. Observing the sideways drift of the aircraft by comparing the motion of objects on the ground to a metal rod along the side of the bombsight, the drift could be seen. Using a knob, the rod was angled away from the side of the aircraft until objects could be seen moving directly along the line of the rod. A gear in the knob that adjusted the rod angle also drove the sights fore or aft, moving them to account for the wind speed. This eliminated the need for a stopwatch to measure the
ground speed. This technique automated the adjustment of the range angle to account for wind, but the Drift Sight was still useful only for bomb runs along the wind line.
Course Setting Bomb Sight . This example has been set for a wind just off the left side of the tail, as indicated by the arrowhead in the compass rose. The matching rotation of the wind bar can be seen. When an aircraft flies in the presence of wind, its flight path over the ground is a function of the aircraft's airspeed, heading, and the speed and direction of the wind. These are combined using basic
vector addition to return the
course made good or
track. These calculations are a basic part of
air navigation and
dead reckoning, taught to all aviators. Wimperis was an expert on the topic, and would later write a well-known book about it. To aid in the necessary calculations, it was common to use a simple
mechanical calculator that combined a
slide-rule like calculator on one side with a vector calculator on the other. The best-known modern example is the
E6B, which remains a basic part of every pilot and navigator's toolkit. Using the vector calculator and basic measurements, one can easily calculate the winds aloft and then the course made good. These calculations are identical to those needed to properly account for the effects of winds on the bombing approach. The problem was that these calculations were complex, time-consuming and error prone. Wimperis decided to attack the calculation problem by incorporating a similar vector calculator directly into the bombsight, combining it with a drift measure similar to the one from the earlier Drift Sight. Like the Drift sight, simply taking a measure of the wind using the sight itself provided all of the unknown variables needed to completely calculate the bombing approach. Unlike the Drift Sight, the new design not only calculated the effect on the distance the bombs travelled, but also indicated the proper direction to fly to approach the target so the aircraft reached it with no residual sideways motion – thereby cancelling any drift no matter the direction of approach. His new Course Setting Bomb Sight featured a large
compass at the rear that could be used for making general calculations of wind speed or solving navigational problems. In most cases these could be ignored; the bomb aimer dialled in the wind direction on the compass, then wind speed, airspeed and altitude on different knobs. Through internal mechanisms, these adjustments carried out all of the calculations needed to set the approach and range angle. Through these calculations the CSBS allowed bombing from any direction, freeing the aircraft from the wind line for the first time.
Production and use In testing in December 1917 at the
Scilly Isles air station, in eight bomb runs the CSBS scored two direct hits, and near-misses on all six other runs. Production quickly followed, and by 1918 about 720 had been produced. The
Royal Flying Corps (RFC) started using the Mark I sight as soon as supplies were available, and by April 1918 were also fully converted to this type. For his work on the CSBS and the Drift Sight Wimperis was awarded £2,100 by the Royal Commission on Awards to Inventors. In the post-war era, work on new bombsights was seriously curtailed, and little new development had taken place by 1930. Several minor variations of the CSBS had been introduced during this period to adapt to higher speeds, higher or lower altitudes, and new types of bombs. These also included a separate adjustment for
trail, the deceleration of the bomb due to
drag. At low speeds and altitudes the time between drop and impact was too short for the bombs to reach
terminal velocity so the trajectory of the bombs was roughly parabolic. At higher altitudes or forward speeds the bombs would reach terminal long before impact, which had the effect of making the last portion of the flight path more vertical. The trail adjustment, set by dialling in the measured terminal velocity for the bombs being dropped, used a
cam to move the height bar forward away from the vertical, reducing the range angle and thereby reducing the range to account for this effect. Many thousands of CSBSs were sold around the world, and many other sights were developed from the basic idea. In the mid-1930s, the basic CSBS concept was largely universal for production bombsights.
Mk. VII and IX During its development prior to the opening of
World War II, the CSBS added several new features. A simple modification found on pre-war models was the
Auxiliary Drift Bar attachment. This consisted of a single drift wire in a C-shaped clamp that could be moved along the main drift wires, and rotated in relation to them. Previously, the bomb aimer would use the main drift bar as a tool to measure wind speed, but it was found that the bomb aimers would forget to reset it to the proper angle for bombing when things got busy. These same measurements could be made with the Auxiliary Bar, leaving the main drift bar in the proper position. Later versions used by
RAF Coastal Command and the
Royal Navy also included a further adjustment, the
Fourth Vector, for attacking moving targets. This was primarily intended for use against
ships and
submarines. This was a fairly complex system of rotating rings and sliders that allowed the bomb aimer to dial in the relative course of the target and its estimated speed. This moved the backsight directly fore and aft, and turning the heading dial adjusted how much the speed dial moved the backsight. As the resulting mechanism was fairly large and complex, the sights were also available with the Fourth Vector removed, denoted with a *, as in the Mk. IX A*.
Mk. X Prior to the war a major redesign of the CSBS was underway. The new
Mk. X replaced the vertical slider used for altitude adjustment with a horizontally-moving backsight at the top of the device, and the entire foresight and drift wire area was made considerably smaller. The calculator and wind drift settings, formerly mounted on top and in front of the large
compass at the rear of the earlier models, was moved to the left side of the device and changed in form to make it smaller as well. The compass, no longer containing pointers and dials, was replaced with a smaller unit. The result was a version of the CSBS that was much smaller than earlier versions. About 5,000 of the new Mk. X were built and awaiting fitting to aircraft at the opening stages of the war. After the
disastrous raid on
Wilhelmshaven in 1939, the RAF was forced to abandon daylight attacks and move to night bombing. The Mk. X proved to have very poor visibility at night, and it would be difficult to modify it to correct this problem. The Mk. X had to be abandoned, and Mk. VII's and Mk. IX's hurriedly re-fit to aircraft. Thus the older versions of the CSBS soldiered on long after they were due to be replaced, and remained the primary British bombsights into 1942. The Mk. VII was widely found on slower aircraft and training schools, while the Mk. IX was used in higher speed aircraft.
Mk. XI Another problem with all of the existing CSBS designs was that it could only be read correctly with the aircraft absolutely level. This was true especially during the run-up to the drop point, when the sight was used to correct the direction of flight through the use of the drift wires. The
biplane bombers the CSBS had been developed for had the ability to slip-turn using the rudder only, which made it simple for the pilot to adjust their heading without affecting the aim too much. Modern monoplanes were subject to an effect known as
dutch roll that makes them oscillate for a time after turning to a new heading. During this time the drift wires were difficult to use, so the entire process of correcting the flight path was greatly extended. In the aftermath of the Wilhelmshaven raid on 3 September 1939, it was found that the lengthy setup and bomb run demanded by the CSBS made its aircraft extremely vulnerable to fighters and
anti-aircraft artillery. At a pre-arranged meeting on 22 December 1939, Air Chief Marshal Sir
Edgar Ludlow-Hewitt made a request for a new bombsight that did not require such a long run into the target, and which would allow the aircraft to manoeuvre throughout the bomb run. The solution to this problem was well understood within the industry: use gyroscopes to provide a level platform to mount the bombsight so it did not move relative to the ground even if the aircraft moved. Today these are known as an
inertial platform. However, the large physical size of the CSBS series, especially the long drift bar, made it difficult to mount successfully on a platform. A compromise solution was designed as the
Mk. XI, which mounted a single drift wire and iron sight on the front of a gyroscope taken from a
Sperry artificial horizon that was already common in RAF use. This provided stabilization in the roll axis, which greatly eased the problem of sighting while maneuvering. In order to make it fit on the platform, all of the mechanical calculator portions of the sight were removed. Instead, the bomb aimer had to use manual
slide rule calculators to find the drift and bombing angles, and then set the bombsight to these values. The bombsight was unable to quickly adapt to changes in direction or altitude, and in this case was even slower to calculate such changes. Very few of the Mk. XI designs were produced.
Mk. XII and Mk. XIV, a new approach , is stabilized and uses an optical system in place of the drift bar. As if these problems were not enough, the RAF found in the training schools that it was all too common for the bomb aimers to dial in an incorrect setting, or forget to update one when conditions changed. It was planned that many of these problems would be solved on the Automatic Bomb Sight (ABS), which had been under development from before the war, and used very simple inputs from the bomb aimer to carry out all the needed calculations. Unfortunately, the ABS was even larger than the CSBS, and the demands for new bombsights to be stabilized would make it even larger and further delay its service entry. Something was needed in the meantime. The physicist and scientific advisor
Patrick Blackett took up the challenge of fixing all of these problems at once, producing the Blackett sight with the
Royal Aircraft Establishment. First, the manual calculator was replaced by an external box operated by a new crew member. The box contained the inputs needed to drive the vector calculator, as well as copies of the various aircraft instruments displaying the required information. The operator simply had to keep the input dials set so their indicators overlapped those on the instruments. Turning the dials drove the machine to calculate the correct angles, as on the earlier CSBS models, but then fed them directly into a remote sighting unit, the
sighting head. This provided practically instant updates of the sighting angles. The wire sights of the earlier models were replaced by
reflector sights indicating the location the bombs would hit if dropped at that instant. This used a lighted optical crosshairs, which was perfectly visible at night. As the sighting head lacked the vector computer it was much smaller than earlier models, which allowed it to be easily mounted on a stabilized platform. This allowed the sights to be used even while the aircraft was maneuvering, and required only 10 seconds to settle. Together, these changes dramatically simplified the task of maintaining an accurate bombsight setting. On the downside, it required the addition of a new crew member to operate the system. This was not a minor problem as most aircraft had no room for them. This led to the ultimate development of the series, the Mk. XIV. This version replaced the manual input dials with ones powered by air suction bled from the engines. Before the mission, the bomb aimer entered basic information about the target altitude and the bombs being dropped, and periodically updated the wind speed and direction. Everything else was fully automated. Versions were also developed that replaced the altitude measurement with a
radar altimeter for low-altitude use, but these
Mk. XV and
Mk. XVII were not used operationally. The Mk. XIV was a major advance over the Mk. IX, but service entry was slow. It was not until January 1942 that it was given priority. This was aided by
Sperry Gyroscope, who re-designed the system to U.S. production methods. They sub-contracted construction to
A.C. Spark Plug who built tens of thousands as the Sperry T-1. It did not offer the level of accuracy of tachometric bombsights like the
Norden or ABS, but for night area bombing from medium altitude as practiced by
RAF Bomber Command this was not an issue. The Mk. XIV remained in RAF use until 1965.
SABS Later in the war the development of the
Tallboy and
Grand Slam earthquake bombs demanded accuracy that even the Mk. XIV could not supply. For this role, the Automatic Bomb Sight was dusted off and mounted to new stabilization platform, producing the
Stabilised Automatic Bomb Sight. This complex device was available only in very small numbers from late 1943 on, and used only by specific groups within the RAF. ==Description==