E.K.Cole Southend-on-Sea & Malmesbury 1939-71

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EKCO E120 Weather Radar System

Chris Poole – March 2007


Complete Unit

Introduction

The E120 Weather Radar system and its later development into the E160 system must be considered the pinnacle of valve technology weather radars and launched EKCO onto the world stage as a serious manufacturer of radar systems for civilian aircraft at a time when there was rapid expansion of passenger traffic coupled with the introduction of jets towards the end of the 1950's.

Development started in late 1951 following the successful development and flight trials of the 'military style' E38 system where valuable lessons were learned about cloud precipitation and the needs of the flight crews of passenger aircraft particularly their need to identify dangerous cloud formations such as cumulo-nimbus clouds.

The project was to take 4 years to reach the production stage, but when launched in the autumn of 1955 was arguably the best weather radar system available, probably only equalled by the RCA AVQ-10 system.

Principal Personnel

A development team was set up under the auspices of Jack Gard as head of Laboratory who assigned Jack Halsall as 'Project Engineer'.

Detailed below are the team and their areas of responsibility.

Jack Halsall – responsible for design of Transmitter/Receiver and EHT block.

John Smith - Junior Engineer - working with Jack Halsall on T/R.

Mike Rose- (Chippenham Mike Rose) gave support as a Laboratory Assistant to Jack Halsall.

Frank Burnill - Design Engineer responsible for E 120/E160 Synchroniser Unit and the Display Unit electronics.

Norman Wall – responsible for IF unit.

Jeff Saunders - responsible to Frank for the design of the display unit. Jeff also assisted Norman Wall with the design of the I.F. Unit.

George 'Gibby' Gibson – Chief mechanical Engineer – with assistance from Miss Jones was responsible for the Scanner unit.

Ian Walker – responsible for Transformer design.

Hugh Green Senior Waveguide Engineer (head of wave-guide lab)– responsible for Wave-guide development and design including 'German Toy' construction adopted for E160.

Frank Oxborough - Engineer, responsible for flight trials of E 120 / E 160, worked on Britannia and Comet installations as well as Servicing of the equipment with BOAC etc.

John Jewsbury - Responsible to Frank Burnill for work on the Synchroniser unit.

John also produced the first handbook for E 120. Organised and gave training courses on E 120 to BOAC. Serviced E 120 at various overseas bases, Singapore, Israel, Beirut and was also involved with aircrew training programmes.

Jim Mines - Lab. Assistant/ Wireman. Assisted Jack Halsall with prototype wiring on E 120 units and various modules in the T/R system including the EHT unit.

Bernard Price - Assisted Frank Oxborough in Britannia support including the Britannia's on the BOAC on Australia and Singapore routes both of which normally exhibited high levels of cumulo-nimbus activity and caused many engine shutdowns (see note below).

Support was also given to De Havilland. on the Comet II trials with E 120 and later on the Comet IV with both E120 and the later the E 160 derivative.

Editors Note. An EKCO team routinely accompanied Bristol Aircraft on flight proving trials as well as airline familiarisation flights, which were not without incident since the Proteus engines fitted to the Britannia were prone to icing within the air intakes due in the main to the construction/design involving a 'S' shaped turn in the air inlet to the turbine. (Heaters were eventually fitted to stop ice particles/fragments entering the engines when the planes reduced altitude prior to landing).

EKCO personnel also participated on the De Havilland Comet IV Icing Trials, which was filmed by the EKCO film unit.

Choice of Wavelength – 'C' Band or 'X' Band?

At the time of the E120 development there was a considerable amount of scientific research and debate within the radar and meteorological world about the best frequency to detect harmful cloud formations where proponents of the 'C' band (5.5cm) were stating that this frequency was the theoretical optimum, which was a view supported by the American radar manufacturers.

This however was not borne out by the joint EKCO-RRE (Radar Research Establishment) flight proving trials in the late 1940's (flying many tropical routes with high cumulo-nimbus cloud activity), which showed that an 'X' band (3cm) system performed with no discernable loss of performance since heavy rainfall zones were limited in area, had better discrimination and suffered less range reduction in the presence of heavy precipitation.

The EKCO-RRE research and proving trials also showed that the optimum 'beam width' for target discrimination should be no more than 5 degree's in order to allow safe passage through turbulent conditions.

Additionally despite the few advantages offered by the use of 'C' band, by adopting 'X' band, this considerably eased the packaging of units by using smaller microwave components in the T/R unit as well as on the Scanner/Antenna. There was also a beneficial effect on the aircraft installation, both in terms of weight and size.

E120 System Technical Specification

The E120 System comprised 6 units, as follows: -

  • The nose mounted Scanner unit E121
  • The avionics tray mounted Transmitter/Receiver E122
  • The avionics tray mounted Servo/Sync unit E123
  • The cockpit mounted Indicator unit(s) E124
  • The cockpit mounted Control unit E125
  • The avionics mounted Back Plate Junction Box E126

The E120 system was an 'X' band system operating on a frequency of 9,375 Mc/s powered by a 60Kw magnetron pulsed at approximately 400pps producing a 2ms pulse with a beamwidth of 5 degree's. This provided a guaranteed scan range of 120 nautical miles.

Azimuth coverage was + 75° about the fore and aft axis of the aircraft with the elevation coverage (tilt upwards and downwards) being + 7° to – 17° from the normal stabilised scanning axis. The scanner unit was roll stabilised to + 45° in roll and +18° to – 22° in pitch.

Range: The system was calibrated to have the following range markers: -

  • 0-20 nautical miles
  • 0-60 nautical miles
  • 0-120 nautical miles

The E120 system was also equipped with Iso- Echo Contour circuits to more accurately discriminate the degree of turbulence within cloud formations.

Iso – Echo Contour Briefly Explained

At the time of development, there was already evidence that the degree of turbulence within a cloud formation was related to the amount of rainfall within the cloud formation.

While an experienced operator could distinguish less dangerous cloud formations by their soft fuzzy appearance, there was a need to help aircrew discriminate and identify potentially harmful cloud formations, which should be avoided both for passenger comfort as well as the structural integrity of the aircraft (in extreme cases).

The Iso-Echo contour system display developed by EKCO for the E120/E160 system was a means to identify potentially harmful cloud formations and is best demonstrated by looking at two cloud formations, which to the naked eye can look similar and had equally intense peak precipitation levels.

Using the Iso-Echo circuitry, this not only looked at the peak precipitation levels, it also measured the rate of build up of the precipitation thus while the two cloud formations look similar, in one of the cloud formations the circuitry showed returns, which were sharper and had well defined edges, whereas in the second case the returns would show up as considerably less well defined.

The cloud formation with the sharp well-defined edges showed that there was considerably higher rate of build up, which in turn meant that this cloud formation should be avoided at all costs although best practice also recommended that both cloud formations be avoided and using the weather radar, a course plotted to avoid both.

Iso Echo 20Nm

The cloud formations show in this photograph of the radar display on the 20 Nm range and shows a strong 'ISO Echo' return from the cloud formation to port at 6 to 10 Nm, which indicates that this cloud is both turbulent and has a potential to be a heavy rain bearing cloud.

The Iso-Echo contour system display also gave the aircrew the option to invert the display on the indicator screen for any signal strength over a certain threshold thus giving the appearance of a 'black hole' on the screen, which therefore emphasised strong weather activity.

To see how effective the Iso-Echo Contour and inversion function were in action, please watch the Comet IV Icing Trials film available on this site.

Principal Customers

The E120/E160 system was widely sold, being the standard fit for the Bristol Britannia and the Comet IV, additionally it was also installed by the RAF in both aircraft being assigned the code number ARI-23041. It was also the standard fit for the Armstrong Withworth Argosy military freighter.

The system may have been fitted to other aircraft types and customers not listed here. If any readers have further information, we would be pleased to include this information.

DH Comet IV = BOAC, BEA, RAF, Aerolineas Argentina, Mexicana, East African Airlines, Olympic Airways, United Arab Airlines, Sudan Airways, Kuwait Airways.

Britannia = BOAC, RAF, El Al, Caladonian Airways, Aeronaves de Mexico, Clanair, Eagle Airways (British Eagle) Cunard, Air links, Transglobe.

Note: the above listing only shows 'first owners' and not subsequent owners, principal of whom was Britannia Airlines in the case of the Britannia and Dan-Air in the case of the Comet IV's.

Brittania Schematic

Schematic of E120 installation in Bristol Britannia – reproduced from August 1957 Ekco radar booklet

Units in Photographs

The complete system undergoing 'Polar Diagram' testing at the EKCO test hut located at RAF Kemble in 1955.

The radome shape in front of the scanner represents the nose profile of the Bristol Britannia.

This test facility was widely used by EKCO Malmesbury since it gave good 'line of sight' being located high in the Cotswolds.

Kemble

The Scanner Unit E121

E121 Scanner Unit

The Scanner unit was a full 'platform stabilised' unit, which had separate axis compensation in pitch and roll supplied from the gyro located to the top of the azimuth gearbox, which was mechanically and independently mounted using anti-vibration mounts.

Its function was to provide error signals (through sensing roll and pitch deviation of the azimuth axis from the vertical of less than a degree) to servo-amplifiers, which commanded servo-motors to maintain the azimuth axis vertical at all times provided that the aircraft stayed within the operating parameters of the system Beam tilt had it's own simple servo fed from the tilt control on the cockpit controller.

As can be seen, the wave-guide was pressurised to cabin pressure allowing operation at maximum aircraft altitude.

The photograph was taken by George Dring, who acted as the staff photographer in the 1950's.

Wimbolt Scanner

Above is a rear view photo of the scanner unit taken in 2005 at the Graham Wimbolt collection. This unit was taken from a Dan Air Comet IV when the aircraft was retired.

The E122 Transmitter/Receiver

George Dring T/R

The above photograph was a semi-official factory photograph taken by George Dring, who acted as the staff photographer in the 1950's.

The E122 Transmitter/Receiver

Wimbolt T/R

Above is a top down photo of the TR unit showing the wave-guide and IF unit: taken in 2005 at the Graham Wimbolt collection.

Below is a close up view of the T/R wave-guide and of great interest is the fact that the wave-guide is fabricated using the 'German Toy' construction technique, which indicates that this unit was manufactured circa 1958 when this system was adopted. Prior to this the wave-guide was fabricated from rectangular section aluminium 'wave-guide' tube, which was difficult to make, time consuming and had a high rejection/scrap rate during manufacture due to the high number of Aluminium brazed joints.

The E122 Transmitter/Receiver

Wimbolt T/R

The Servo-Sync Unit E123

E122 Transmitter/Receiver

Servo/Sync

The above photograph is another from the George Dring Collection showing the E123 Servo-Sync Unit opened up. Note the large cooling fan.

Close up of the Servo-Sync control 'pre-sets' photographed at the Graham Wimbolt collection 2005.

The E122 Transmitter/Receiver

Servo/Sync pre-set

The Servo-Sync Unit controlled the servo circuits for Scanner Pitch and Roll to ensure that the scanner unit followed aircraft movements and kept the scanning axis vertical within 1?degree. The Synchroniser section managed the 'Time Base', Range Markers, Iso-Echo Contour, Automatic Gain Control and Sensitivity Time Control Waveform.

The E124 Indicator Unit

E122 Transmitter/Receiver

E1240 Indicator Unit

The E124 indicator unit is a 5 inch CRT using a Plan Position Indictor (PPI) display with the position of the aircraft shown in the bottom centre. The orange colour is from a polarised Perspex front screen, which assisted the aircrew to view the screen in high ambient daylight conditions. Typically aircraft had two indictors units (one for pilot and one for co-pilot).

When active, the range markers are displayed on the screen using the signals generated by the E122 Transmitter/Receiver.

The E122 Transmitter/Receiver

Internal of Indicator

Indicator unit inner, photo from Graham Wimbolt collection.

The E122 Transmitter/Receiver

Comet IV Cockpit

Nice Cockpit photograph of Comet IVC operated by Mexicana (Reg. number XA-NAC which is under restoration) showing E124 indicator unit in situ.

The E125 Cockpit Control Unit

The E122 Transmitter/Receiver

E125 Cockpit Control Unit

This unit was the main cockpit control unit and allowed the aircrew to select the main operating functions and adjustments with the exception of the display contrast and brightness, which were adjustable on the E124 indicator unit.

The E126 Back-Plate Junction Box

The E122 Transmitter/Receiver

Backplate

The E126 Back-Plate Junction Box is the common connection box fitted to the rear of the T/R and Servo/Sync unit in the avionics bay of the aircraft. This unit linked together all the individual units. Photograph taken in 2005 for the Graham Wimbolt Collection.

The author wishes to thank Jack Halsall for his considerable contribution and invaluable guidance, additionally I also wish to kindly thank Mike Rose, John Jewsbury, John Smith and Bernard Price who all contributed their recollections as source information.








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