Ramsden surveying instruments

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Ramsden RS, the theodolite of 1787. Destroyed by war damage in 1941.

The Ramsden surveying instruments discussed in this article are those constructed by Jesse Ramsden and used in high precision geodetic surveys carried out in the period 1784 to 1853. This includes the five great theodolites—great in name, great in size and great in accuracy—used in surveys of Britain and other parts of the world. Ramsden also provided the equipment used in the measurement of the many base lines of these surveys and also the zenith telescope used in latitude determinations.

The great theodolites[edit]

A total of eight such instruments were manufactured by Ramsden and others for use in Britain, India and Switzerland.[1][2] Ramsden himself constructed three theodolites and a further two were completed to his design by Mathew Berge, his son-in-law and business successor, after Ramsden's death in 1805. Of the other instruments one was constructed by William Cary and the other two by the firm of Troughton and Simms.

The Royal Society theodolite[edit]

In 1783 the Royal Society of London reacted to French criticism of Greenwich Observatory by seeking Royal assent to undertake a high precision geodetic survey, the Anglo-French Survey (1784–1790), between Greenwich and the established French survey stations on the other side of the English Channel. Approval having been granted, General William Roy agreed to undertake the work and he immediately approached Ramsden to commission new instruments. Three years later the "great" theodolite was delivered after a delay attributable to Ramsden's tardiness, workshop accidents and his prediliction for continuous refinement—"this won't do, we must have at it again".[3] The instrument was paid for by the Crown and the King immediately presented it to the Royal Society; for this reason the theodolite is designated as the Royal Society theodelite, or Ramsden RS in short.

There is a complete description of this theodolite in the final report of the Anglo-French Survey (1784–1790).[4] The instrument was large, 36 inches (914 mm) across and it was normally mounted on a stand which placed the sighting telescope between 5 and 6 ft. high. It weighed about 200 lb (90 kilo) and the accessories and cases weighed as much again. It travelled around Britain for over sixty years, in its own sprung carriage, to locations where it was hauled up mountains, church towers and even scaffolded steeples.

Detail of the micrometer microscopes.

The horizontal circular scale was divided very accurately with divisions at 15 minute (of arc) intervals using one of Ramden's own dividing engines;[5] the marks on the 36 inch diameter scale would be about 1/6 inch (or 4mm) apart. The position of the telescope could therefore be read to the nearest quarter of a degree by eye but the exact position between the divisions was read with the aid of micrometer microscopes fitted with adjustable cross wires in the focal plane, as shown. The threads of the screws were such that fifteen full turns moved from from one scale mark to the next, i.e. 15 minutes, and since the scale on the adjusting knob allowed one sixtieth of a turn to be measured the resulting accuracy was within one arc second.

The instrument is also fitted with a vertical semi-circular scale to measure the elevations of distant stations and therefore a height difference. Cross wires similar to those used in the microscopes are fitted into the eyepiece; they are adjustable by a screw thread which allowed angles to be measured to within five arc seconds.

Typical distances in the Anglo-French survey were less than 20 miles (32 km): at that distance one second of arc corresponds to lateral or vertical displacements at the target station of approximately 7 inches (17 cm). No other theodolite could match this precision at that time. It was the first instrument to be able to measure the spherical excess of a large survey triangles.

After completion of the Anglo-French survey this instrument was stored at the Royal Society but in 1799 the Board of Ordnance requested its use for the Principal Triangulation of Great Britain. On completion of the Survey the theodolite was stored in the headquarters of the Ordnance Survey at Southampton where it was destroyed in the bomb raids of 1941.[6]

The Board of Ordnance theodolite[edit]

Ramsden BO, the theodolite of 1791. Now in the Science Museum, London[7]

In his report to the Royal Society in 1875 William Roy had noted the suitability of India as a location for both meridian arc and parallel arc measurements. To his delight the East India Company were willing to undertake such a venture and ordered a second great theodolite from Ramsden. It was ready in 1791 but Ramsden felt obliged to increase the price because of problems in its manufacture. To his surprise the company rejected his price and refused to purchase the instrument. It was bought by the Duke of Richmond who, as Master of the Board of Ordnance, had provided most of the finance for Roy's Anglo-French Survey (1784–1790). The theodolite is designated as the Board of Ordnance theodolite, or Ramsden BO in short. Richmond's intention was to use the new theodolite on the extension of Roy's survey to the southern counties of Britain. The instrument was basically the same as the first with added refinements, mainly to the number and placement of the microscopes with their precision micrometer stages. It was in use until the completion of the Principal Triangulation of Great Britain in 1853 and it is now in the Science Museum in London.[7]

There is a description of the improvements made to this theodolite in the account of the Trigonometrical Survey for the years 1791–1794 by Mudge, Williams and Dalby.[8]

Other Ramsden theodolites[edit]

Ramsden made at least one other 3ft. theodolite of which parts were discovered in Switzerland.[2] After his death his firm was inherited by Mathew Berge who is known to have constructed two more large instruments to Ramsden's design.[2] Ramsden made many theodolites including an eighteen inch instrument of the same general design as the great theodolites.[9] This instrument and his two great theodolites are described in the account of the Principal Triangulation by Clarke & James (1858).[10]

Great theodolites by other builders[edit]

Although the East India company turned down Ramsden's second theodolite they commissioned a similar design from another London instrument maker, William Cary. This theodolite was in use in India from 1802 although there was a slight hiatus in 1808 when it was damaged when being hauled to the top of a building. It was repaired and in use for sixty years. A new theodolite to an improved design was made for the Indian Survey by Troughton and Sims in 1830 and the two together saw service until 1874 when the Cary instrument was replaced by another by Troughton and Sims. This last instrument was a monster weighing 1455 lbs when in its travelling cases: it was no surprise that it was deemed too heavy for transport up mountains and it passed to South Africa in 1882.[2] No more great instruments were made after 1874 for continuing advances in precision instruments eclipsed their performance: by the end of the nineteenth century an accuracy of 1 arc second could be obtained with 12 inch instrument.[11]

Chains and rods[edit]

Eighteenth century surveyors used Gunter's chains which were 22 yards long (one chain with 100 links of 7.92 inches). Their accuracy was adequate for cadastral surveying but they were deemed insufficiently accurate for the Anglo-French Survey (1784–1790), Britains first high precision survey. Roy asked Ramsden to prepare a new chain of 100 links, each one foot in length.[12] He also asked Ramsden to prepare three precisely calibrated wooden rods 20 feet long. These proved to be a failure because of fluctuations in length due to varying humidity; instead three calibrated glass tubes were used. The chain proved to be as accurate as the glass tubes and it was in use for baseline surveys over the next thirty years.[13] Later, even more precise measurements showed that the accuracy of Ramsden's chain was about three inches in five miles. In actual use the chain was supported throughout its length by wooden trestles and tensioned with a known constant weight. It's coefficient of thermal expansion was carefully measured so that temperature fluctuations could be taken into account. Full details (with plates) are given in Roy's account of the measurement of the Hounslow baseline.[14]

The zenith telescope[edit]

Ramsden's zenith telescope.

The zenith telescope constructed by Jesse Ramsden in 1802 which was used to determine the latitude of many stations of the Principal Triangulation of Great Britain. This portable instrument was designed to bring observatory work to field work. The outer frame stood about 12 ft. high and the telescope mounted on an inner frame was 8 ft. long. The telescope was restricted to observations within a few degrees of the zenith in order to prevent errors due to refraction. A complete description of the instrument is given by Pearson.[15]


References[edit]

  1. ^ McConnell 2007Jesse Ramsden (1735–1800)
  2. ^ a b c d Insley 2008 The Great Theodolites
  3. ^ Ramsden the optician
  4. ^ Roy 1790 pp135-160 The final report of the Anglo-French Survey (1784–1790).
  5. ^ Ramsden 1877 The dividing engines.
  6. ^ Owen & Pilbeam 1992, page 9
  7. ^ a b Ramsden's three foot geodetic theodolite, 1792, Science Museum, retrieved 2010-07-10 
  8. ^ Mudge, Dalby & Williams 1795, pp. 445–446 Account of the Trigonometrical Survey for the years 1791–1794.
  9. ^ Picture of Ramsden's 18 inch theodolite
  10. ^ Clarke & James (1858) Principal Triangulation Section 2, page 43.
  11. ^ Turner 1983 Chapter 14.
  12. ^ Picture of Ramsden's chain
  13. ^ The chains were superseded by Colby's compenstion bars. See Clarke & James (1858) Principal Triangulation Section 5, page 200
  14. ^ Roy (1785). Measurement of the Hounslow baseline.
  15. ^ Pearson (1829) An introduction to Astronomy.

Bibliography[edit]