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made by an altitude screw, using a high accuracy bubble level fixed to the telescope. This can be viewed by a mirror whilst adjusting, or the ends of the bubble in a "split bubble" display can be viewed within the telescope. This also allows assurance of the accurate level of the telescope whilst the sight is being taken. However, in the case of an automatic level, altitude adjustment is done automatically by a suspended prism due to gravity, as long as the coarse levelling of the instrument base is accurate within certain limits.
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additional assurance that the telescope is level whilst taking the sight. This allows faster operation as the bottom mount need not be truly level, though it will introduce a slight error as the vertical axis of the mount is not completely coincident with the telescope centre. The split bubble works by displaying half of both ends of the bubble side by side in the telescope, and when the curved ends are aligned it is level.
363:) that, when set close to level, automatically removes any remaining variation. This reduces the need to set the instrument base truly level, as with a dumpy level. Self-levelling instruments are the preferred instrument on building sites, construction, and during surveying due to ease of use and rapid setup time.
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vertical at the point under measurement. The surveyor rotates the telescope until the graduated staff is in the crosshairs and records the reading. This is repeated for all sightings from that datum. Should the instrument be moved to another position within sighting distance, it is re-levelled, and a
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which is graduated in inches or centimeters. The level staff is placed with its foot on the point for which the level measurement is required. The telescope is rotated and focused until the level staff is plainly visible in the crosshairs. In the case of a tilting level, the fine level adjustment is
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staff using electronic laser methods. The height of the staff where the level beam crosses the staff is shown on a digital display. This type of level removes interpolation of graduation by a person, thus removing a source of error and increasing accuracy. During night time, the dumpy level is used
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errors. Because the telescope is not fixed to the level adjusting mechanism, the "Y" instrument is assembled and disassembled for each sighting station. However, the dumpy level is permanently secured to its two support arms and the levelling mechanism, thereby reducing measurement uncertainty and
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is a variant which has a precision vertical adjustment screw which tilts both the telescope and the high accuracy bubble level attached to it to make them level. This reduces the complete reliance on the levelling accuracy of the instruments' bottom mount, and the "split bubble" display gives
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are used to achieve the necessary accuracy. Traditionally the instrument was completely adjusted manually to ensure a level line of sight, but modern automatic versions self-compensate for slight errors in the coarse levelling of the instrument, and are thereby quicker to use.
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466:, the narrator states, "He knew every subtle incline of the ten miles of ground between Abbot's Cernel and Sherton—the market town to which he journeyed—as accurately as any surveyor could have learnt it by a Dumpy level."
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When level, the staff graduation readings at the crosshairs and stadia marks are recorded, and an identifying mark or marker placed where the level staff rested on the object or position being surveyed.
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of a target object with respect to a reference in the horizontal plane. The instrument is rotated to sight the target, and the vertical and horizontal angles are read off calibrated scales
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The telescope of the historic "Y" level is held in two brass arms, which are part of the mount and the telescope could be easily removed to allow sighting reversal though 180 degrees or an
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is the oldest and bulkiest of the older style optical instruments. A low-powered telescope is placed in a pair of clamp mounts, and the instrument then leveled using a
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or the historic "Y" level. It operates on the principle of establishing a visual level relationship between two or more points, for which an inbuilt
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considerably reducing the time taken to set up the instrument. The dumpy uses the same basic principle of level sighting.
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After careful setup of the level, the height of the crosshairs is determined by either sighting from a known
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A "Y" level. The telescope can be removed and reversed, or be axially rotated, to remove collimation errors.
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sighting taken of a known level in the previous survey. This relates any new levels to the previous levels.
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with known height determined by a previous survey or an arbitrary point with an assumed height is used.
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to measure height differences and to transfer, measure, and set heights of known objects or marks.
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The surveyor looks through the eyepiece of the telescope while an assistant holds a vertical
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The azimuth is the angle formed between two points of interest in the horizontal plane
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A "Y" level. The telescope can be removed and reversed or rotated to remove errors.
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Gravatt's
Improved Level, commonly called (from its appearance) the Dumpy Level.
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The internal prism mechanism of an automatically levelling telescope.
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in conjunction with an auto cross laser for accurate scale readings.
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A modern automatic optical level with a horizontal transit readout.
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Sighting is done with an assistant surveyor who holds a graduated
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It is also known as a surveyor's level, builder's level,
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includes an internal compensator mechanism (a swinging
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Modern automatic level in use on a construction site
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241:, who was commissioned to examine a scheme for the
60:. Unsourced material may be challenged and removed.
460:In the first chapter of Thomas Hardy's 1887 novel
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193:The optical level should not be confused with a
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120:Learn how and when to remove this message
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450:Low accuracy check leveler for hand use
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532:Saikia; et al. (30 Oct 2010).
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610:"All About Transit Levels"
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560:. craig-telescope.co.uk
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581:. "dumpy", adj, 2.
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564:2012-05-31
519:References
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80:newspapers
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534:Surveying
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328:The term
319:wye level
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477:See also
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