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Theodolite ppt in 7


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  • 1. ARUN.H.KAMA Diamond training 8453426818
  • 2. WealthA DXN Presentation By:- Navneet Verma ©Navneet Verma +91-9935618181
  • 4. VIDEO
  • 5. INTRODUCTION Theodolite is used to measure the horizontal and vertical angles. Theodolite is more precise than magnetic compass. Magnetic compass measures the angle up to as accuracy of 30’. However a vernier theodolite measures the angles up to and accuracy of 10’’, 20”. There are variety of theodolite vernier, optic, electronic etc.
  • 7. Vertical axisVERNIER THEODOLITETraverse/horizontal axis Vertical circle rigidly fixed to the telescope Line of Sight Alidade assembly  Vernier theodolite is also known and transit. Horizontal circle assembly  A transit theodolite is one in which the telescope can be Levelling head assembly rotated in a vertical plane. Three assemblies of Theodolite
  • 8.  Main parts of a theodolite  Levelling head (7): Levelling head is used to attach the instrument to tripod and attach the plumb bob along the vertical axis of the instrument.
  • 9. MAIN PARTS-2 Lower plate/circle plate (18): an annular horizontal plate with the graduations provided all around, from 0 to 360°, in a clockwise direction. The graduations are in degree divided in to 3 parts so that each division equals to 20 min. Horizontal angles are measured with this plate. The size of the theodolite is defined by the diameter of horizontal circle. Upper plate (17): Horizontal plate of smaller diameter provided with two verniers. on diametrically opposite parts of its circumference. These verniers are designated as A and B. They are used to read fractions of the horizontal circle plate graduations. The verniers are graduated in 20 min and each minute is divided in 3 to 5 parts making least count 20” or 10”.
  • 10. MAIN PARTS-3 Clamps and tangent screws (15, 19):  There are two clamps and associated tangent screws with the plate. These screws facilitate the motion of the instruments in horizontal plane.  Lower clamp screw locks or releases the lower plate. When this screw is unlocked both upper and lower plates move together. The associated lower tangent screw allows small motion of the plate in locked position.  The upper clamp screw locks or releases the upper vernier plate. When this clamp is released the lower plate does not move but the upper vernier plate moves with the instrument. This causes the change in the reading. The upper tangent screw allows the fine adjustment.
  • 11. MAIN PARTS-4 Plate level (5):  Spirit level with the bubble and graduation on glass cover.  A single level or two levels fixed in perpendicular direction may be provided.  The spirit level can be adjusted with the foot screw (21) of the levelling head (7). Telescope (10): The essential parts of the telescopes are eye-piece, diaphragm with cross hairs, object lens and arrangements to focus the telescope.
  • 12. MAIN PARTS-5 Vertical circle (1): circular plate supported on horizontal axis of the instrument between the A-frames. Vertical circle has graduation 0-90 in four quadrants. Vertical circle moves with the telescope when it is rotated in the vertical plane. Vertical circle clamp and tangent screw (11): Clamping the vertical circle restrict the movement of telescope in vertical plane. Altitude level (2): A highly sensitive bubble is used for levelling particularly when taking the vertical angle observations.
  • 13. Reading atheodolite Vernier scale graduation
  • 14. Important Definition Changing face  Revolving the telescope by 180 in vertical plane about horizontal axis  Again revolving the telescope in horizontal plane about vertical axis.
  • 15. Adjustment of the theodolite Temporary Adjustment Setting up the theodolite
  • 16. Measurement of horizontal angle  Measurement of Angle ABC  The instrument is set over B.  The lower clamp is kept fixed and upper clamp is loosened.  Turn the telescope clockwise set vernier A to 0° and vernier B to approximately 180°.  Upper clamp is tightened and using the upper tangent screw the vernier A and B are exactly set to 0° and 180°.  Upper clamp is tightly fixed, lower one is loosened and telescope is directed towards A and bisect the ranging rod at A.  Tightened the lower clamp and turn the lower tangent screw to perfectly bisect ranging rod at A.  Loose the upper clamp and turn the telescope clockwise to bisect the ranging rod at C tightened the upper clamp and do the fine adjustment with upper tangent screw.  The reading on vernier A and B are noted. Vernier A gives the angle directly and vernier B gives the reading by subtracting the initial reading (180°) from final reading
  • 17.  Read these two method  Repetition method  Reiteration method
  • 18. Vertical angle measurement-1
  • 19. Vertical angle measurement-2
  • 20. VIDEO
  • 21. Measurements of Deflection angle magnetic bearing P B  A N B C  A
  • 22.  Anging and extending a line Method of traversing  Included angle method  Deflection angle method  Fast angle (or magnetic bearing method)
  • 23. VIDEO
  • 24. Computation of latitude and departure Latitude of a line is the distances measured parallel to the north south of the North-South direction Departure of the line is the distance measured parallel to the east-west direction
  • 25. Computing latitude and departure
  • 26. PROBLEM-1 While making survey through the woods, a surveyor with the hand compass started from point A and walked a thousand steps in the direction S67⁰W and reached a point B. then he changed his direction and walked 512 steps in the direction N10⁰E and reached a point C then again he changed his direction and walked 15 04 steps in the direction S65⁰E and reached a point D as shown in Figure Now the surveyor wants to return to the starting point A. In which direction should he move and how many steps should he take.
  • 27. Sources of errors in theodolite Instrumental errors  Non adjustment of plate bubble  Line of collimation not being perpendicular to horizontal axis  Horizontal axis not being perpendicular to vertical axis  Line of collimation not being parallel to axis of telescope  Eccentricity of inner and outer axes  Graduation not being uniform  Verniers being eccentric
  • 28.  . Personal errors Natural errors  High temperature causes error due to irregular refraction.  High winds cause vibration in the instrument, and this may lead to wrong readings on verniers Closing error
  • 29. Balancing of traverse Bowditch’s rule:  Total error is distributed in proportion to the lengths of the traverse legs.
  • 30. Calculation of traverse area
  • 31. PROBLEM Calculate the latitudes, departures and closing error for the following traverse conducted at allahabad. Adjust also the traverse using Bowditch’s rule. Line Length WCB AB 89.31 45⁰ 10’ BC 219.76 72⁰ 05’ CD 151.18 161⁰ 52’ DE 159.10 228⁰ 43’ EA 232.26 300⁰ 42’