Tacheometry by optical wedge (subtense wedge) system: The theodolites designed for this method have which distinctive feature?

Difficulty: Easy

Correct Answer: A glass wedge fitted inside the telescope

Explanation:


Introduction / Context:
Tacheometric distance measurement can be achieved by several optical principles: fixed stadia hairs, anallatic lenses, and optical wedge (subtense wedge) systems. The wedge method introduces a fixed angular separation in the line of sight, allowing distance to be computed from the staff intercept formed by the wedge, without relying on traditional stadia hairs.


Given Data / Assumptions:

  • Instrument is a theodolite adapted for tacheometry.
  • Optical wedge produces a constant small angular displacement.
  • Standard staff with suitable markings is observed.


Concept / Approach:

In the optical wedge system, a glass wedge (or a pair forming a small prism angle) is fitted inside the telescope. The wedge splits or displaces the image to create a fixed angular subtense at the eye. The observed intercept on the staff, when multiplied by a constant, yields the horizontal distance. This differs from classical stadia where stadia hairs define the fixed subtense.


Step-by-Step Solution:

Recognize that a wedge provides constant angular separation.Relate staff intercept to distance via distance = K * intercept (constant depends on wedge angle).Note that no additional external attachment is required when the wedge is built inside the telescope.


Verification / Alternative check:

Manufacturer specifications of wedge tacheometers describe an internal optical wedge element and corresponding constants, confirming option (c).


Why Other Options Are Wrong:

(a) describes stadia-hair tacheometers; (d) implies an external wedge in front of the objective, uncommon in standard designs; (e) refers to a different micrometer-based technique; (b) is incomplete because although classical stadia hairs may be omitted, the defining feature is the internal wedge.


Common Pitfalls:

Confusing an anallatic lens (which corrects additive constant) with a wedge system; assuming the wedge is external rather than internal.


Final Answer:

A glass wedge fitted inside the telescope

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