Rotation of Cartesian Frames of Reference

The (east, north) coordinates, in the electronic total station (ETS) frame of reference, of a target point may differ from the relative coordinates in the UTM (Universal Transverse Mercator) frame of reference. True north is difficult to determine to an accuracy of better than a couple of degrees, and, true north is not necessarily the same as north on our part of the UTM grid.

In the figure above, let X and Y represent the ETS frame of reference (X = east, Y = north), while X’ and Y’ represent the map (UTM) frame of reference (map east and north respectively). The ETS measures a coordinate (x,y) in the (X,Y) frame of reference. How do we convert this (x,y) into its correct (x’,y’) coordinate in the map (X’,Y’) frame of reference?

Let θ = angle (measured counterclockwise) of the rotation needed for axis X to be in the same position as axis X’. It can be shown that coordinates (x’,y’) are found by calculating

 

 

 

The coefficients needed to rotate coordinates from (X,Y) to (X’,Y’) can be expressed as the rotation matrix A

 

 

 

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