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JCMT Pointing Model - Parameter 4

JCMT Pointing Model - Parameter 4


The amount by which the telescope beam is not perpendicular to the elevation axis.

In the following diagram :

A, A' indicate the directions of the ideal and real telescope beams.
A star at real azimuth a has apparent azimuth a' , so the change in azimuth is   a' - a = -theta.

Any misalignment of the beam in the elevation direction is incorporated into the elevation zero-point.


imc @ jach.hawaii.edu
Updated: 09 October 1997
Contact: Iain Coulson. Updated: Sat Nov 6 18:00:33 HST 2004

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