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SLA_UNPCD - Remove Radial Distortion

ACTION:
Remove pincushion/barrel distortion from a distorted $[\,x,y\,]$ to give tangent-plane $[\,x,y\,]$.
CALL:
CALL sla_UNPCD (DISCO,X,Y)
GIVEN:

DISCO D pincushion/barrel distortion coefficient
X,Y D distorted $[\,x,y\,]$
RETURNED:

X,Y D tangent-plane $[\,x,y\,]$
NOTES:
  1. The distortion is of the form $\rho = r (1 + c r^{2})$, where $r$ is the radial distance from the tangent point, $c$ is the DISCO argument, and $\rho$ is the radial distance in the presence of the distortion.
  2. For pincushion distortion, C is +ve; for barrel distortion, C is $-$ve.
  3. For X,Y in units of one projection radius (in the case of a photographic plate, the focal length), the following DISCO values apply:




    Geometry DISCO
    astrograph 0.0
    Schmidt $-$0.3333
    AAT PF doublet +147.069
    AAT PF triplet +178.585
    AAT f/8 +21.20
    JKT f/8 +14.6




  4. The present routine is a rigorous inverse of the companion routine sla_PCD. The expression for $\rho$ in Note 1 is rewritten in the form $x^3 + ax + b = 0$ and solved by standard techniques.

  5. Cases where the cubic has multiple real roots can sometimes occur, corresponding to extreme instances of barrel distortion where up to three different undistorted $[\,x,y\,]$s all produce the same distorted $[\,x,y\,]$. However, only one solution is returned, the one that produces the smallest change in $[\,x,y\,]$.


next up previous 269
Next: SLA_V2TP - Direction Cosines to Tangent Plane
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SLALIB --- Positional Astronomy Library
Starlink User Note 67
P. T. Wallace
19 December 2005
E-mail:ussc@star.rl.ac.uk

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