Stereographic projection
Up to the release jul23, the GILDAS implementation was:
where
are the celestial coordinates and
the
projection plane coordinates.
is an intermediate quantity.
is
the distance from the reference point in the projection plane, and
the inclination angle (not detailed here). After a few computations
one can show that the
angle is compatible with the AIPS
definition (AIPS memo 46 Eq. 3):
 |
(8) |
But, on the other hand, the coordinate modulus in the AIPS convention
is (AIPS memo 46 section 2.1.2):
 |
(9) |
which can be written as
 |
(10) |
thanks to traditional trigonometric identities 6, i.e. twice the
modulus used in
GILDAS. In other words, the spatial scaling in the GILDAS and AIPS
conventions differ by a factor 2. Of these two definitions, the
GILDAS convention was the unsatisfying one because angles from the
reference point are projected as twice less distance on the projection
plane (
for small angles, i.e.
for the GILDAS definition, while one would prefer
for correct distance measurement in the projected
plane). This has been considered as a bug in the implementation and
this was fixed with the appropriate factor in the aug23 GILDAS release. Doing so, the stereographic projection implementation in
GILDAS is now fully compatible with the AIPS one, and thus to the
CG02 one.