#include <psSphereOps.h>
We need to be able to convert between ICRS, Galactic and Ecliptic coordinates, and potentially between arbitrary spherical coordinate systems. All of these basic spherical transformations represent rotations of the spherical coordinate reference.
Definition at line 32 of file psSphereOps.h.
Data Fields | |
| double | q0 |
| double | q1 |
| double | q2 |
| double | q3 |
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Definition at line 34 of file psSphereOps.h. |
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Definition at line 35 of file psSphereOps.h. |
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Definition at line 36 of file psSphereOps.h. |
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Definition at line 37 of file psSphereOps.h. |
1.4.2