#include <psCoord.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. We specify a general transformation function which takes a structure, psSphereTransform, defining the transformation between two spherical coordinate systems
Definition at line 107 of file psCoord.h.
Data Fields | |
| double | alphaP |
| Longitude of the target system pole in the source system. | |
| double | cosDeltaP |
| Cosine of target pole latitude in the source system. | |
| double | sinDeltaP |
| Sine of target pole latitude in the source system. | |
| double | phiP |
| Longitude of the ascending node in the target system. | |
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Longitude of the target system pole in the source system.
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Cosine of target pole latitude in the source system.
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Longitude of the ascending node in the target system.
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Sine of target pole latitude in the source system.
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1.4.1