The SEDRIS Data Representation Model
APPENDIX A - Classes SEC 3D Location |
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An instance of this DRM class specifies a coordinate for an SRF based on the Solar Ecliptic SRFT.
See 8.5.12 Solar ecliptic SRFT of ISO/IEC 18026 for a complete definition.
SRFs derived from the Solar Ecliptic SRFT are convenient for representing such data as:
SEC is quasi-inertial in that it has a yearly rotation.
See the SRM for additional details.
SRM_Spherical_3D_Coordinate | coordinate; | 1 |
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The coordinate field specifies the set of coordinate-component values.
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