A coordinate within the Solar Magnetic (SM) 3D Spatial Reference Frame (SRF).
The Solar Magnetic Spatial Reference Frame also known as Solar Geomagnetic (SG), is based on a Cartesian coordinate system with 3 orthogonal axes and an origin at the Object Reference Model/Earth Reference Model (ORM/ERM) mass-center as defined by the World Geodetic System (WGS) 1984 ellipsoid). The Z axis is defined as coincident with the geomagnetic (magnetic dipole) axis and is positive towards the north. The Y axis is defined as perpendicular to the Earth-Sun line (positive towards dusk) and lies in the Geomagnetic Equatorial plane. The X axis is defined as orthogonal to the other axes and lying in the Geomagnetic Equatorial plane, (although it does not necessarily point to the Sun), so as to form a right-handed orthogonal set.
Locations are defined as {lon, lat, r} triplets from the origin (ORM/ERM mass-center). Longitude (lon) is defined as the geocentric angle in the Geomagnetic Equatorial plane from the Geomagnetic meridian containing the Earth-Sun line to the Geomagnetic meridian containing the radius vector (and positive towards the East). Latitude (lat) is defined as the geocentric angle between the radius vector and the Geomagnetic Equatorial plane; it is positive towards the north. R is the magnitude of the radius vector.
See the SEDRIS Spatial Reference Model (SRM) for additional details.
SM provides a convenient system for ordering data controlled more strongly by the Earth's dipole field than by solar wind. It has been used for representing magnetopause cross-sections and magnetospheric magnetic fields.
| SE_FLOAT64 | longitude; | (notes) |
|---|---|---|
| SE_FLOAT64 | latitude; | (notes) |
| SE_FLOAT64 | radius; | (notes) |
the center point for the LOD test
in degrees
in degrees
in meters