Orbit2Sp3Format
Writes orbits to SP3 format.
SP3 orbits are usually given in the terrestrial reference frame (TRF), so providing earthRotation automatically rotates the orbits from the celestial reference frame (CRF) to the TRF. Since SP3 orbits often use the center of Earth as a reference, a correction from center of mass to center of Earth can be applied to the orbits by providing gravityfield (e.g. ocean tides).
See also Sp3Format2Orbit.
Name | Type | Annotation |
---|---|---|
outputfile | filename | |
satellite | sequence | |
inputfileOrbit | filename | |
inputfileClock | filename | |
inputfileCovariance | filename | |
identifier | string | 3 characters (e.g. GNSS PRN: G01) |
orbitAccuracy | double | [m] used for accuracy codes in header (0 = unknown) |
earthRotation | earthRotation | rotate data into Earth-fixed frame |
gravityfield | gravityfield | degree 1 fluid mantle for CM2CE correction (SP3 orbits should be in center of Earth) |
comment | string | comment lines (77 char max) |
firstLine | string | Text for first line e.g: u+U IGb14 KIN ITSG |
writeVelocity | boolean | write velocity in addition to position |
useSp3kFormat | boolean | use the extended sp3k format |