This function converts cartesian tridimensional geodentric coordinates into
geodetic coordinates.
INPUT ARGUMENTS:
- X is a column vector containing the X geocentric coordinate, in meters.
- Y is a column vector containing the Y geocentric coordinate, in meters.
- Z is a column vector containing the Z geocentric coordinate, in meters.
- a is a scalar containing the semi-major axis of the ellipsoid, in meters.
- e2 is a scalar containing the squared first eccentricity of the ellipsoid.
OUTPUT ARGUMENTS:
- lon is a column vector containing the geodetic longitude, in radians.
- lat is a column vector containing the geodetic latitude, in radians.
- h is a column vector containing the ellipsoidal height, in meters
The coordinate vectors X, Y and Z must be all scalars or
all column vectors (of the same size).
See also: _op_geod2geoc.