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 can be scalars, vectors
or 2D matrices. lon, lat, and h will be according to the
input dimensions.
See also: _op_geod2geoc.