Convert direction cosine matrix to geodetic latitude and longitude
The Direction Cosine Matrix ECEF to NED to Latitude and Longitude block converts a 3-by-3 direction cosine matrix (DCM) into geodetic latitude and longitude. The DCM matrix performs the coordinate transformation of a vector in Earth-centered Earth-fixed (ECEF) axes (ox0, oy0, oz0) into a vector in north-east-down (NED) axes (ox2, oy2, oz2). The order of the axis rotations required to bring this about is:
A rotation about oz0 through the longitude (ι) to axes (ox1, oy1, oz1)
A rotation about oy1 through the geodetic latitude (μ) to axes (ox2, oy2, oz2)
Combining the two axis transformation matrices defines the following DCM.
To determine geodetic latitude and longitude from the DCM, the following equations are used:
|3-by-3 direction cosine matrix||Transforms ECEF vectors to NED vectors.|
|2-by-1 vector||Contains the geodetic latitude and longitude, in degrees.|
This implementation generates a geodetic latitude that lies between ±90 degrees, and longitude that lies between ±180 degrees.
The implementation of the ECEF coordinate system assumes that the origin is at the center of the planet, the x-axis intersects the Greenwich meridian and the equator, the z-axis is the mean spin axis of the planet, positive to the north, and the y-axis completes the right-hand system.
Stevens, B. L., and F. L. Lewis, Aircraft Control and Simulation, John Wiley & Sons, New York, 1992.
Zipfel, P. H., Modeling and Simulation of Aerospace Vehicle Dynamics, AIAA Education Series, Reston, Virginia, 2000.
“Atmospheric and Space Flight Vehicle Coordinate Systems,” ANSI/AIAA R-004-1992.