Periapsis radius and velocity at periapsis to semi major axis and eccentricity
[sma,ecc] = CL_op_rpvp2ae(rp,vp [,mu])
Computes semi major axis and eccentricity from periapsis radius and velocity at periapsis (elliptic and hyperbolic orbits).
Note:
The results are correct even if (rp,vp) are data that actually correspond to the apoapsis.
Periapsis radius [m] (1xN or 1x1)
Velocity at periapsis [m/s] (1xN or 1x1)
(optional) Gravitational constant [m^3/s^2] (default value is %CL_mu)
Semi major axis [m] (1xN)
Eccentricity (1xN)
CNES - DCT/SB