Periapsis radius and velocity at infinity to semi major axis and eccentricity (hyperbolic orbits) - DEPRECATED
[sma, ecc] = CL_op_rpvinf2ae(rp, vinf [[, mu]])
This function is deprecated.
Replacement function: CL_kp_apsConvert
Use 'CL_kp_apsConvert("rp", rp, "vinf", vinf, ["sma", "ecc"])' instead of 'CL_op_rpvinf2ae(rp, vinf)'.
Computes semi major axis and eccentricity from periapsis radius and velocity at infinity (hyperbolic orbits only).
Nota: The velocity at infinity vinf must be greater than zero
Periapsis radius [m] (1xN or 1x1)
Velocity at infinity [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