Apoapsis/periapsis radius to Apoapsis/periapsis velocity (elliptic orbits) - DEPRECATED
[v1, v2] = CL_op_rarp2vavp(r1, r2 [, mu])
This function is deprecated.
Replacement function: CL_kp_apsConvert
Use 'CL_kp_apsConvert("ra", ra, "rp", rp, ["va", "vp"])' instead of 'CL_op_rarp2vavp(ra, rp)'.
Computes velocity at apoapsis and periapsis from apoapsis and periapsis radii (elliptic orbits only).
Note:
[v1, v2] = CL_op_rarp2vavp(r1, r2, mu) gives the same results (same v1 and v2) as [v2, v1] = CL_op_rarp2vavp(r2, r1, mu)
Radius at position 1 (apoapsis or periapsis). [m] (1xN or 1x1)
Radius at position 2 (periapsis or apoapsis). [m] (1xN or 1x1)
(optional) Gravitational constant. Default: %CL_mu. [m^3/s^2] (1x1)
velocity at position 1. [m/s] (1xN)
velocity at position 2. [m/s] (1xN)
CNES - DCT/SB