Bi-elliptic transfer - DEPRECATED
[delta_v,dv1,dv2,dv3,anv1,anv2,anv3]=CL_man_biElliptic(ai,af,rt [,mu])
This function is deprecated.
Replacement function: CL_man_dvBiElliptic
Computes the maneuvers of a bi-elliptical transfer from a circular orbit with semi-major axis ai to a circular orbit with semi-major axis af.
The apogee radius of the elliptical transfer orbit is rt.
delta-v is the sum of the norms of the velocity increments.
Velocity increments are expressed in spherical coordinates in the "qsw" local orbital frame.
Semi-major axis of initial circular orbit [m] (1xN or 1x1)
Semi-major axis of final circular orbit [m] (1xN or 1x1)
Radius at the position of the second maneuver [m] (1xN or 1x1)
(optional) Gravitational constant [m^3/s^2] (default value is %CL_mu)
Total |delta-V| (=|dv1|+|dv2|+|dv3]) [m/s] (1xN)
First delta-V, in spherical coordinates in the "qsw" frame [lambda;phi;|dv|] [rad,rad,m/s] (3xN)
Second delta-V, in spherical coordinates in the "qsw" frame [lambda;phi;|dv|] [rad,rad,m/s] (3xN)
Third delta-V, in spherical coordinates in the "qsw" frame [lambda;phi;|dv|] [rad,rad,m/s] (3xN)
True anomaly at the position of the 1st maneuver: initial orbit is circular so this is an arbitrary value of 0 (1xN)
True anomaly at the position of the 2nd maneuver (either 0 or pi) [rad] (1xN)
True anomaly at the position of the 3rd maneuver (either 0 or pi) [rad] (1xN)
CNES - DCT/SB
1) Orbital Mechanics for engineering students, H D Curtis, Chapter 6