CL_man_hohmann — Delta V for a hohmann transfer
[delta_v,dv1,dv2,anv1,anv2] = CL_man_hohmann(ai,af,[mu])
The output delta_v is the sum of the |delta-v| required (dv1 + dv2).
Velocity increments are given in spherical coordinates in the QSW frame : first parameter lambda is the in plane component (pi ~= towards planet and pi/2 = along velocity) second parameter phi is the out of plane component, positive towards the kinetic moment, third parameter is the norm
radius of initial circular orbit (semi major axis). [m] (1xN)
radius of final cirular orbit (semi major axis). [m] (1xN)
(optionnal) gravitational constant. [m^3/s^2] (default value is %CL_mu)
total delta-v required = |dv1| + |dv2|. [m/s] (1xN)
First velocity increment, given in spherical coordinates in the QSW frame [lambda;phi;|dv|] [rad,rad,m/s] (3xN)
Second velocity increment, given in spherical coordinates in the QSW frame [lambda;phi;|dv|] [rad,rad,m/s] (3xN)
true anomaly of first impulse : as the initial orbit is circular, anv1 is set to 0 arbitrarily (1xN)
true anomaly of second impulse (either 0 or %pi) [rad] (1xN)