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CL_man_dvSma

Change of semi-major axis (elliptical orbits)

Calling Sequence

[deltav,dv,anv] = CL_man_dvSma(ai,ei,af [,posman,mu])
man = CL_man_dvSma(ai,ei,af [,posman,mu], res="s")

Description

Parameters

ai :

Initial semi major axis [m] (1xN or 1x1)

ei :

Initial eccentricity (1xN or 1x1)

af :

Final semi major axis [m] (1xN or 1x1)

posman:

(optional) Flag specifying the position of the maneuver: 0 or "per" -> periapsis, 1 or "apo" -> apoapsis. Default is at the periapsis. (1xN or 1x1)

mu :

(optional) Gravitational constant. [m^3/s^2] (default value is %CL_mu)

res :

(string, optional) Type of output: "d" or "s" for . Default is "d".

deltav :

Norm of velocity increment. [m/s] (1xN)

dv :

Velocity increment (in cartesian coordinates) in the "qsw" local frame [m/s] (3xN)

anv :

True anomaly at the position of maneuver [rad] (1xN)

man :

Structure containing all the output data.

Authors

See also

Examples

ai = 7200.e3;
af = 7000.e3;
ei = 0.1;
[deltav,dv,anv] = CL_man_dvSma(ai,ei,af)

// Check results :
kep = [ai ; ei ; %pi/2 ; 0 ; 0 ; anv]; // mean anomaly = true anomaly
CL_man_applyDvKep(kep,dv)

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