Path: Orbit/OrbitManeuver
% Solve the Linear Terminal Velocity Constraint problem. dr/dt = c1 + c2*vH where vH is the horizontal velocity and c1 and c2 are constants Since version 2. -------------------------------------------------------------------------- Form: v0 = LTVCon( r0, r, c1, c2, orbitType, mu ) -------------------------------------------------------------------------- ------ Inputs ------ r0 (3,1) Initial position vector r (3,1) Final position vector c1 (1,1) Constant c2 (1,1) Constant orbitType (1,:) 'direct' or 'retrograde' mu (1,1) Gravitational parameter (default is the earth) ------- Outputs ------- v0 (1,1) Initial velocity -------------------------------------------------------------------------- References: Bond, V.R. and M. C. Allman, "Modern Astrodynamics", Princeton University Press, 1996, pp. 88-90 --------------------------------------------------------------------------
Math: Linear/Mag Orbit: OrbitMechanics/TARes
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