Exemple #1
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/// Implementation of the constraint function.
void earth_planet::compute_constraints_impl(constraint_vector &c, const decision_vector &x) const
{
	// We decode the decision vector into a multiple fly-by trajectory
	trajectory.init_from_full_vector(x.begin(),x.end(),encoding);

	// We evaluate the state mismatch at the mid-point. And we use astronomical units to scale them
	trajectory.evaluate_all_mismatch_con(c.begin(), c.begin() + 7);
	for (int i=0; i<3; ++i) c[i]/=ASTRO_AU;
	for (int i=3; i<6; ++i) c[i]/=ASTRO_EARTH_VELOCITY;

	// We evaluate the constraints on the throttles writing on the 7th mismatch constrant (mass is off)
	trajectory.get_leg(0).get_throttles_con(c.begin() + 6, c.begin() + 6 + n_segments);

	// We evaluate the constraint on the initial launch velocity
	c[6 + n_segments] = (trajectory.evaluate_leg_vinf2_i(0) - vmax*vmax) / ASTRO_EARTH_VELOCITY / ASTRO_EARTH_VELOCITY;

	// We evaluate the linear constraint on the epochs (tf > ti)
	c[7 + n_segments] = trajectory.get_leg(0).get_t_i().mjd2000() - trajectory.get_leg(0).get_t_f().mjd2000();
}
Exemple #2
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/// Implementation of the constraint function.
void gtoc5_rendezvous::compute_constraints_impl(constraint_vector &c, const decision_vector &x) const
{
	using namespace kep_toolbox;
	// We set the leg.
	const epoch epoch_i(x[0],epoch::MJD), epoch_f(x[1] + x[0],epoch::MJD);
	array3D v0, r0, vf, rf;
	m_source.eph(epoch_i,r0,v0);
	m_target.eph(epoch_f,rf,vf);
	m_leg.set_leg(epoch_i,sc_state(r0,v0,m_leg.get_spacecraft().get_mass()),x.begin() + 3, x.end(),epoch_f,sc_state(rf,vf,x[2]),ASTRO_MU_SUN);

	// We evaluate the state mismatch at the mid-point. And we use astronomical units to scale them
	m_leg.get_mismatch_con(c.begin(), c.begin() + 7);
	for (int i=0; i<3; ++i) c[i]/=ASTRO_AU;
	for (int i=3; i<6; ++i) c[i]/=ASTRO_EARTH_VELOCITY;
	c[6] /= m_leg.get_spacecraft().get_mass();
	// We evaluate the constraints on the throttles writing on the 7th mismatch constrant (mass is off)
	m_leg.get_throttles_con(c.begin() + 7, c.begin() + 7 + m_n_segments);
}
Exemple #3
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std::string gtoc5_rendezvous::pretty(const decision_vector &x) const
{
	using namespace kep_toolbox;
	// We set the leg.
	const epoch epoch_i(x[0],epoch::MJD), epoch_f(x[1] + x[0],epoch::MJD);
	array3D v0, r0, vf, rf;
	m_source.eph(epoch_i,r0,v0);
	m_target.eph(epoch_f,rf,vf);
	m_leg.set_leg(epoch_i,sc_state(r0,v0,m_leg.get_spacecraft().get_mass()),x.begin() + 3, x.end(),epoch_f,sc_state(rf,vf,x[2]),ASTRO_MU_SUN);

	std::ostringstream oss;
	oss << m_leg << '\n' << m_source << '\n' << m_target << '\n';
	return oss.str();
}
Exemple #4
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std::string gtoc5_launch::pretty(const decision_vector &x) const
{
	using namespace kep_toolbox;
	// 1 - We set the leg.
	const epoch epoch_i(x[0],epoch::MJD), epoch_f(x[1] + x[0],epoch::MJD);
	array3D v0, r0, vf, rf;
	m_earth.get_eph(epoch_i,r0,v0);
	m_target.get_eph(epoch_f,rf,vf);

	v0[0] += x[2];
	v0[1] += x[3];
	v0[2] += x[4];
	m_leg.set_leg(epoch_i,sc_state(r0,v0,m_leg.get_spacecraft().get_mass()),x.begin() + 6, x.end(),epoch_f,sc_state(rf,vf,x[5]),ASTRO_MU_SUN);

	std::ostringstream oss;
	oss << m_leg << '\n' << m_earth << '\n' << m_target << '\n';
	return oss.str();
}
Exemple #5
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    void tsp_vrplc::compute_constraints_impl(constraint_vector &c, const decision_vector& x) const 
    {
        decision_vector::size_type n_cities = get_n_cities();

        switch( get_encoding() ) 
        {
            case FULL:
            {
                // 1 - We set the equality constraints
                for (size_t i = 0; i < n_cities; i++) {
                    c[i] = 0;
                    c[i+n_cities] = 0;
                    for (size_t j = 0; j < n_cities; j++) 
                    {
                        if(i==j) continue; // ignoring main diagonal
                        decision_vector::size_type rows = compute_idx(i, j, n_cities);
                        decision_vector::size_type cols = compute_idx(j, i, n_cities);
                        c[i] += x[rows];
                        c[i+n_cities] += x[cols];
                    }
                    c[i] = c[i]-1;
                    c[i+n_cities] = c[i+n_cities]-1;
                }

                //2 - We set the inequality constraints
                //2.1 - First we compute the uj (see http://en.wikipedia.org/wiki/Travelling_salesman_problem#Integer_linear_programming_formulation)
                //      we start always out tour from the first city, without loosing generality
                size_t next_city = 0,current_city = 0;
                std::vector<int> u(n_cities);
                for (size_t i = 0; i < n_cities; i++) 
                {
                    u[current_city] = i+1;
                    for (size_t j = 0; j < n_cities; j++) 
                    {
                        if (current_city==j) continue;
                        if (x[compute_idx(current_city, j, n_cities)] == 1) 
                        {
                            next_city = j;
                            break;
                        }
                    }
                    current_city = next_city;
                }
                int count=0;
                for (size_t i = 1; i < n_cities; i++) {
                    for (size_t j = 1; j < n_cities; j++) 
                    {
                        if (i==j) continue;
                        c[2*n_cities+count] = u[i]-u[j] + (n_cities+1) * x[compute_idx(i, j, n_cities)] - n_cities;
                        count++;
                    }
                }
                break;
            }
            case RANDOMKEYS:
                break;
            case CITIES:
            {
                std::vector<population::size_type> range(n_cities);
                for (std::vector<population::size_type>::size_type i=0; i<range.size(); ++i) 
                {
                    range[i]=i;
                }
                c[0] = !std::is_permutation(x.begin(),x.end(),range.begin());
                break;
            }
        }
        return;
    }
Exemple #6
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/// Implementation of the objective function.
void earth_planet::objfun_impl(fitness_vector &f, const decision_vector &x) const
{
	trajectory.init_from_full_vector(x.begin(),x.end(),encoding);
	f[0] = trajectory.get_leg(0).evaluate_dv() / 1000;
}