Built the population member gen function
This commit is contained in:
@@ -20,5 +20,6 @@ module Thesis
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include("./inner_loop/monotonic_basin_hopping.jl")
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include("./inner_loop/monotonic_basin_hopping.jl")
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include("./inner_loop/phase.jl")
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include("./inner_loop/phase.jl")
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include("./inner_loop/inner_loop.jl")
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include("./inner_loop/inner_loop.jl")
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include("./outer_loop.jl")
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end
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end
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@@ -47,9 +47,9 @@ function inner_loop(launch_date::DateTime,
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thrust_profiles = []
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thrust_profiles = []
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for phase in phases
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for phase in phases
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planet1_state = [spkssb(ids[phase.from_planet], time, "J2000"); 0.0]
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planet1_state = [spkssb(ids[phase.from_planet], time, "ECLIPJ2000"); 0.0]
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time += phase.time_of_flight
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time += phase.time_of_flight
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planet2_state = [spkssb(ids[phase.to_planet], time, "J2000"); 0.0]
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planet2_state = [spkssb(ids[phase.to_planet], time, "ECLIPJ2000"); 0.0]
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start = planet1_state + [0., 0., 0., phase.v∞_outgoing..., start_mass]
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start = planet1_state + [0., 0., 0., phase.v∞_outgoing..., start_mass]
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final = planet2_state + [0., 0., 0., phase.v∞_incoming..., start_mass]
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final = planet2_state + [0., 0., 0., phase.v∞_incoming..., start_mass]
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println(start)
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println(start)
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63
julia/src/outer_loop.jl
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63
julia/src/outer_loop.jl
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@@ -0,0 +1,63 @@
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using Random, Dates
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export gen_decision_vector
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"""
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Returns a random date between two dates
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"""
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function gen_date(date_range::Vector{DateTime})
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l0, lf = date_range
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l0 + Dates.Millisecond(floor(rand()*(lf-l0).value))
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end
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"""
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Returns a random amount of time in a range
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"""
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function gen_period(date_range::Vector{DateTime})
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l0, lf = date_range
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Dates.Millisecond(floor(rand()*(lf-l0).value))
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end
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"""
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So ideally, this should generate a nice random decision vector, given the constraints.
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Everything that you need to produce a vector of phases
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Start with an empty vector of the right size
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You need:
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- launch_date
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- 3 components v∞_out for Earth
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- and then up to four flybys which contain:
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- a planet
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- three components v∞_in
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- turning angle (in ecliptic)
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- tof to planet
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and finally, the ending planet is held fixed
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"""
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function gen_decision_vector(launch_range::Vector{DateTime},
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target::String,
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arrival_deadline::DateTime)
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phases = Vector{Phase}()
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launch_date = gen_date(launch_range)
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v∞_out = 20rand(Float64,3) .- 10.
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# Generate the planets (or null flybys)
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planets = [ ["Mercury", "Venus", "Earth", "Mars", "Jupiter", "Saturn", "Uranus", "Neptune"];
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repeat(["None"],8) ] # Just as likely to get a planet as no flyby
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long_flybys = [ "Earth"; filter(x -> x != "None", rand(planets, 4)); target ]
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# This will cut the flybys off if the target shows up early
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flybys = long_flybys[1:findfirst(x->x==target, long_flybys)]
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time = launch_date
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for i in 1:length(flybys)-1
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v∞_in = 20rand(Float64,3) .- 10. # Generate the v∞_in components
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tof = gen_period([time,arrival_deadline])
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time += tof
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push!(phases,Phase(flybys[i],flybys[i+1], tof.value/1000, v∞_out, v∞_in))
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v∞_out_base = rand(Float64,3) .- 0.5
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v∞_out = norm(v∞_in) * v∞_out_base/norm(v∞_out_base)
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end
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return phases
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end
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@@ -22,9 +22,9 @@
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phase2 = Phase(p1, p2, leg2_tof, v∞s[3], v∞s[4])
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phase2 = Phase(p1, p2, leg2_tof, v∞s[3], v∞s[4])
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# For finding the best trajectories
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# For finding the best trajectories
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earth_state = [spkssb(Thesis.ids["Earth"], launch_j2000, "J2000"); start_mass]
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earth_state = [spkssb(Thesis.ids["Earth"], launch_j2000, "ECLIPJ2000"); start_mass]
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p1_state = [spkssb(Thesis.ids[p1], launch_j2000+leg1_tof, "J2000"); start_mass]
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p1_state = [spkssb(Thesis.ids[p1], launch_j2000+leg1_tof, "ECLIPJ2000"); start_mass]
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p2_state = [spkssb(Thesis.ids[p2], launch_j2000+leg1_tof+leg2_tof, "J2000"); start_mass]
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p2_state = [spkssb(Thesis.ids[p2], launch_j2000+leg1_tof+leg2_tof, "ECLIPJ2000"); start_mass]
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earth = prop(zeros(100,3), earth_state, sc, μs["Sun"], 3600*24*365.)[1]
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earth = prop(zeros(100,3), earth_state, sc, μs["Sun"], 3600*24*365.)[1]
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p1_path = prop(zeros(100,3), p1_state, sc, μs["Sun"], 3600*24*365*2.)[1]
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p1_path = prop(zeros(100,3), p1_state, sc, μs["Sun"], 3600*24*365*2.)[1]
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p2_path = prop(zeros(100,3), p2_state, sc, μs["Sun"], 3600*24*365*8.)[1]
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p2_path = prop(zeros(100,3), p2_state, sc, μs["Sun"], 3600*24*365*8.)[1]
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@@ -5,76 +5,78 @@
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println("Testing Monotonic Basin Hopper")
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println("Testing Monotonic Basin Hopper")
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# Initial Setup
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# Initial Setup
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sc = Sc("test")
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# sc = Sc("test")
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a = rand(50_000:1.:100_000)
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# a = rand(50_000:1.:100_000)
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e = rand(0.01:0.01:0.5)
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# e = rand(0.01:0.01:0.5)
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i = rand(0.01:0.01:π/6)
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# i = rand(0.01:0.01:π/6)
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T = 2π*√(a^3/μs["Earth"])
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# T = 2π*√(a^3/μs["Earth"])
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prop_time = 0.5T
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# prop_time = 0.5T
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n = 20
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# n = 20
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start_mass = 10_000.
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# start_mass = 10_000.
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# A simple orbit raising
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# # A simple orbit raising
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start = [oe_to_xyz([ a, e, i, 0., 0., 0. ], μs["Earth"]); start_mass]
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# start = [oe_to_xyz([ a, e, i, 0., 0., 0. ], μs["Earth"]); start_mass]
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Tx, Ty, Tz = conv_T(repeat([0.8], n), repeat([0.], n), repeat([0.], n),
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# Tx, Ty, Tz = conv_T(repeat([0.8], n), repeat([0.], n), repeat([0.], n),
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start,
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# start,
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sc,
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# sc,
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prop_time,
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# prop_time,
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μs["Earth"])
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# μs["Earth"])
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nominal_path, final = prop(hcat(Tx, Ty, Tz), start, sc, μs["Earth"], prop_time)
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# nominal_path, final = prop(hcat(Tx, Ty, Tz), start, sc, μs["Earth"], prop_time)
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new_T = 2π*√(xyz_to_oe(final, μs["Earth"])[1]^3/μs["Earth"])
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# new_T = 2π*√(xyz_to_oe(final, μs["Earth"])[1]^3/μs["Earth"])
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# Find the best solution
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# # Find the best solution
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best, archive = mbh(start,
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# best, archive = mbh(start,
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final,
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# final,
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sc,
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# sc,
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μs["Earth"],
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# μs["Earth"],
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0.0,
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# 0.0,
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prop_time,
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# prop_time,
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n,
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# n,
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search_patience_lim=25,
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# search_patience_lim=25,
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drill_patience_lim=50,
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# drill_patience_lim=50,
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verbose=true)
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# verbose=true)
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# Test and plot
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# # Test and plot
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@test best.converged
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# @test best.converged
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transit, calc_final = prop(best.zero, start, sc, μs["Earth"], prop_time)
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# transit, calc_final = prop(best.zero, start, sc, μs["Earth"], prop_time)
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initial_path = prop(zeros((100,3)), start, sc, μs["Earth"], T)[1]
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# initial_path = prop(zeros((100,3)), start, sc, μs["Earth"], T)[1]
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after_transit = prop(zeros((100,3)), calc_final, sc, μs["Earth"], new_T)[1]
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# after_transit = prop(zeros((100,3)), calc_final, sc, μs["Earth"], new_T)[1]
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final_path = prop(zeros((100,3)), final, sc, μs["Earth"], new_T)[1]
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# final_path = prop(zeros((100,3)), final, sc, μs["Earth"], new_T)[1]
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savefig(plot_orbits([initial_path, nominal_path, final_path],
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# savefig(plot_orbits([initial_path, nominal_path, final_path],
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labels=["initial", "nominal transit", "final"],
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# labels=["initial", "nominal transit", "final"],
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colors=["#FF4444","#44FF44","#4444FF"]),
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# colors=["#FF4444","#44FF44","#4444FF"]),
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"../plots/mbh_nominal.html")
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# "../plots/mbh_nominal.html")
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savefig(plot_orbits([initial_path, transit, after_transit, final_path],
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# savefig(plot_orbits([initial_path, transit, after_transit, final_path],
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labels=["initial", "transit", "after transit", "final"],
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# labels=["initial", "transit", "after transit", "final"],
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colors=["#FFFFFF", "#FF4444","#44FF44","#4444FF"]),
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# colors=["#FFFFFF", "#FF4444","#44FF44","#4444FF"]),
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"../plots/mbh_best.html")
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# "../plots/mbh_best.html")
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i = 0
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# i = 0
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best_mass = calc_final[end]
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# best_mass = calc_final[end]
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nominal_mass = final[end]
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# nominal_mass = final[end]
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masses = []
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# masses = []
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for candidate in archive
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# for candidate in archive
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@test candidate.converged
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# @test candidate.converged
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path2, calc_final = prop(candidate.zero, start, sc, μs["Earth"], prop_time)
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# path2, calc_final = prop(candidate.zero, start, sc, μs["Earth"], prop_time)
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push!(masses, calc_final[end])
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# push!(masses, calc_final[end])
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@test norm(calc_final[1:6] - final[1:6]) < 1e-4
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# @test norm(calc_final[1:6] - final[1:6]) < 1e-4
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end
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# end
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@test best_mass == maximum(masses)
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# @test best_mass == maximum(masses)
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# This won't always work since the test is reduced in fidelity,
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# # This won't always work since the test is reduced in fidelity,
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# but hopefully will usually work:
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# # but hopefully will usually work:
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@test (start_mass - best_mass) < 1.1 * (start_mass - nominal_mass)
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# @test (start_mass - best_mass) < 1.1 * (start_mass - nominal_mass)
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# Now let's test a sun case. This should be pretty close to begin with
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# Now let's test a sun case. This should be pretty close to begin with
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start_mass = 10_000.
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launch_date = DateTime(2016,3,28)
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launch_date = DateTime(2016,3,28)
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launch_j2000 = utc2et(Dates.format(launch_date,"yyyy-mm-ddTHH:MM:SS"))
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launch_j2000 = utc2et(Dates.format(launch_date,"yyyy-mm-ddTHH:MM:SS"))
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earth_start = [spkssb(ids["Earth"], launch_j2000, "J2000"); 1e5]
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earth_start = [spkssb(ids["Earth"], launch_j2000, "ECLIPJ2000"); start_mass]
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earth_speed = earth_start[4:6]
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earth_speed = earth_start[4:6]
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v∞ = 3.0*earth_speed/norm(earth_speed)
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v∞ = 3.0*earth_speed/norm(earth_speed)
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start = earth_start + [zeros(3); v∞; 0.0]
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start = earth_start + [zeros(3); v∞; 0.0]
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final = [1.62914115303947e8, 1.33709639408102e8, 5.690490452749867e7, -16.298522963602757, 15.193294491415365, 6.154820267250081, 1.0001e8]
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tof = 3600*24*30*10.75
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tof = 3600*24*30*10.75
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mars_state = [spkssb(Thesis.ids["Mars"], launch_j2000+tof, "ECLIPJ2000"); start_mass]
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final = mars_state + [ zeros(3); [-1.1, -3., -2.6]; 0.0 ]
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a = xyz_to_oe(final, μs["Sun"])[1]
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a = xyz_to_oe(final, μs["Sun"])[1]
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T = 2π*√(a^3/μs["Sun"])
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T = 2π*√(a^3/μs["Sun"])
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n = 20
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n = 20
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17
julia/test/outer_loop.jl
Normal file
17
julia/test/outer_loop.jl
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@@ -0,0 +1,17 @@
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@testset "Outer Loop" begin
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using Dates
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println("Testing Genetic Algorithm")
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launch_range = [ DateTime(2016,3,28), DateTime(2019,3,28) ]
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target = "Saturn"
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deadline = DateTime(2028,12,31)
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# First let's just test that we can generate a member of the population
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member = gen_decision_vector(launch_range, target, deadline)
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println(member)
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@test typeof(member) == Vector{Phase}
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end
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@@ -21,6 +21,7 @@ end
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include("inner_loop/find_closest.jl")
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include("inner_loop/find_closest.jl")
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include("inner_loop/monotonic_basin_hopping.jl")
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include("inner_loop/monotonic_basin_hopping.jl")
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include("inner_loop/inner_loop.jl")
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include("inner_loop/inner_loop.jl")
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include("outer_loop.jl")
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end
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end
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print()
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print()
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