コード例 #1
0
            vz=-2.17699042180559e-5)  # Uranus
rebound.add(m=1. / 19314.,
            x=-3.01777243405203e+1,
            y=+1.91155314998064e+0,
            z=-1.53887595621042e-1,
            vx=-2.17471785045538e-4,
            vy=-3.11361111025884e-3,
            vz=+3.58344705491441e-5)  # Neptune
rebound.add(m=0,
            x=-2.13858977531573e+1,
            y=+3.20719104739886e+1,
            z=+2.49245689556096e+0,
            vx=-1.76936577252484e-3,
            vy=-2.06720938381724e-3,
            vz=+6.58091931493844e-4)  # Pluto

# Set the center of momentum to be at the origin
rebound.move_to_com()

# timestep counter
steps = 0
# Integrate until t=1e6 (unit of time in this example is days)
while rebound.t < 1e6:
    rebound.step()
    steps += 1
    # Print particle positions every 100 timesteps
    if steps % 100 == 0:
        for p in rebound.particles:
            #     time       x    y    z
            print(rebound.t, p.x, p.y, p.z)
コード例 #2
0
ファイル: problem.py プロジェクト: tasha-urbancic/rebound
def simulation(par):
    integrator = par
    rebound.reset()
    k = 0.01720209895    
    G = k*k
    rebound.set_G(G)     
    rebound.set_dt(dt)
    rebound.set_integrator(integrator)

    rebound.add_particle(m=1.00000597682, x=-4.06428567034226e-3, y=-6.08813756435987e-3, z=-1.66162304225834e-6, vx=+6.69048890636161e-6, vy=-6.33922479583593e-6, vz=-3.13202145590767e-9)   # Sun
    rebound.add_particle(m=1./1047.355,   x=+3.40546614227466e+0, y=+3.62978190075864e+0, z=+3.42386261766577e-2, vx=-5.59797969310664e-3, vy=+5.51815399480116e-3, vz=-2.66711392865591e-6)   # Jupiter
#    rebound.add_particle(m=1./3501.6,     x=+6.60801554403466e+0, y=+6.38084674585064e+0, z=-1.36145963724542e-1, vx=-4.17354020307064e-3, vy=+3.99723751748116e-3, vz=+1.67206320571441e-5)   # Saturn
#    rebound.add_particle(m=1./22869.,     x=+1.11636331405597e+1, y=+1.60373479057256e+1, z=+3.61783279369958e-1, vx=-3.25884806151064e-3, vy=+2.06438412905916e-3, vz=-2.17699042180559e-5)   # Uranus
#    rebound.add_particle(m=1./19314.,     x=-3.01777243405203e+1, y=+1.91155314998064e+0, z=-1.53887595621042e-1, vx=-2.17471785045538e-4, vy=-3.11361111025884e-3, vz=+3.58344705491441e-5)   # Neptune
#    rebound.add_particle(m=0,             x=-2.13858977531573e+1, y=+3.20719104739886e+1, z=+2.49245689556096e+0, vx=-1.76936577252484e-3, vy=-2.06720938381724e-3, vz=+6.58091931493844e-4)   # Pluto
    N = rebound.get_N()

    def move_to_heliocentric():
        particles = rebound.get_particles()
        
        for i in xrange(1,N):
            particles[i].x -= particles[0].x
            particles[i].y -= particles[0].y
            particles[i].z -= particles[0].z
            particles[i].vx -= particles[0].vx
            particles[i].vy -= particles[0].vy
            particles[i].vz -= particles[0].vz
        particles[0].x  = 0.
        particles[0].y  = 0. 
        particles[0].z  = 0. 
        particles[0].vx = 0. 
        particles[0].vy = 0. 
        particles[0].vz = 0. 


    def energy():
        if integrator=="wh":
            rebound.move_to_center_of_momentum()
        particles = rebound.get_particles()
        E_kin = 0.
        E_pot = 0.
        for i in xrange(N):
            E_kin += 0.5*particles[i].m*(particles[i].vx*particles[i].vx + particles[i].vy*particles[i].vy + particles[i].vz*particles[i].vz)
            for j in xrange(i+1,N):
                dx = particles[i].x-particles[j].x
                dy = particles[i].y-particles[j].y
                dz = particles[i].z-particles[j].z
                r2 = dx*dx + dy*dy + dz*dz
                E_pot -= G*particles[i].m*particles[j].m/np.sqrt(r2)
        if integrator=="wh":
            move_to_heliocentric()
        return E_kin+E_pot

    rebound.move_to_center_of_momentum()

    es = []

    ei = energy()
    for time in xrange(Nsteps):
        rebound.step()
        ef = energy()
        e = (ei-ef)
        es.append(e)
        ei = ef

    es = np.array(es)
    print integrator + " done."
    return [es]
コード例 #3
0
ファイル: problem.py プロジェクト: stefano-meschiari/rebound
def simulation(par):
    integrator, mass = par
    rebound.reset()
    mass = pow(10.,mass)
    k = 0.01720209895    
    G = k*k
    rebound.G = G     
    rebound.dt = 0.
    rebound.integrator = integrator

    rebound.add(m=1.00000597682, x=-4.06428567034226e-3, y=-6.08813756435987e-3, z=-1.66162304225834e-6, vx=+6.69048890636161e-6, vy=-6.33922479583593e-6, vz=-3.13202145590767e-9)   # Sun
    rebound.add(m=mass,   x=+3.40546614227466e+0, y=+3.62978190075864e+0, z=+3.42386261766577e-2, vx=-5.59797969310664e-3, vy=+5.51815399480116e-3, vz=-2.66711392865591e-6)   # Jupiter
    rebound.add(m=mass,     x=+6.60801554403466e+0, y=+6.38084674585064e+0, z=-1.36145963724542e-1, vx=-4.17354020307064e-3, vy=+3.99723751748116e-3, vz=+1.67206320571441e-5)   # Saturn
    rebound.add(m=mass,     x=+1.11636331405597e+1, y=+1.60373479057256e+1, z=+3.61783279369958e-1, vx=-3.25884806151064e-3, vy=+2.06438412905916e-3, vz=-2.17699042180559e-5)   # Uranus
    rebound.add(m=mass,     x=-3.01777243405203e+1, y=+1.91155314998064e+0, z=-1.53887595621042e-1, vx=-2.17471785045538e-4, vy=-3.11361111025884e-3, vz=+3.58344705491441e-5)   # Neptune
    N = rebound.N

    def move_to_heliocentric():
        particles = rebound.particles
        
        for i in xrange(1,N):
            particles[i].x -= particles[0].x
            particles[i].y -= particles[0].y
            particles[i].z -= particles[0].z
            particles[i].vx -= particles[0].vx
            particles[i].vy -= particles[0].vy
            particles[i].vz -= particles[0].vz
        particles[0].x  = 0.
        particles[0].y  = 0. 
        particles[0].z  = 0. 
        particles[0].vx = 0. 
        particles[0].vy = 0. 
        particles[0].vz = 0. 


    def energy():
        if integrator=="wh":
            rebound.move_to_com()
        particles = rebound.particles
        E_kin = 0.
        E_pot = 0.
        for i in xrange(N):
            E_kin += 0.5*particles[i].m*(particles[i].vx*particles[i].vx + particles[i].vy*particles[i].vy + particles[i].vz*particles[i].vz)
            for j in xrange(i+1,N):
                dx = particles[i].x-particles[j].x
                dy = particles[i].y-particles[j].y
                dz = particles[i].z-particles[j].z
                r2 = dx*dx + dy*dy + dz*dz
                E_pot -= G*particles[i].m*particles[j].m/np.sqrt(r2)
        if integrator=="wh":
            move_to_heliocentric()
        return E_kin+E_pot

    rebound.move_to_com()
    ei = energy()

    es = 1e-20

    for s in xrange(1000):
        rebound.step()
        ef = energy()
        e = np.fabs((ei-ef)/ei)
        es = max(es,e)

    return es
コード例 #4
0
ファイル: problem.py プロジェクト: dsspiegel/rebound
k = 0.01720209895       # Gaussian constant 
rebound.set_G(k*k)      # Gravitational constant

# Setup particles (data taken from NASA Horizons)
# This could also be easily read in from a file.
rebound.particle_add( Particle( m=1.00000597682, x=-4.06428567034226e-3, y=-6.08813756435987e-3, z=-1.66162304225834e-6, vx=+6.69048890636161e-6, vy=-6.33922479583593e-6, vz=-3.13202145590767e-9) )  # Sun
rebound.particle_add( Particle( m=1./1047.355,   x=+3.40546614227466e+0, y=+3.62978190075864e+0, z=+3.42386261766577e-2, vx=-5.59797969310664e-3, vy=+5.51815399480116e-3, vz=-2.66711392865591e-6) )  # Jupiter
rebound.particle_add( Particle( m=1./3501.6,     x=+6.60801554403466e+0, y=+6.38084674585064e+0, z=-1.36145963724542e-1, vx=-4.17354020307064e-3, vy=+3.99723751748116e-3, vz=+1.67206320571441e-5) )  # Saturn
rebound.particle_add( Particle( m=1./22869.,     x=+1.11636331405597e+1, y=+1.60373479057256e+1, z=+3.61783279369958e-1, vx=-3.25884806151064e-3, vy=+2.06438412905916e-3, vz=-2.17699042180559e-5) )  # Uranus
rebound.particle_add( Particle( m=1./19314.,     x=-3.01777243405203e+1, y=+1.91155314998064e+0, z=-1.53887595621042e-1, vx=-2.17471785045538e-4, vy=-3.11361111025884e-3, vz=+3.58344705491441e-5) )  # Neptune
rebound.particle_add( Particle( m=0,             x=-2.13858977531573e+1, y=+3.20719104739886e+1, z=+2.49245689556096e+0, vx=-1.76936577252484e-3, vy=-2.06720938381724e-3, vz=+6.58091931493844e-4) )  # Pluto

# Set the center of momentum to be at the origin
rebound.move_to_center_of_momentum()

# Get the particle data
# Note: this is a pointer and will automatically update as the simulation progresses
particles = rebound.particles_get()
# timestep counter
steps = 0 
# Integrate until t=1e6 (unit of time in this example is days)
while rebound.get_t()<1e6:
    rebound.step()
    steps += 1
    # Print particle positions every 100 timesteps
    if steps%100==0:
        for i in range(rebound.get_N()):
            #     time             particle id   x               y               z 
            print rebound.get_t(), i,            particles[i].x, particles[i].y, particles[i].z

コード例 #5
0
def simulation(par):
    integrator, mass = par
    rebound.reset()
    mass = pow(10., mass)
    k = 0.01720209895
    G = k * k
    rebound.G = G
    rebound.dt = 0.
    rebound.integrator = integrator

    rebound.add(m=1.00000597682,
                x=-4.06428567034226e-3,
                y=-6.08813756435987e-3,
                z=-1.66162304225834e-6,
                vx=+6.69048890636161e-6,
                vy=-6.33922479583593e-6,
                vz=-3.13202145590767e-9)  # Sun
    rebound.add(m=mass,
                x=+3.40546614227466e+0,
                y=+3.62978190075864e+0,
                z=+3.42386261766577e-2,
                vx=-5.59797969310664e-3,
                vy=+5.51815399480116e-3,
                vz=-2.66711392865591e-6)  # Jupiter
    rebound.add(m=mass,
                x=+6.60801554403466e+0,
                y=+6.38084674585064e+0,
                z=-1.36145963724542e-1,
                vx=-4.17354020307064e-3,
                vy=+3.99723751748116e-3,
                vz=+1.67206320571441e-5)  # Saturn
    rebound.add(m=mass,
                x=+1.11636331405597e+1,
                y=+1.60373479057256e+1,
                z=+3.61783279369958e-1,
                vx=-3.25884806151064e-3,
                vy=+2.06438412905916e-3,
                vz=-2.17699042180559e-5)  # Uranus
    rebound.add(m=mass,
                x=-3.01777243405203e+1,
                y=+1.91155314998064e+0,
                z=-1.53887595621042e-1,
                vx=-2.17471785045538e-4,
                vy=-3.11361111025884e-3,
                vz=+3.58344705491441e-5)  # Neptune
    N = rebound.N

    def move_to_heliocentric():
        particles = rebound.particles

        for i in xrange(1, N):
            particles[i].x -= particles[0].x
            particles[i].y -= particles[0].y
            particles[i].z -= particles[0].z
            particles[i].vx -= particles[0].vx
            particles[i].vy -= particles[0].vy
            particles[i].vz -= particles[0].vz
        particles[0].x = 0.
        particles[0].y = 0.
        particles[0].z = 0.
        particles[0].vx = 0.
        particles[0].vy = 0.
        particles[0].vz = 0.

    def energy():
        if integrator == "wh":
            rebound.move_to_com()
        particles = rebound.particles
        E_kin = 0.
        E_pot = 0.
        for i in xrange(N):
            E_kin += 0.5 * particles[i].m * (
                particles[i].vx * particles[i].vx + particles[i].vy *
                particles[i].vy + particles[i].vz * particles[i].vz)
            for j in xrange(i + 1, N):
                dx = particles[i].x - particles[j].x
                dy = particles[i].y - particles[j].y
                dz = particles[i].z - particles[j].z
                r2 = dx * dx + dy * dy + dz * dz
                E_pot -= G * particles[i].m * particles[j].m / np.sqrt(r2)
        if integrator == "wh":
            move_to_heliocentric()
        return E_kin + E_pot

    rebound.move_to_com()
    ei = energy()

    es = 1e-20

    for s in xrange(1000):
        rebound.step()
        ef = energy()
        e = np.fabs((ei - ef) / ei)
        es = max(es, e)

    return es