示例#1
0
    def test_plot(self):
        # Have to enable debug stuff in Cython file.
        potential = sp.LeeSutoTriaxialNFWPotential(v_h=0.5, r_h=20., a=1., b=1., c=1., units=galactic)

        ll = np.zeros((6000,self.nstars), dtype=float)
        x,v = rewinder_likelihood(ll, -1., 6000, potential.c_instance,
                                  self.prog, self.stars, 2.5E6, 0.,
                                  1.25, self.betas, -0.3, True)

        w = np.vstack((x.T,v.T)).T
        fig = sd.plot_orbits(w, ix=0, marker=None, alpha=0.5)
        plt.show()
示例#2
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文件: mockdata.py 项目: adrn/KingKong
    def plot(self, **kwargs):
        """
        TODO:
        """
        if 'ls' not in kwargs and 'linestyle' not in kwargs:
            kwargs['linestyle'] = 'none'

        if 'marker' not in kwargs:
            kwargs['marker'] = '.'

        fig = gd.plot_orbits(self.X, **kwargs)
        return fig
示例#3
0
文件: dynamics.py 项目: abonaca/gary
def make_orbit_files(potential, w0, N_max=6, suffix="", overwrite=False,
                     force_harmonic_oscillator=False):

    orbit_filename = os.path.join(plot_path, "orbits{}.npy".format(suffix))
    units = potential.units
    nsteps = 100000
    dt = 5.

    #NT = 9*N_max**3/2
    #every = nsteps // NT

    if overwrite and os.path.exists(orbit_filename):
        os.remove(orbit_filename)

    toy_potential = None
    if not os.path.exists(orbit_filename):
        # integrate an orbit in a axisymmetric potential
        logger.debug("Integrating orbit for {} steps...".format(nsteps))
        acc = lambda t,w: np.hstack((w[...,3:],potential.acceleration(w[...,:3])))
        integrator = si.DOPRI853Integrator(acc)
        # acc = lambda t,x: potential.acceleration(x)
        # integrator = si.LeapfrogIntegrator(acc)
        t,w = integrator.run(w0, dt=dt, nsteps=nsteps)
        logger.debug("...done!")

        loop = sd.classify_orbit(w)
        if np.any(loop == 1) and not force_harmonic_oscillator: # loop orbit
            logger.debug("Orbit classified as LOOP")
            m,b = sd.fit_isochrone(w, units=units)
            toy_potential = sp.IsochronePotential(m=m, b=b, units=units)
        else:
            logger.debug("Orbit classified as BOX")
            omegas = sd.fit_harmonic_oscillator(w, units=units)
            toy_potential = sp.HarmonicOscillatorPotential(omega=omegas, units=units)

        # also integrate the orbit in the best-fitting toy potential
        toy_steps = w.shape[0]//10
        logger.debug("Integrating toy orbit for {} steps...".format(toy_steps))
        acc = lambda ts,ws: np.hstack((ws[...,3:],toy_potential.acceleration(ws[...,:3])))
        integrator = si.DOPRI853Integrator(acc)
        # acc = lambda t,x: toy_potential.acceleration(x)
        # integrator = si.LeapfrogIntegrator(acc)
        toy_t,toy_w = integrator.run(w0, dt=dt, nsteps=toy_steps)
        logger.debug("...done!")

        # cache the orbits
        np.save(orbit_filename, (t,w,toy_t,toy_w))

        logger.debug("Orbit computed and saved to file: {}".format(orbit_filename))
    else:
        t,w,toy_t,toy_w = np.load(orbit_filename)
        logger.debug("Orbit read from file: {}".format(orbit_filename))

    # for i in range(100):
    #     omega0 = np.random.uniform(0.,100.,size=3)
    #     omegas = sd.fit_harmonic_oscillator(w, units=units, omega=omega0)
    #     print(omegas)
    #     toy_potential = sp.HarmonicOscillatorPotential(omega=omegas, units=units)
    # sys.exit(0)

    if toy_potential is None:
        loop = sd.classify_orbit(w)
        if np.any(loop == 1) and not force_harmonic_oscillator: # loop orbit
            m,b = sd.fit_isochrone(w, units=units)
            toy_potential = sp.IsochronePotential(m=m, b=b, units=units)
        else:
            omegas = sd.fit_harmonic_oscillator(w, units=units)
            toy_potential = sp.HarmonicOscillatorPotential(omega=omegas, units=units)

    logger.debug("Toy potential: {}".format(toy_potential))

    # plot a smaller section of the orbit in projections of XYZ
    plot_w = w[:w.shape[0]//10]
    fig = sd.plot_orbits(toy_w, marker=None, linestyle='-',
                         alpha=0.5, triangle=True, c='r')
    fig = sd.plot_orbits(plot_w, axes=fig.axes, marker=None, linestyle='-',
                         alpha=0.8, triangle=True, c='k')
    fig.savefig(os.path.join(plot_path, "orbit_xyz{}.png".format(suffix)))

    # plot a smaller section of the orbit in the meridional plane
    fig,ax = plt.subplots(1,1,figsize=(6,6))
    R = np.sqrt(plot_w[:,0,0]**2 + plot_w[:,0,1]**2)
    toy_R = np.sqrt(toy_w[:,0,0]**2 + toy_w[:,0,1]**2)
    ax.plot(toy_R, toy_w[:,0,2], marker=None, linestyle='-', alpha=0.5, c='r')
    ax.plot(R, plot_w[:,0,2], marker=None, linestyle='-', alpha=0.8, c='k')
    ax.set_xlabel("$R$")
    ax.set_ylabel("$Z$", rotation='horizontal')
    fig.savefig(os.path.join(plot_path, "orbit_Rz{}.png".format(suffix)))

    return t,w,toy_potential