コード例 #1
0
    def test_plot_cauchyrv(self):
        def true_alpha_density_ratio(sample):
            return cauchy.pdf(sample, 0, 1. / 8) / (
                alpha * cauchy.pdf(sample, 0, 1. / 8) +
                (1 - alpha) * cauchy.pdf(sample, 0, 1. / 2))

        def estimated_alpha_density_ratio(sample):
            return densratio_obj.compute_density_ratio(sample)

        np.random.seed(1)
        x = cauchy.rvs(size=200, loc=0, scale=1. / 8)
        y = cauchy.rvs(size=200, loc=0, scale=1. / 2)
        alpha = 0
        densratio_obj = densratio(x, y, alpha=alpha)
        sample_points = np.linspace(-1, 3, 400)
        plt.plot(sample_points,
                 true_alpha_density_ratio(sample_points),
                 'b-',
                 label='True Alpha-Relative Density Ratio')
        plt.plot(sample_points,
                 estimated_alpha_density_ratio(sample_points),
                 'r-',
                 label='Estimated Alpha-Relative Density Ratio')
        plt.title(
            "Alpha-Relative Density Ratio - Cauchy Random Variables (alpha={:03.2f})"
            .format(alpha))
        plt.legend()
        plt.show()
        assert True
コード例 #2
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def generate_point(distribution, noise, cluster_number, number_of_clusters):
    max_value = number_of_clusters * 10
    overlap = (noise * np.random.uniform(low=0, high=1))
    min = (10 * cluster_number) - (overlap * 10)
    max = 10 + (overlap * 10) + (10 * cluster_number)
    if distribution == 'g':
        point = [
            np.random.normal(loc=(max + min) / 2, scale=(max - min) / 3),
            np.random.normal(loc=(max + min) / 2),
            np.random.normal(loc=(max + min) / 2, scale=(max - min) / 3),
            np.random.randint(max_value),
            np.random.randint(4) * (max_value / 4),
            np.random.randint(2) * max_value, 12345, cluster_number * 10
        ]
    elif distribution == 'c':
        point = [
            cauchy.rvs(loc=(max + min) / 2, scale=(max - min) / 100),
            cauchy.rvs(loc=(max + min) / 2, scale=(max - min) / 100),
            cauchy.rvs(loc=(max + min) / 2, scale=(max - min) / 100),
            np.random.randint(max_value),
            np.random.randint(4) * (max_value / 4),
            np.random.randint(2) * max_value, 12345, cluster_number * 10
        ]
    else:
        point = [
            np.random.uniform(low=(10 * cluster_number),
                              high=(10 * cluster_number) + 10),
            np.random.uniform(low=min, high=max),
            np.random.uniform(low=min, high=max),
            np.random.randint(max_value),
            np.random.randint(4) * (max_value / 4),
            np.random.randint(2) * max_value, 12345, cluster_number * 10
        ]
    return point
コード例 #3
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def line(N, width, line="MnKa"):
    """
    Simulate Ka/Kb Line
    
    Parameters (and their default values):
        N:      desired number of pulse
        width:  width (FWHM) of gaussian (voigt) profile
        line:   line to simulate (Default: MnKa)
    
    Return (e):
        e:      simulated data
    """

    if width == 0:
        # Simulate by Cauchy (Lorentzian)
        e = np.array([])
        fs = np.asarray(Constants.FS[line])
        for f in fs[fs.T[2].argsort()]:
            e = np.concatenate((e, cauchy.rvs(loc=f[0], scale=Analysis.fwhm2gamma(f[1]), size=int(f[2]*N))))
        e = np.concatenate((e, cauchy.rvs(loc=f[0], scale=Analysis.fwhm2gamma(f[1]), size=int(N-len(e)))))
        
    else:
        # Simulate by Voigt
        pdf = lambda E: Analysis.line_model(E, 0, width, line=line)
        Ec = np.array(Constants.FS[line])[:,0]
        _Emin = np.min(Ec) - width*50
        _Emax = np.max(Ec) + width*50
        e = random(pdf, N, _Emin, _Emax)
    
    return e
コード例 #4
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ファイル: Simulation.py プロジェクト: robios/PyTES
def line(N, width, line="MnKa"):
    """
    Simulate Ka/Kb Line
    
    Parameters (and their default values):
        N:      desired number of pulse
        width:  width (FWHM) of gaussian (voigt) profile
        line:   line to simulate (Default: MnKa)
    
    Return (e):
        e:      simulated data
    """

    if width == 0:
        # Simulate by Cauchy (Lorentzian)
        fs = np.asarray(Constants.FS[line])
        renorm = fs.T[2].sum()**-1
        e = np.concatenate([ cauchy.rvs(loc=f[0], scale=Analysis.fwhm2gamma(f[1]), size=int(f[2]*renorm*N)) for f in fs ])
        if N - len(e) > 0:
            e = np.concatenate((e, cauchy.rvs(loc=f[0], scale=Analysis.fwhm2gamma(f[1]), size=int(N-len(e)))))
        
    else:
        # Simulate by Voigt
        pdf = lambda E: Analysis.line_model(E, 0, width, line=line)
        Ec = np.array(Constants.FS[line])[:,0]
        _Emin = np.min(Ec) - width*50
        _Emax = np.max(Ec) + width*50
        e = random(pdf, N, _Emin, _Emax)
    
    return e[:N]
コード例 #5
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def Ridgway_generator(d, seed, cpam):
    np.random.seed(seed)
    X = cauchy.rvs(scale=cpam, size=(d, d))
    a = cauchy.rvs(scale=cpam, size=d)
    Sigma = X.T @ X
    normalizer = np.diag(1 / np.sqrt(np.diag(Sigma)))
    Sigma = normalizer @ Sigma @ normalizer
    a = normalizer @ a
    return Sigma, a
コード例 #6
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 def generate(self, num_instances):
     self.num_instances = num_instances
     N0, N1 = self.generate_instances_numbers()
     S0 = cauchy.rvs(loc=self.mu0, scale=self.scale0,
                     size=N0)  #np.random.normal(self.mu0, self.sigma0, N0)
     S1 = cauchy.rvs(loc=self.mu1, scale=self.scale1,
                     size=N1)  #np.random.normal(self.mu1, self.sigma1, N1)
     X = np.array(np.concatenate((S0, S1), axis=0))
     y = np.asarray([0] * N0 + [1] * N1)
     return X, y
コード例 #7
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 def get_system_noise(self):
     """v_t vector"""
     data_noise = np.zeros((self.ydim, self.PARTICLES_NUM), dtype=np.float64)
     for i in xrange(self.ydim):
         data_noise[i,:] = cauchy.rvs(loc=[0]*self.PARTICLES_NUM, scale=np.power(10,self.particles[self.ydim]),
                                 size=self.PARTICLES_NUM)
     data_noise[data_noise==float("-inf")] = -1e308
     data_noise[data_noise==float("inf")] = 1e308
     
     parameter_noises = np.zeros((self.pdim, self.PARTICLES_NUM), dtype=np.float64)
     for i in xrange(self.pdim):
         parameter_noises[i,:] = cauchy.rvs(loc=0, scale=self.nois_sh_parameters[i], size=self.PARTICLES_NUM)
     return np.vstack((data_noise, parameter_noises))
コード例 #8
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def selectF(muF):
    # randomly generate new F based on a Cauchy distribution
    newF = cauchy.rvs(loc=muF, scale=0.1)
    # if it is smaller than 0, try to generate a new F value that is not 
    # smaller than 0
    if newF <= 0: 
        while newF <= 0:
            newF = cauchy.rvs(loc=muF, scale=0.1)
    # when the newly calculated F value is greater than 1 -> return 1
    if newF > 1: 
        return 1
    else: 
        return newF
コード例 #9
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def CauchyBoxplotTukey():
    tips, result, count = [], [], 0
    for size in sizes:
        for i in range(NUMBER_OF_REPETITIONS):
            distribution = cauchy.rvs(size=size)
            distribution.sort()
            count += count_out(distribution)
        result.append(count / (size * NUMBER_OF_REPETITIONS))
        distribution = cauchy.rvs(size=size)
        distribution.sort()
        tips.append(distribution)
    DrawBoxplot(tips, CAUCHY)
    printAnswer(result)
    return
コード例 #10
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def selectF(mF):
    # get a random index ri in the F memory
    ri = np.random.randint(0, mF.shape[0])
    # get random new F by a chauchy distribution where mF[ri] is the centre
    newF = cauchy.rvs(loc=mF[ri], scale=0.1)
    # if it is smaller than 0, try to generate a new F value that is not
    # smaller than 0
    if newF <= 0:
        while newF <= 0:
            newF = cauchy.rvs(loc=mF[ri], scale=0.1)
    # when the newly calculated F value is greater than 1 -> return 1
    if newF > 1:
        return 1
    else:
        return newF
コード例 #11
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    def __init__(self,
                 d,
                 gamma=1,
                 D=50,
                 metric='rbf',
                 device=torch.device('cpu')):
        '''
		d: dimension of input
		D: number of Fourier features
		metric: 'rbf' or 'laplace'
		'''
        self.D = D

        # Sample frequencies
        if metric == 'rbf':
            self.w = np.sqrt(2 * gamma) * torch.empty(
                (D, d), device=device).normal_().double()
        elif metric == 'laplace':
            self.w = cauchy.rvs(scale=gamma, size=(D, d))
            self.w = torch.from_numpy(self.w).double().to(device)
        self.w_inv = torch.pinverse(self.w)

        # Sample offsets
        self.b = 2 * np.pi * torch.empty(
            (D, ), device=device, dtype=torch.double).random_(0, to=1)
コード例 #12
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def cauchy_distribution(select_size, asked=rvs, x=0):
    if asked == rvs:
        return cauchy.rvs(size=select_size)
    elif asked == pdf:
        return cauchy.pdf(x)
    elif asked == cdf:
        return cauchy.cdf(x)
コード例 #13
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def randwalk(lgth,
             stiff,
             start=[0., 0.],
             step=1.,
             adrift=0.,
             anoise=.2,
             dist="const"):
    """generates a 2d random walk with variable angular correlation and optional constant (+noise) angular drift.
    Arguments: walk length "lgth", stiffness factor "stiff" - consecutive orientations are derived by adding stiff*(random number in [-1,1]).
    Parameters "adrift" and "anoise" add a constant drift angle adrift modulated by a noise factor adrift*(random number in [-1,1]).
    The dist parameter accepts non-constant step length distributions (right now, only cauchy/gaussian distributed random variables)"""
    rw = [
        list(start)
    ]  #user provided initial coordinates: make (reasonably) sure it's a nested list type.
    ang = [0]
    #step lengths are precalculated for each step to account for
    if dist == "cauchy": steps = cauchy.rvs(size=lgth)
    elif dist == "norm": steps = norm.rvs(size=lgth)
    else: steps = array([step] * lgth)  #Overkill for constant step length ;)
    #first generate angular progression vila cumulative sum of increments (random/stiff + drift terms)
    angs = cumsum(stiff * uniform.rvs(size=lgth, loc=-1, scale=2) + adrift *
                  (1. + anoise * uniform.rvs(size=lgth, loc=-1, scale=2)))
    #x/y trace via steplength and angle for each step, some array reshuffling (2d conversion and transposition)
    rw = concatenate([
        concatenate([array(start[:1]),
                     cumsum(steps * sin(angs)) + start[0]]),
        concatenate([array(start)[1:],
                     cumsum(steps * cos(angs)) + start[1]])
    ]).reshape(2, -1).transpose()
    return rw, angs
コード例 #14
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ファイル: task2.py プロジェクト: Doxxer/SPbAU-Spring-2014
def solve(n):
    x_cauchy = cauchy.rvs(size=n * M, loc=a, scale=s).reshape(M, n)
    x_median = np.apply_along_axis(np.median, 1, x_cauchy)
    x_mad = np.apply_along_axis(mad, 1, x_cauchy)
    mu = -x_median / x_mad
    ka = 1 / x_mad

    ci_par = a_ci(ci_parametric(mu, gamma), x_median, x_mad)
    ci_non_par = a_ci(ci_non_parametric(mu, gamma), x_median, x_mad)

    x_med = mean(x_median)
    empirical_cl_non_par, empirical_cl_par, sd_width_non_par, sd_width_par, width_non_par, width_par = \
        test_ci(ci_non_par, ci_par, x_med)

    print("LOCATION | N = {0:5}; Non-parametric: width = {1} ({2}); empirical CL = {3}".format(
        n, mean(width_non_par), sd_width_non_par, empirical_cl_non_par))
    print("LOCATION | N = {0:5};     Parametric: width = {1} ({2}); empirical CL = {3}".format(
        n, mean(width_par), sd_width_par, empirical_cl_par))

    # ---------------------------------

    ci_par = s_ci(ci_parametric(ka, gamma), x_mad)
    ci_non_par = s_ci(ci_non_parametric(ka, gamma), x_mad)

    mad_ = np.exp(mean(np.log(np.abs(x_cauchy - x_med))))
    empirical_cl_non_par, empirical_cl_par, sd_width_non_par, sd_width_par, width_non_par, width_par = \
        test_ci(ci_non_par, ci_par, mad_)

    print("SCALE    | N = {0:5}; Non-parametric: width = {1} ({2}); empirical CL = {3}".format(
        n, mean(width_non_par), sd_width_non_par, empirical_cl_non_par))
    print("SCALE    | N = {0:5};     Parametric: width = {1} ({2}); empirical CL = {3}".format(
        n, mean(width_par), sd_width_par, empirical_cl_par))
    print
    print
コード例 #15
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async def iot_handler(websocket, path):
    await websocket.send(motd)
    # mode_query = "What kind of sensor would you like? (temperature,occupancy)"
    # await websocket.send(mode_query)

    # mode = await websocket.recv()
    mode = "all"

    rooms = get_simulated_rooms()

    while True:
        await asyncio.sleep(erlang.rvs(1, 0, size=1))

        room = random.choice(list(rooms.keys()))
        dat = {"time": datetime.now().isoformat()}

        if mode.startswith(("all", "tem")):
            dat["temperature"] = cauchy.rvs(loc=rooms[room]["loc"],
                                            scale=rooms[room]["scale"],
                                            size=1).tolist()
        if mode.startswith(("all", "occ")):
            dat["occupancy"] = poisson.rvs(rooms[room]["occ"], size=1).tolist()
        if mode.startswith(("all", "co")):
            dat["co2"] = gamma.rvs(rooms[room]["co"], size=1).tolist()

        await websocket.send(json.dumps({room: dat}))
コード例 #16
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async def iot_handler(websocket, path):
    """
    generate simulated data for each room and sensor
    """

    await websocket.send(motd)
    mode = "all"

    rooms = get_simulated_rooms()

    print("IoT simulator connected to", websocket.remote_address)
    while True:
        await asyncio.sleep(erlang.rvs(1, 0, size=1).item())

        room = random.choice(list(rooms.keys()))
        dat = {"time": datetime.now().isoformat()}

        if mode.startswith(("all", "tem")):
            dat["temperature"] = cauchy.rvs(
                loc=rooms[room]["loc"], scale=rooms[room]["scale"], size=1
            ).tolist()
        if mode.startswith(("all", "occ")):
            dat["occupancy"] = poisson.rvs(rooms[room]["occ"], size=1).tolist()
        if mode.startswith(("all", "co")):
            dat["co2"] = gamma.rvs(rooms[room]["co"], size=1).tolist()

        try:
            await websocket.send(json.dumps({room: dat}))
        except websockets.exceptions.ConnectionClosedOK:
            print("Closing connection to", websocket.remote_address)
            break
コード例 #17
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def gen_free_energy(distribution, spread=2.0, location=0.0, size=1):
    """
    Generate example free energies from a specified distribution

    Parameters
    ----------
    distribution: str
        the distribution from which to draw samples
    size: int
        number of samples to generate
    spread: list or float
        the spread/scale parameter of the distribution, e.g. standard deviation for gaussian
    location: list of float
        the center of the distribution, e.d.

    Returns
    -------
    numpy.ndarray
    samples of free energy with dimentions equal to spread and location

    """
    if distribution.lower() == 'gaussian':
        f_true = np.random.normal(loc=location, scale=spread, size=size)
    elif distribution.lower() == 'cauchy':
        from scipy.stats import cauchy
        f_true = cauchy.rvs(loc=location, scale=spread, size=size)
    else:
        raise Exception(
            'The distribution must be either "gaussain" or "cauchy".')
    return f_true
コード例 #18
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    def rvs(cls,
            alpha: float,
            beta: float,
            gamma=1.,
            delta=0.,
            pm=1,
            size: Numeric = 1):
        cls._check_parameters(alpha, beta, gamma, pm)
        delta, gamma = cls._parameterize(alpha, delta, gamma, beta, pm)

        if np.isclose(alpha, 1) and np.isclose(beta, 0):
            z = cauchy.rvs(size=size)
        else:
            theta = np.pi * (np.random.uniform(size=size) - 0.5)
            w = np.random.standard_exponential(size)

            bt = beta * tanpi2(alpha)
            t0 = min(max(-PI2, np.arctan(bt) / alpha), PI2)
            at = alpha * (theta + t0)

            c = (1 + bt**2)**(1 / (2 * alpha))

            z = (c * np.sin(at) * (np.cos(theta)**(-1 / alpha)) *
                 ((np.cos(theta - at) / w)**((1 - alpha) / alpha)) - bt)

        return z * gamma + delta
コード例 #19
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ファイル: quickquasars.py プロジェクト: desihub/desisim
def mod_cauchy(loc,scale,size,cut):
    samples=cauchy.rvs(loc=loc,scale=scale,size=3*size)
    samples=samples[abs(samples)<cut]
    if len(samples)>=size:
       samples=samples[:size]
    else:
        samples=mod_cauchy(loc,scale,size,cut)   ##Only added for the very unlikely case that there are not enough samples after the cut.
    return samples
コード例 #20
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ファイル: lab3.py プロジェクト: b14ckster/TeorVer
def distributions(size):
    n = norminvgauss.rvs(1, 0, size=size)
    l = laplace.rvs(size=size, scale=1 / m.sqrt(2), loc=0)
    p = poisson.rvs(10, size=size)
    c = cauchy.rvs(size=size)
    u = uniform.rvs(size=size, loc=-m.sqrt(3), scale=2 * m.sqrt(3))
    counted_distributions = [n, l, p, c, u]
    return counted_distributions
コード例 #21
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def mod_cauchy(loc,scale,size,cut):
    samples=cauchy.rvs(loc=loc,scale=scale,size=3*size)
    samples=samples[abs(samples)<cut]
    if len(samples)>=size:
       samples=samples[:size]
    else:
        samples=mod_cauchy(loc,scale,size,cut)   ##Only added for the very unlikely case that there are not enough samples after the cut.
    return samples
コード例 #22
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def generate_panel(N, T, k, q, d, lam):
    beta = []
    rho = []
    # cov_rho = []
    for l in range(k):
        beta.append(generate_beta(d - 1))
        temp_rho = generate_rho(q, lam)
        rho.append(temp_rho)

    panel1 = np.array([[[1.0 for fea in range(d)] for t in range(T)]
                       for i in range(N)])
    panel2 = np.array([[[1.0 for fea in range(d)] for t in range(T)]
                       for i in range(N)])
    mean = [0 for i in range(d - 2)]
    cov = np.identity(d - 2)

    # mean vector of each individual
    mean_individual = []
    cluster = np.random.randint(0, k, N)
    for i in range(N):
        temp = np.random.multivariate_normal(mean, cov, 1)[0]
        temp = temp / np.sqrt(square_sum(temp)) * np.random.uniform(0, 5)
        mean_individual.append(temp)
    #for i in range(N):
    #    l2 = square_sum(mean_individual[i])
    #    norm = random.uniform(0, 10)
    #    for dim in range(d-1):
    #        mean_individual[i][dim] *= math.sqrt(norm / l2)
    # model of each individual
    mean_error = [0 for i in range(T)]
    for i in range(N):
        # Gaussian error
        mean_i = np.random.multivariate_normal(
            mean_individual[i], cov * square_sum(mean_individual[i]), T)
        error_i = []
        error_basic = np.random.normal(0, 1, T)
        for t in range(T):
            error_i.append(error_basic[t])
            for tt in range(min(t - 1, q)):
                error_i[t] += rho[cluster[i]][tt] * error_i[t - tt - 1]
        for t in range(T):
            panel1[i][t][0:-2] = mean_i[t]
            panel1[i][t][d - 1] = np.dot(panel1[i][t][0:d - 1],
                                         beta[cluster[i]]) + error_i[t]
        # Cauchy error
        error_i = []
        error_basic = cauchy.rvs(
            0, 2, T
        )  # errors drawn from Cauchy distribution with x0 = 0 and gamma = 2
        for t in range(T):
            error_i.append(error_basic[t])
            for tt in range(min(t - 1, q)):
                error_i[t] += rho[cluster[i]][tt] * error_i[t - tt - 1]
        for t in range(T):
            panel2[i][t][0:-2] = mean_i[t]
            panel2[i][t][d - 1] = np.dot(panel2[i][t][0:d - 1],
                                         beta[cluster[i]]) + error_i[t]
    return panel1, panel2
コード例 #23
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ファイル: LpSearch.py プロジェクト: erankfmn/lpsearch
 def _generate_uniform_planes(self, size, input_dim):
     """ Generate uniformly distributed hyperplanes and return it as a 2D
     numpy array.
     """
     if (self.lazy):
         self.uniform_planes = cauchy.rvs(
             size=[size, self.hash_size, self.points.shape[1]])
     else:
         self.uniform_planes = np.random.randn(size, self.hash_size,
                                               input_dim)
コード例 #24
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ファイル: main.py プロジェクト: nikos72344/MathStat
def cauchyFunc():
    for i in range(len(size)):
        n = size[i]
        fig, ax = plt.subplots(1, 1)
        ax.set_title("Распределение Коши, n = " + str(n))
        x = np.linspace(cauchy.ppf(0.01), cauchy.ppf(0.99), 100)
        ax.plot(x, cauchy.pdf(x), 'b-', lw=5, alpha=0.6)
        r = cauchy.rvs(size=n)
        ax.hist(r, density=True, histtype='stepfilled', alpha=0.2)
        plt.show()
コード例 #25
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    def generate_signals(self, sig, noise_type = 4):
        '''
        generate noises for given sig and noise type

        '''
        # TODO: add different noises
        if noise_type == 0: #gaussian
            noise = np.random.normal(size=sig.shape)
        elif noise_type == 1: # cauchy
            from scipy.stats import cauchy
            noise = cauchy.rvs(size=sig.shape) 
        elif noise_type == 2: # poisson
            noise = np.random.poisson(size=sig.shape)
        elif noise_type == 3: # speckle: Multiplicative noise using out = image + n*image,where  n is gaussion noise with specified mean & variance.
            noise = np.random.randn(size=sig.shape)*sig
        else:# mix of 0 & 1 
            from scipy.stats import cauchy
            noise = np.random.normal(size=sig.shape) + cauchy.rvs(size=sig.shape) 
        return noise
コード例 #26
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def generate_data(room: T.Dict[str, float]) -> T.Dict[str, T.Union[str, float]]:
    """
    generate simulated data
    """

    return {
        "time": datetime.now().isoformat(),
        "temperature": cauchy.rvs(loc=room["loc"], scale=room["scale"], size=1).tolist(),
        "occupancy": poisson.rvs(room["occ"], size=1).tolist(),
        "co2": gamma.rvs(room["co"], size=1).tolist(),
    }
コード例 #27
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    def get_system_noise(self):
        """v_t vector"""
        data_noise = np.zeros((self.ydim, self.PARTICLES_NUM),
                              dtype=np.float64)
        for i in xrange(self.ydim):
            data_noise[i, :] = cauchy.rvs(loc=[0] * self.PARTICLES_NUM,
                                          scale=np.power(
                                              10, self.particles[self.ydim]),
                                          size=self.PARTICLES_NUM)
        data_noise[data_noise == float("-inf")] = -1e308
        data_noise[data_noise == float("inf")] = 1e308

        parameter_noises = np.zeros((self.pdim, self.PARTICLES_NUM),
                                    dtype=np.float64)
        for i in xrange(self.pdim):
            parameter_noises[i, :] = cauchy.rvs(
                loc=0,
                scale=self.nois_sh_parameters[i],
                size=self.PARTICLES_NUM)
        return np.vstack((data_noise, parameter_noises))
コード例 #28
0
ファイル: lab1.py プロジェクト: tmffv/MathStat
def cauchyNumbers():
    for size in sizes:
        fig, ax = plt.subplots(1, 1)
        ax.hist(cauchy.rvs(size=size), histtype='stepfilled', alpha=0.5, color='blue', density=True)
        x = np.linspace(cauchy().ppf(0.01), cauchy().ppf(0.99), 100)
        ax.plot(x, cauchy().pdf(x), '-')
        ax.set_title('CauchyNumbers n = ' + str(size))
        ax.set_xlabel('CauchyNumbers')
        ax.set_ylabel('density')
        plt.grid()
        plt.show()
    return
コード例 #29
0
 def random_growth(self):
     """ Cauchy distribution with barriers at -30 and 15 percent.
     """
     growth = cauchy.rvs(size=1,
                         loc=self.config['growth_mu'],
                         scale=self.config['growth_sigma'])[0]
     if growth < -0.30:
         return -0.30
     elif growth > 0.15:
         return 0.15
     else:
         return growth
def dg_cauchy(n=150,
              num_groups=40,
              group_size=40,
              p=1600,
              ro=0.5,
              num_non_zero_coef_per_group=8,
              num_non_zero_groups=7,
              loc=0,
              scale=3):
    """
    Generate a dataset formed by groups of variables. All the groups have the same size.
    num_non_zero_coef_per_group
    num_non_zero_groups
    :param n: number of observations
    :param num_groups: number of groups
    :param group_size: size of the groups
    :param p: number of variables
    :param ro: correlation between variables inside a group
    :param num_non_zero_coef_per_group: controls how many significant variables we want
    :param num_non_zero_groups: controls how many groups we want to store significant variables
    :param loc: location parameter for cauchy error
    :param scale: scale parameter for cauchy error
    :return: x, y index
    If num_non_zero_coef_per_group=8 and num_non_zero_groups=7 we will have 8 groups with 7 significant variables,
    and num_groups-num_non_zero_coef_per_group groups with all non-significant variables
    The error distribution is a student t with 3 degrees of freedom
    """
    p = num_groups * group_size
    group_levels = np.arange(1, (num_groups + 1), 1)
    num_non_zeros_per_group = [0] * num_groups
    num_non_zeros_per_group[0:num_non_zero_groups] = [
        num_non_zero_coef_per_group
    ] * num_non_zero_groups
    group_index = np.repeat(group_levels, [group_size] * num_groups, axis=0)
    s = np.zeros((p, p))
    for level in group_levels:
        s[(level - 1) * group_size:level * group_size,
          (level - 1) * group_size:level * group_size] = ro
    np.fill_diagonal(s, 1)
    x = np.random.multivariate_normal(np.repeat(0, p), s, n)
    betas = np.zeros(p)
    for i in range(num_groups):
        betas[(i * group_size):((i + 1) * group_size)] = np.arange(
            1, group_size + 1, 1)
    for i in range(num_groups):
        betas[((group_levels[i] - 1) * group_size +
               num_non_zeros_per_group[i]):group_levels[i] * group_size] = 0
    e = cauchy.rvs(loc=loc, scale=scale, size=n)
    y = np.dot(x, betas) + e
    data = dict(x=x, y=y, true_beta=betas, index=group_index)
    logger.debug('Function finished without errors')
    return data
コード例 #31
0
ファイル: lab3.py プロジェクト: Drozdova-Daria/Math_Stat_Lab3
def selection(mu, sigma, size, distribution):
    if distribution == Distribution.NORMAL:
        return norm.rvs(mu, sigma, size)
    elif distribution == Distribution.CAUCHY:
        return cauchy.rvs(mu, sigma, size)
    elif distribution == Distribution.LAPLACE:
        return laplace.rvs(mu, sigma, size)
    elif distribution == Distribution.POISSON:
        return poisson.rvs(mu, size=size)
    elif distribution == Distribution.UNIFORM:
        return uniform.rvs(mu, sigma, size)
    else:
        return None
コード例 #32
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ファイル: Timing.py プロジェクト: Khev/coarse_grain_networks
def make_positive_cauchy_rv(N, mean, var):
    """ Makes a list of N POSITIVE random variates drawn from a cauchy dist
        with given mean and var (or whatever pars define the dist).
        
    """

    omega = []
    for i in range(N):
        temp = -1
        while temp < 0:
            temp = float(cauchy.rvs(size=1, scale=var_omega, loc=mean_omega))
        omega.append(temp)
    return omega
コード例 #33
0
    def dataGeneration(self, x1=-5, x2=5, N=100):
        c = Cauchy_regression1.c
        d = Cauchy_regression1.d

        np.random.seed()
        x = np.random.uniform(x1, x2, N)
        s_rand = np.zeros(N)
        for i in range(len(x)):
            gamma = abs(c * x[i] + d)
            s_rand[i] = cauchy.rvs(loc=0, scale=gamma, size=1)
        y = self.a * x + self.b + s_rand

        return np.append(x, y).reshape(2, N).transpose()
コード例 #34
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def Cauchy():
    for s in size:
        density = cauchy()
        histogram = cauchy.rvs(size=s)
        fig, ax = plt.subplots(1, 1)
        ax.hist(histogram, density=True, alpha=0.6)
        x = np.linspace(density.ppf(0.01), density.ppf(0.99), 100)
        ax.plot(x, density.pdf(x), LINE_TYPE, lw=1.5)
        ax.set_xlabel("CAUCHY")
        ax.set_ylabel("DENSITY")
        ax.set_title("SIZE: " + str(s))
        plt.grid()
        plt.show()
コード例 #35
0
ファイル: Timing.py プロジェクト: Khev/coarse_grain_networks
def make_positive_cauchy_rv(N, mean, var):
    """ Makes a list of N POSITIVE random variates drawn from a cauchy dist
        with given mean and var (or whatever pars define the dist).
        
    """
    
    omega = []
    for i in range(N):
        temp = -1
        while temp < 0:
            temp =  float(cauchy.rvs(size = 1, scale = var_omega,  loc = mean_omega))
        omega.append(temp)
    return omega
コード例 #36
0
ファイル: gsm_test.py プロジェクト: mhahn0106/cisa
	def test_train(self):
		gsm = GSM(1, 10)
		gsm.train(laplace.rvs(size=[1, 10000]), max_iter=100, tol=-1)

		p = kstest(gsm.sample(10000).flatten(), laplace.cdf)[1]

		# test whether GSM faithfully reproduces Laplace samples
		self.assertTrue(p > 0.0001)

		gsm = GSM(1, 6)
		gsm.train(cauchy.rvs(size=[1, 10000]), max_iter=100, tol=-1)

		# test for stability of training
		self.assertTrue(not any(isnan(gsm.scales)))
コード例 #37
0
ファイル: _stable.py プロジェクト: chrisburr/copulae
    def rvs(cls, alpha: float, beta: float, gamma=1., delta=0., pm=1, size: Numeric = 1):
        cls._check_parameters(alpha, beta, gamma, pm)
        delta, gamma = cls._form_parameters(alpha, delta, gamma, beta, pm)

        if np.isclose(alpha, 1) and np.isclose(beta, 0):
            z = cauchy.rvs(size=size)
        else:
            theta = np.pi * (np.random.uniform(size=size) - 0.5)
            w = np.random.standard_exponential(size)

            bt = beta * tanpi2(alpha)
            t0 = min(max(-PI2, np.arctan(bt) / alpha), PI2)
            at = alpha * (theta + t0)

            c = (1 + bt ** 2) ** (1 / (2 * alpha))

            z = c * np.sin(at) \
                * (np.cos(theta - at) / w) ** (1 / alpha - 1) \
                / np.cos(theta) ** (1 / alpha) \
                - bt

        return z * gamma + delta
コード例 #38
0
N = 1000
x = 4
Inf = float("inf")

# scipy.integrateでの積分
h1 = lambda t: t * norm(loc=x).pdf(t) * cauchy.pdf(t)
h2 = lambda t: norm(loc=x).pdf(t) * cauchy.pdf(t)
num = scipy.integrate.quad(h1, -Inf, Inf)[0]
den = scipy.integrate.quad(h2, -Inf, Inf)[0]
I = num / den
print("scipy.integrate:", I)

# (1) コーシー分布からサンプリングするモンテカルロ積分の収束テスト
# 分子も分母も同じサンプルを使用すると仮定
theta = cauchy.rvs(size=N)
num = theta * norm(loc=x).pdf(theta)
den = norm(loc=x).pdf(theta)

# 分母に0がくるサンプルを削除
num = num[den != 0]
den = den[den != 0]
Ndash = len(num)

y = num / den
estint = (np.cumsum(num) / np.arange(1, Ndash + 1)) / \
    (np.cumsum(den) / np.arange(1, Ndash + 1))
esterr = np.sqrt(np.cumsum((y - estint) ** 2)) / np.arange(1, Ndash + 1)

plt.subplot(2, 1, 1)
plt.plot(estint, color='red', linewidth=2)
コード例 #39
0
ファイル: isa.py プロジェクト: lucastheis/isa
	def initialize(self, X=None, method='data'):
		"""
		Initializes parameter values with more sensible values.

		@type  X: array_like
		@param X: data points stored in columns

		@type  method: string
		@param method: type of initialization ('data', 'gabor' or 'random')
		"""

		if self.noise:
			L = self.A[:, :self.num_visibles]

		if method.lower() == 'data':
			# initialize features with data points
			if X is not None:
				if X.shape[1] < self.num_hiddens:
					raise ValueError('Number of data points to small.')

				else:
					# whitening matrix
					val, vec = eig(cov(X))

					# whiten data
					X_ = dot(dot(diag(1. / sqrt(val)), vec.T), X)

					# sort by norm in whitened space
					indices = argsort(sqrt(sum(square(X_), 0)))[::-1]

					# pick 25% largest data points and normalize
					X_ = X_[:, indices[:max([X.shape[1] / 4, self.num_hiddens])]]
					X_ = X_ / sqrt(sum(square(X_), 0))

					# pick first basis vector at random
					A = X_[:, [randint(X_.shape[1])]]

					for _ in range(self.num_hiddens - 1):
						# pick vector with large angle to all other vectors
						A = hstack([
							A, X_[:, [argmin(max(abs(dot(A.T, X_)), 0))]]])

					# orthogonalize and unwhiten
					A = dot(sqrtmi(dot(A, A.T)), A)
					A = dot(dot(vec, diag(sqrt(val))), A)

					self.A = A

		elif method.lower() == 'gabor':
			# initialize features with Gabor filters
			if self.subspaces[0].dim > 1 and not mod(self.num_hiddens, 2):
				for i in range(self.num_hiddens / 2):
					G = gaborf(self.num_visibles)
					self.A[:, 2 * i] = real(G)
					self.A[:, 2 * i + 1] = imag(G)
			else:
				for i in range(len(self.subspaces)):
					self.A[:, i] = gaborf(self.num_visibles, complex=False)

		elif method.lower() == 'random':
			# initialize with Gaussian white noise
			self.A = randn(num_visibles, num_hiddens)

		elif method.lower() in ['laplace', 'student', 'cauchy', 'exponpow']:
			if method.lower() == 'laplace':
				# approximate multivariate Laplace with GSM
				samples = randn(self.subspaces[0].dim, 10000)
				samples = samples / sqrt(sum(square(samples), 0))
				samples = laplace.rvs(size=[1, 10000]) * samples

			elif method.lower() == 'student':
				samples = randn(self.subspaces[0].dim, 50000)
				samples = samples / sqrt(sum(square(samples), 0))
				samples = t.rvs(2., size=[1, 50000]) * samples

			elif method.lower() == 'exponpow':
				exponent = 0.8
				samples = randn(self.subspaces[0].dim, 200000)
				samples = samples / sqrt(sum(square(samples), 0))
				samples = gamma(1. / exponent, 1., (1, 200000))**(1. / exponent) * samples

			else:
				samples = randn(self.subspaces[0].dim, 100000)
				samples = samples / sqrt(sum(square(samples), 0))
				samples = cauchy.rvs(size=[1, 100000]) * samples

			if self.noise:
				# ignore first subspace
				gsm = GSM(self.subspaces[1].dim, self.subspaces[1].num_scales)
				gsm.train(samples, max_iter=200, tol=1e-8)

				for m in self.subspaces[1:]:
					m.scales = gsm.scales.copy()
			else:
				# approximate distribution with GSM
				gsm = GSM(self.subspaces[0].dim, self.subspaces[0].num_scales)
				gsm.train(samples, max_iter=200, tol=1e-8)

				for m in self.subspaces:
					m.scales = gsm.scales.copy()

		else:
			raise ValueError('Unknown initialization method \'{0}\'.'.format(method))

		if self.noise:
			# don't initialize noise covariance
			self.A[:, :self.num_visibles] = L
コード例 #40
0
ファイル: lcprimitives.py プロジェクト: demorest/PINT
 def random(self,n):
     if hasattr(n,'__len__'):
         n = len(n)
     return np.mod(cauchy.rvs(loc=self.p[-1],scale=self.p[0]/TWOPI,size=n),1)
コード例 #41
0
ファイル: ex_11.py プロジェクト: amaggi/bda
# posterior
theta_post = theta_post_unnorm / Z

# approximate the posterior distribution
theta_mean = trapz(theta * theta_post, theta)
theta_var = trapz((theta-theta_mean)**2 * theta_post, theta)
theta_post_approx = norm(theta_mean, np.sqrt(theta_var))

# get samples from approximate posterior
theta_samples = theta_post_approx.rvs(size=N_SAMP)

# sample the posterior predictive distribution for y6
y6_samples = np.empty(N_SAMP, dtype=float)
for ith in xrange(N_SAMP):
    y6_samples[ith] = cauchy.rvs(loc=theta_samples[ith], scale=1) 

# plot
fig, axes = plt.subplots(1, 3)
plt.sca(axes[0])
plt.plot(theta, theta_post, label='actual')
plt.plot(theta, theta_post_approx.pdf(theta), label='approx')
plt.legend()
plt.xlabel('theta')
plt.ylabel('P(theta | y1...y5)')
plt.sca(axes[1])
plt.hist(theta_samples)
plt.xlabel('theta')
plt.sca(axes[2])
plt.hist(y6_samples)
plt.xlabel('y6')
コード例 #42
0
ファイル: generate.py プロジェクト: calonlay-hj/ppaml-cp4
def sample_episodes(numepisodes, physics):

  episodes = []

  total_events, num_reasonable_events = 0, 0
  
  for epinum in xrange(numepisodes):
    
    events = []
    detections = []
    assocs = []

    # first generate all the events

    numevents = poisson.rvs( physics.lambda_e * 4 * pi * physics.R ** 2
                             * physics.T )
    
    for evnum in xrange(numevents):
      
      # longitude is uniform from -180 to 180
      evlon = uniform.rvs(-180, 360)
      # sin(latitude) is uniform from -1 to 1
      evlat = degrees(arcsin(uniform.rvs(-1, 2)))
      # magnitude has an exponential distribution as per Gutenberg-Richter law
      while True:
        evmag = expon.rvs(physics.mu_m, physics.theta_m)
        # magnitude saturates at some maximum value,
        # re-sample if we exceed the max
        if evmag > physics.gamma_m:
          continue
        else:
          break
        
      # time is uniform
      evtime = uniform.rvs(0, physics.T)
      
      event = Event(evlon, evlat, evmag, evtime)
      
      events.append(event)

      truedets = []

      #print ("event mag %f" % event.mag)

      # for each event generate its set of true detections
      for stanum, station in enumerate(STATIONS):

        dist = compute_distance((station.lon, station.lat),
                                (event.lon, event.lat))
        sta_to_ev_az = compute_azimuth((station.lon, station.lat),
                                       (event.lon, event.lat))

        detprob = logistic(physics.mu_d0[stanum]
                           + physics.mu_d1[stanum] * event.mag
                           + physics.mu_d2[stanum] * dist)

        #print ("stanum %d dist %f detprob %f" % (stanum, dist, detprob))
        
        # is detected ?
        if bernoulli.rvs(detprob):

          dettime = laplace.rvs(event.time + compute_travel_time(dist)
                                + physics.mu_t[stanum],
                                physics.theta_t[stanum])

          # Note: the episode only has detections within the first T
          # seconds. Late arriving detections will not be available.
          if dettime < physics.T:
            degdiff = laplace.rvs(physics.mu_z[stanum], physics.theta_z[stanum])
            detaz = (sta_to_ev_az + degdiff + 360) % 360
            
            detslow = laplace.rvs(compute_slowness(dist) + physics.mu_s[stanum],
                                  physics.theta_s[stanum])

            while True:
              # resample if the detection amplitude is infinite
              try:
                detamp = exp(norm.rvs(physics.mu_a0[stanum]
                                      + physics.mu_a1[stanum] * event.mag
                                      + physics.mu_a2[stanum] * dist,
                                      physics.sigma_a[stanum]))

              except FloatingPointError:
                continue
              
              # disallow zero or infinite amplitudes
              if detamp == 0 or isinf(detamp):
                continue
              break
            
            truedets.append(len(detections))
            detections.append(Detection(stanum, dettime, detaz, detslow,
                                        detamp))

      assocs.append(truedets)

      total_events += 1
      
      if len(truedets) >= 2:
        num_reasonable_events += 1

    # now generate the false detections
    for stanum in xrange(len(STATIONS)):
      numfalse = poisson.rvs(physics.lambda_f[stanum] * physics.T)
      
      for dnum in xrange(numfalse):
        dettime = uniform.rvs(0, physics.T)
        detaz = uniform.rvs(0, 360)
        detslow = uniform.rvs(compute_slowness(180),
                              compute_slowness(0) - compute_slowness(180))

        while True:
          # resample if the detection amplitude is infinite
          try:
            detamp = exp(cauchy.rvs(physics.mu_f[stanum],
                                    physics.theta_f[stanum]))
          except FloatingPointError:
            continue
          
          # disallow zero or infinite amplitudes
          if detamp == 0 or isinf(detamp):
            continue
          break
        
        detections.append(Detection(stanum, dettime, detaz, detslow, detamp))
        
    episodes.append(Episode(events, detections, assocs))
    
  print ("{:d} events generated".format(total_events))
  print ("{:.1f} % events have at least two detections"
         .format(100 * num_reasonable_events / total_events))
  return episodes
コード例 #43
0
ファイル: shade.py プロジェクト: TakeumiYamamura/labolatry
  SF = []
  CR = []
  F = []
  p = []
  u = []
  alldeltaf = []
  deltaf = []
  for var1 in range(0, N):
    r = random.randrange(0, N)
    cr = rand_normal(MCR[var1], math.sqrt(0.1))
    if cr > 1:
      cr = 1
    if cr < 0:
      cr = 0
    CR.append(copy.deepcopy(cr))
    f = cauchy.rvs()
    while True:
      if f > 1:
        f = 1.0
        break
      if f > 0:
        break
      f = cauchy.rvs()
    # print f
    F.append(copy.deepcopy(f)) #コーシー乱数発生よく分かっておらず そもそもなんでコーシー乱数?
    p = random.uniform(2.0/NP, 0.2)
    # generate_trial_vector(x, P, A, p, N, CR, F)
    u.append(generate_trial_vector(population[var1], population, A, p, N, CR[var1], F[var1]))#current to pbest/1/bin
  test_count = 0

  # print len(u)