コード例 #1
0
def SpectralDensityFunction(f, H):
    '''Spectral density function (-0.5<f<0.5) for fractional Gaussian noise with Hurst Exponent H
    I don't know how to derive this formula. It is in Voichita's matlab code, and she refers to it as 
    "the almost exact formula from Percival and Walden".
    I have a feeling that it might be a Taylor series approximation to the Fourier transform of the auto-covariance relation
    for fractional Gaussian Noise.
    >>> SpectralDensityFunction(0.26,0.2367)
    1.1067908939278011
    '''
    if (H == 0):
        return 2 * sin(pi * f)**2
    else:
        M = 100  #sum from k = -M to M of 1/|k+f|^(2H+1)
        s = sum([1 / (abs(x + f)**(2 * H + 1)) for x in range(-M, M + 1)])

        s += 1 / (2 * H * (M + 1 - f)**(2 * H))
        s += 1 / (2 * H * (M + 1 + f)**(2 * H))
        s -= (2 * H + 1) * (2 * H + 2) * (2 * H +
                                          3) / (720 * (M + 1 - f)**(2 * H + 4))
        s -= (2 * H + 1) * (2 * H + 2) * (2 * H +
                                          3) / (720 * (M + 1 + f)**(2 * H + 4))
        s += (2 * H + 1) / (12 * (M + 1 - f)**(2 * H + 2))
        s += (2 * H + 1) / (12 * (M + 1 + f)**(2 * H + 2))
        s += 1 / (2 * (M + 1 - f)**(2 * H + 1))
        s += 1 / (2 * (M + 1 + f)**(2 * H + 1))

        s *= 4 * gamma(2 * H + 1) * sin(pi * H) * (sin(pi * f)**2)
        s /= (2 * pi)**(2 * H + 1)

        return s
コード例 #2
0
def IntegratedSpectralDensity(H, wsteps, quadraturesteps, i):
    if(H==0.0):
        if i==0:
            return 1-2**wsteps/pi*sin(pi/2**wsteps)
        else:
            x=2**(wsteps+1-i)
            return 1-(x/pi)*sin(2*pi/x)+(x/pi)*sin(pi/x)
    elif(H==1.0):
        if i==0:
            return 2**wsteps
        else:
            return 1e-50
    else:
        if i==0:
            return gamma(2*H+1)*sin(pi*H)/(2*pi)**(2*H-1)/(1-H)*2**((wsteps+1)*(2*H-1)-1)
        else:
            scale=2**(wsteps+2-i)

            xold=1.0
            yold=SpectralDensityFunction(xold/scale,H)
            sum=0
            for j in range(1,quadraturesteps+1):
                xnew=(1+float(j)/quadraturesteps)
                ynew=SpectralDensityFunction(xnew/scale,H)
                sum+=(xnew-xold)*(ynew+yold)
                xold=xnew
                yold=ynew
            return sum/2.0
コード例 #3
0
def SpectralDensityFunction(f,H):
    '''Spectral density function (-0.5<f<0.5) for fractional Gaussian noise with Hurst Exponent H
    I don't know how to derive this formula. It is in Voichita's matlab code, and she refers to it as 
    "the almost exact formula from Percival and Walden".
    I have a feeling that it might be a Taylor series approximation to the Fourier transform of the auto-covariance relation
    for fractional Gaussian Noise.
    >>> SpectralDensityFunction(0.26,0.2367)
    1.1067908939278011
    ''' 
    if(H==0): 
        return 2*sin(pi*f)**2
    else:
        M=100  #sum from k = -M to M of 1/|k+f|^(2H+1)
        s=sum( [1/(abs(x+f)**(2*H+1)) for x in range(-M,M+1)] )
        
        s+=1/(2*H*(M+1-f)**(2*H))
        s+=1/(2*H*(M+1+f)**(2*H))
        s-=(2*H+1)*(2*H+2)*(2*H+3)/(720*(M+1-f)**(2*H+4))
        s-=(2*H+1)*(2*H+2)*(2*H+3)/(720*(M+1+f)**(2*H+4))

        s+=(2*H+1)/(12*(M+1-f)**(2*H+2))
        s+=(2*H+1)/(12*(M+1+f)**(2*H+2))
        s+=1/(2*(M+1-f)**(2*H+1))
        s+=1/(2*(M+1+f)**(2*H+1))
        
        s*=4*gamma(2*H+1)*sin(pi*H)*(sin(pi*f)**2)
        s/=(2*pi)**(2*H+1)

        return s
コード例 #4
0
def IntegratedSpectralDensity(H, wsteps, quadraturesteps, i):
    if (H == 0.0):
        if i == 0:
            return 1 - 2**wsteps / pi * sin(pi / 2**wsteps)
        else:
            x = 2**(wsteps + 1 - i)
            return 1 - (x / pi) * sin(2 * pi / x) + (x / pi) * sin(pi / x)
    elif (H == 1.0):
        if i == 0:
            return 2**wsteps
        else:
            return 1e-50
    else:
        if i == 0:
            return gamma(2 * H + 1) * sin(pi * H) / (2 * pi)**(2 * H - 1) / (
                1 - H) * 2**((wsteps + 1) * (2 * H - 1) - 1)
        else:
            scale = 2**(wsteps + 2 - i)

            xold = 1.0
            yold = SpectralDensityFunction(xold / scale, H)
            sum = 0
            for j in range(1, quadraturesteps + 1):
                xnew = (1 + float(j) / quadraturesteps)
                ynew = SpectralDensityFunction(xnew / scale, H)
                sum += (xnew - xold) * (ynew + yold)
                xold = xnew
                yold = ynew
            return sum / 2.0
コード例 #5
0
def IntegratedSpectralDensityFunction(H, wsteps, quadraturesteps=20):
    '''
    Appears to be the expected values of the wavelet coefficients of a fractional Gaussian noise.
    In the general 0<H<1 fine scale case these are calculated by doing a numerical integration
    over a region of the Spectral Density. I have no idea where this formula comes from, and
    have copied it from Voichita's matlab code (the function SDF_Int), and then clarified the calculation.
    >>> IntegratedSpectralDensityFunction(0.0,5)
    [0.0016056069643816118, 0.011220690747206885, 0.044596134335340376, 0.17386272609022058, 0.62707677142194329, 1.6366197723675813]
    >>> IntegratedSpectralDensityFunction(1.0,5)
    [32, 1e-50, 1e-50, 1e-50, 1e-50, 1e-50]
    >>> IntegratedSpectralDensityFunction(0.76,5)
    [6.4284808246144252, 2.5337868118662028, 1.7592398286153024, 1.2077211418590617, 0.8012983421742671, 0.51762057939023354]
    >>> IntegratedSpectralDensityFunction(0.76,5,10)
    [6.4284808246144252, 2.5344386424271996, 1.7596935438138646, 1.2080370431239666, 0.80152942631348534, 0.5178955503380388]
    >>> IntegratedSpectralDensityFunction(0.35,8)
    [0.16634193518773813, 0.24327887427188533, 0.29962683660583778, 0.36932052594955755, 0.45630849916626082, 0.56762788846911971, 0.71869843738552097, 0.94205671645702882, 1.2302926459188461]
    '''
    if (H == 0.0):
        c = range(wsteps + 1, 0, -1)
        c = [2.0**x for x in c]
        c = [
            1 - (x / pi) * sin(2 * pi / x) + (x / pi) * sin(pi / x) for x in c
        ]
        c[0] = 1 - 2**wsteps / pi * sin(pi / 2**wsteps)
        return c

    elif (H == 1.0):
        c = range(wsteps + 1, 0, -1)
        c = [1e-50 for x in c]
        c[0] = 2**wsteps
        return c

    else:
        c = []
        c.append(
            gamma(2 * H + 1) * sin(pi * H) / (2 * pi)**(2 * H - 1) / (1 - H) *
            2**((wsteps + 1) * (2 * H - 1) - 1))
        grid = range(quadraturesteps + 1)
        grid = [1 + x * 1.0 / quadraturesteps for x in grid]
        for i in range(wsteps + 1, 1, -1):
            fvals = [x / (2**i) for x in grid]
            SDFvals = [SpectralDensityFunction(f, H) for f in fvals]
            c.append(TrapeziumIntegration(grid, SDFvals))
        return c
コード例 #6
0
def IntegratedSpectralDensityFunction(H,wsteps,quadraturesteps=20):
    '''
    Appears to be the expected values of the wavelet coefficients of a fractional Gaussian noise.
    In the general 0<H<1 fine scale case these are calculated by doing a numerical integration
    over a region of the Spectral Density. I have no idea where this formula comes from, and
    have copied it from Voichita's matlab code (the function SDF_Int), and then clarified the calculation.
    >>> IntegratedSpectralDensityFunction(0.0,5)
    [0.0016056069643816118, 0.011220690747206885, 0.044596134335340376, 0.17386272609022058, 0.62707677142194329, 1.6366197723675813]
    >>> IntegratedSpectralDensityFunction(1.0,5)
    [32, 1e-50, 1e-50, 1e-50, 1e-50, 1e-50]
    >>> IntegratedSpectralDensityFunction(0.76,5)
    [6.4284808246144252, 2.5337868118662028, 1.7592398286153024, 1.2077211418590617, 0.8012983421742671, 0.51762057939023354]
    >>> IntegratedSpectralDensityFunction(0.76,5,10)
    [6.4284808246144252, 2.5344386424271996, 1.7596935438138646, 1.2080370431239666, 0.80152942631348534, 0.5178955503380388]
    >>> IntegratedSpectralDensityFunction(0.35,8)
    [0.16634193518773813, 0.24327887427188533, 0.29962683660583778, 0.36932052594955755, 0.45630849916626082, 0.56762788846911971, 0.71869843738552097, 0.94205671645702882, 1.2302926459188461]
    '''
    if(H==0.0):
        c=range(wsteps+1,0,-1)
        c=[2.0**x for x in c]
        c=[1-(x/pi)*sin(2*pi/x)+(x/pi)*sin(pi/x) for x in c]
        c[0]=1-2**wsteps/pi*sin(pi/2**wsteps)
        return c

    elif(H==1.0):
        c=range(wsteps+1,0,-1)
        c=[1e-50 for x in c]
        c[0]=2**wsteps
        return c

    else:
        c=[]
        c.append(gamma(2*H+1)*sin(pi*H)/(2*pi)**(2*H-1)/(1-H)*2**((wsteps+1)*(2*H-1)-1))
        grid=range(quadraturesteps+1)
        grid=[1+x*1.0/quadraturesteps for x in grid]
        for i in range(wsteps+1,1,-1):
            fvals=[x/(2**i) for x in grid]
            SDFvals=[SpectralDensityFunction(f,H) for f in fvals]
            c.append(TrapeziumIntegration(grid,SDFvals))
        return c