示例#1
0
文件: eval.py 项目: cygnine/spyctral
def dweighted_wiener(x,k,s=1.,t=0.,shift=0.,scale=1.):

    from numpy import sqrt, array
    from spyctral.fourier.eval import fseries as genfourier
    from spyctral.fourier.eval import dfseries as dgenfourier
    from spyctral.wiener.maps import dtheta_dx
    from spyctral.wiener.maps import x_to_theta as x2theta
    from spyctral.wiener.weights import sqrt_weight_bias as wx_sqrt
    from spyctral.wiener.weights import dsqrt_weight_bias as dwx_sqrt

    # Preprocessing and setup
    x = array(x)
    x = x.ravel()
    k = array(k,dtype=int)
    k = k.ravel()

    theta = x2theta(x,shift=shift,scale=scale)

    # First term: wx_sqrt * d/dx Phi
    psi = (dtheta_dx(x,shift=shift,scale=scale)*dgenfourier(theta,k,s-1.,t).T).T
    psi = (wx_sqrt(x,s,t,shift=shift,scale=scale)*(psi.T)).T
    
    # Second term: d/dx wx_sqrt * Phi
    psi += (dwx_sqrt(x,s,t,shift=shift,scale=scale)*genfourier(theta,k,s-1.,t).T).T

    return psi/sqrt(scale)
示例#2
0
文件: fft.py 项目: cygnine/spyctral
def fft_collocation_overhead(N,s=1.,t=0.,shift=0.,scale=1.):

    from numpy import sqrt
    from spyctral.fourier.fft import fft_overhead
    from spyctral.wiener.weights import sqrt_weight_bias as wx_sqrt
    from spyctral.wiener.quad import gq

    overhead = fft_overhead(N,gamma=s-1.,delta=t)
    x = gq(N,s=1.,t=0.,shift=shift,scale=scale)[0]
    premult = sqrt(scale)/wx_sqrt(x,s=s,t=t,shift=shift,scale=scale)

    return [premult,overhead]
示例#3
0
文件: fft.py 项目: cygnine/spyctral
def fft_collocation(f,s=1.,t=0.,shift=0.,scale=1.):

    from spyctral.fourier.fft import fft as fft_Psi
    from spyctral.wiener.weights import sqrt_weight_bias as wx_sqrt
    from spyctral.wiener.quad import gq
    from numpy import sqrt

    # This stuff can all be overhead
    N = f.size
    x = gq(N,s=1.,t=0.,shift=shift,scale=scale)[0]
    modes = f/wx_sqrt(x,s=s,t=t,shift=shift,scale=scale)

    temp = fft_Psi(modes,gamma=s-1.,delta=t)*float(sqrt(scale))
    temp[-s:] = 0
    temp[:s] = 0

    return temp
示例#4
0
文件: eval.py 项目: cygnine/spyctral
def weighted_wiener(x,k,s=1.,t=0.,shift=0.,scale=1.):

    from numpy import sqrt, array
    from spyctral.fourier.eval import fseries as genfourier
    from spyctral.wiener.maps import x_to_theta as x2theta
    from spyctral.wiener.weights import sqrt_weight_bias as wx_sqrt

    # Preprocessing and setup
    x = array(x)
    x = x.ravel()
    k = array(k,dtype=int)
    k = k.ravel()

    theta = x2theta(x,shift=shift,scale=scale)

    psi = genfourier(theta,k,s-1.,t)

    psi = (wx_sqrt((x-shift)/scale,s,t)*(psi.T)).T

    return psi/sqrt(scale)
示例#5
0
文件: fft.py 项目: cygnine/spyctral
def ifft_collocation(F,s=1.,t=0.,shift=0.,scale=1.):

    from spyctral.fourier.fft import ifft as ifft_Psi
    from spyctral.wiener.weights import sqrt_weight_bias as wx_sqrt
    from spyctral.wiener.quad import gq
    from numpy import sqrt

    from spyctral.fourier.fft import fft_overhead, ifft_online

    N = F.size

    #overhead = fft_overhead(N,g=s-1.,d=t)
    #fx = ifft_online(f,overhead)
    fx = ifft_Psi(F,gamma=s-1.,delta=t)
    
    x = gq(N,s=1.,t=0.,shift=shift,scale=scale)[0]
    fx *= wx_sqrt(x,s=s,t=t,shift=shift,scale=scale)/float(sqrt(scale))
    #print "hi"

    return fx
示例#6
0
文件: eval.py 项目: cygnine/spyctral
def xiw(x,n,s=1.,t=0.,shift=0.,scale=1.):

    from numpy import sqrt, array
    from spyctral.fourier.eval import fseries as genfourier
    from spyctral.wiener.weights import sqrt_weight_bias as wx_sqrt
    from spyctral.wiener.maps import x_to_theta as x2theta

    # Preprocessing and setup
    x = array(x)
    x = x.ravel()
    n = array(n,dtype=int)
    n = n.ravel()

    theta = x2theta(x,shift=shift,scale=scale)

    psi = genfourier(theta,n,s-1.,t).real

    psi = (wx_sqrt((x-shift)/scale,s,t)*(psi.T)).T

    psi[:,n==0] *= sqrt(2)
    psi[:,n!=0] *= 2

    return psi/sqrt(scale)