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Functions.py
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Functions.py
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# -*- coding: utf-8 -*-
"""
Created on Mon Feb 25 11:25:45 2013
@author: Ben
New functions module to concatenate all the functions needed
"""
resistivity = 0. #default to zero resistivity
force_gpu = False #Default to using cpu for ffts
def eta_switch(switch=False):
"""
Set the default value for eta
"""
if(switch):
global resistivity
resistivity = 1.4E-7
else:
global resistivity
resistivity = 0.
return
def gpu_fft_on():
"""
turn on gpu fft's
"""
global force_gpu
force_gpu = True
def gpu_fft_off():
"""
turn off gpu ffts
"""
global force_gpu
force_gpu = False
def eta():
"""
defines a constant, the resistivity
"""
return resistivity
def read_data(file_in,dens_inc=False):
"""
Reads in data from file_in.vtk into x, y, z, b, u
"""
import vtk as vtk
from vtk.util.numpy_support import vtk_to_numpy
from numpy import rollaxis, reshape, array
#Some vtk bookkeeping and object stuff
reader = vtk.vtkStructuredPointsReader()
reader.SetFileName(file_in)
reader.ReadAllVectorsOn()
reader.ReadAllScalarsOn()
reader.Update()
data = reader.GetOutput()
dim = data.GetDimensions()
nx = dim[0] - 1
ny = dim[1] - 1
nz = dim[2] - 1
D = data.GetSpacing()
N = (nx, ny, nz)
#Read the raw data from the vtk file
#u = vtk_to_numpy(data.GetCellData().GetArray('velocity')).reshape(nx, ny, nz, 3,order='F')
#b = vtk_to_numpy(data.GetCellData().GetArray('cell_centered_B')).reshape(nx, ny, nz, 3,order='F')
## #Convert to C-order and make a the 1st array index the vector component
#b = array([b[...,0].ravel(order='F').reshape(nx,ny,nz), b[...,1].ravel(order='F').reshape(nx,ny,nz), b[...,2].ravel(order='F').reshape(nx,ny,nz)])
#u = array([u[...,0].ravel(order='F').reshape(nx,ny,nz), u[...,1].ravel(order='F').reshape(nx,ny,nz), u[...,2].ravel(order='F').reshape(nx,ny,nz)])
## #Read the raw data from the vtk file
u = vtk_to_numpy(data.GetCellData().GetArray('velocity')).reshape(nz,ny,nx,3)
b = vtk_to_numpy(data.GetCellData().GetArray('cell_centered_B')).reshape(nz, ny, nx,3)
if(dens_inc):
rho = vtk_to_numpy(data.GetCellData().GetArray('density')).reshape(nz,ny,nx)
return (N,D,b.T,u.T,rho.T)
#u = ascontiguousarray(array([u[...,0], u[...,1], u[...,2]]))
#b = ascontiguousarray(array([b[...,0], b[...,1], b[...,2]]))
#u = u.transpose(3,2,1,0)
#b = b.transpose(3,2,1,0)
return (N, D, b.T, u.T)
def define_k(N, D):
"""
Creates the 3d k arrays from N and D
"""
from numpy.fft import fftfreq
from numpy import array, pi, float32
nx, ny, nz = N
dx, dy, dz = D
#Use a matlab like ndgrid to create the wave-vectors with the proper shape to take advantage of pythons vectorization
kx, ky, kz = ndgrid(fftfreq(nx, dx)*2.*pi, fftfreq(ny, dy)*2.*pi, fftfreq(nz, dz)*2.*pi, dtype=float32)
#Output a single vector
return array([kx, ky, kz], dtype = float32)
def EMF(file_in, U=None, B=None, delt=False):
"""
This function calculates the EMF (u x b). If u and b are already read in, pass them to the function to save time.
"""
if U is None or B is None: #Check if U or B are defined, otherwise read them in
N, D, U, B = read_data(file_in)
if(delt): #Make the fluctuating components if needed
u = delta(U)
b = delta(B)
return crossp(U, B), delta(crossp(U, B))
#Old parts of the code, will need revising if utilized ****
#return cross_p(U, B), delta(cross_p(u, b))
#Test Moffat 1978:
# e = -(u x <B>) - (<U> x b) - (u x b) + <u x b>
#return cross_p(U, B), -cross_p(u, (B-b)) - cross_p((U-u), b) - cross_p(u, b) + delta(cross_p(u, b))
#******
else:
return crossp(U, B)
def CurrentDensity(file_in, B=None, k=None, delt=False):
"""
Function to calculate the electric current, curl(b) in Fourier Space. If b or k are defined can pass them to speed calculation.
"""
if B is None or k is None: #Check if B or k are defined, else read in
N,D,B,U = read_data(file_in)
k = define_k(N,D)
#Calculate J in k-space,\tilde{J} = ik \cdot \tilde{B}
J = ifftvec(1.j*crossp(k, fftvec(B)))
if(delt):
return J, delta(J)
else:
return J
def CurrentHelicity(file_in, J=None, B=None, k=None, delt=False):
"""
Function to calculate the current helicity, j dot b. Faster if J and b are known.
"""
# Check how much work we have to do
if J is None:
if B is None or k is None:
N, D, B, U = read_data(file_in)
k = define_k(N, D)
J = CurrentDensity(file_in, B, k)
if(delt):
b = delta(B)
jc = delta(J)
return dot_p(J, B), LargeScale(dot_p(jc, b))
else:
return dot_p(J, B)
def helicity(u,k):
"""
Function to calculate the fluid helicity
w = u \cdot \nabla \times u
"""
return dot_p(u, ifftvec(1.j*crossp(k,fftvec(u))))
def vorticity(u,k):
"""
Function which calculates the vorticity in Fourier Space
"""
return ifftvec(1.j*crossp(k,fftvec(u)))
def Potential(file_in, J=None, E=None, k=None, D=None, N=None, delt=False):
"""
Function to calculate the vector and scalar potentials using the spectral_poisson3d function
Spectral_poisson3d takes a source term (scalar, 3d) and the grid spacing as a tuple and returns the potential
"""
from numpy import array
#Check for defined variables, read in or calculate as needed
if D is None or J is None or E is None:
N,D,B,U = read_data(file_in)
if k is None:
k = define_k(N,D)
#Call spectral_poisson3d to set the potentials and return
if E is None:
E = EMF(file_in, U, B)
if J is None:
J = CurrentDensity(file_in,B,k)
#Make a 4-vector [phi, Ax, Ay, Az] by calling the Poisson solver for each component
# The solver takes care of the fft/ifft if fft_source is True
A = array([spectral_poisson3d(-1.j*dot_p(k,fftvec(E)),D), #Phi = (ik \cdot E)/k^2 --There is a - sign in the poisson solver
spectral_poisson3d(J[0],D,fft_source=True), #Ax = -Jx/k^2
spectral_poisson3d(J[1],D,fft_source=True), #Ay = -Jy/k^2
spectral_poisson3d(J[2],D,fft_source=True) #Az = -Jz/k^2
])
if delt:
a = array([delta(A[0]), delta(A[1]), delta(A[2]), delta(A[3])])
return A, a
else:
return A
def MagneticHelicity(file_in, A=None, B=None, delt=False, large=False):
"""
Function to calculate the magnetic helicity, a dot b. Faster if a and b are known.
"""
from numpy import copy
#Again, check and see how much work is already done
if B is None:
N, D, B, U = read_data(file_in)
if A is None:
A = Potential(file_in)
A = A[1:].copy()
#H is a simple dot product
#H = A \cdot B, <H> = <A> \cdot <B>, h = <a \cdot b>
if(delt):
b = delta(B)
a = delta(A)
if(large):
#return dot_p(A, B), dot_p((A-a), (B-b)), dot_p(A, B) - dot_p((A-a), (B-b))
return dot_p(A, B), dot_p((A-a), (B-b)), LargeScale(dot_p(a, b))
else:
return dot_p(A, B), LargeScale(dot_p(a, b))
else:
return dot_p(A, B)
def MagneticHelicityFlux(file_in, A=None, E=None, delt=False, large=False):
"""
Function to calculate the flux of magnetic helicity
"""
from numpy import copy
if(delt):
N, D, B, U = read_data(file_in)
k = define_k(N,D)
E, e = EMF(file_in, U, B, delt=True)
b = delta(B)
Jc, jc = CurrentDensity(file_in, B, k, delt = True)
if A is None:
A, a = Potential(file_in, delt=True)
else:
a = A.copy()
a[0] = delta(A[0])
a[1:] = delta(A[1:])
#Split the 4-vector into the scalar and vector potentials
Phi = A[0].copy()
A = A[1:].copy()
phi = a[0].copy()
a = a[1:].copy()
#Total:
#J_H = A \times E + \Phi B + \eta J \times A
#Small scale:
#J_h = < a \times e > + <phi b> + <\eta j \times a>
#Large scale:
#<J_H> = <A> \times <E> + <\Phi B> + \eta <J> \times <A>
Jh = crossp(A, E) + Phi*B + eta()*crossp(Jc, A)
Jh_small = LargeScale(crossp(a, e)) + LargeScale(phi*b) + LargeScale(eta()*crossp(jc, a))
#Jh_small = crossp(a, e) + phi*b + eta()*crossp(jc, a)
if(large):
#Returns, Total, Small Scale, Large Scale
return Jh, Jh_small, crossp((A-a), (E-e)) + LargeScale(Phi*B) + eta()*crossp((Jc-jc), (A-a))
else:
return Jh, Jh_small
else:
if E is None:
N, D, B, U = read_data(file_in)
E = EMF(file_in, U, B)
if A is None:
A, Phi = Potential(file_in)
Phi = A[0].copy()
A = A[1:].copy()
return Jh
##Functions to manipulate data
def spectral_poisson3d(source,h,fft_source=False):
"""
Solves the 3D Poisson equation using ffts
Input the source term and a tuple of the grid spacing
EX:
phi = spectral_poisson3d(rho, (dx,dy,dz))
"""
from numpy.fft import fftfreq
from numpy import pi
nx, ny, nz = source.shape
hx, hy, hz = h
#Define the k-vector, in retrospect, I could have used the function for this
kx, ky, kz = ndgrid(fftfreq(nx,hx)*2.*pi, fftfreq(ny,hy)*2.*pi, fftfreq(nz,hz)*2.*pi)
k2 = -(kx**2 + ky**2 + kz**2)
k2[0,0,0] = 1. #Set the DC component gain = 1 (will subtract this off later anyway)
if fft_source: #If the source needs to be fft'ed
V = fftvec(-source)/k2
else: #Otherwise, just divide by k^2
V = -source/k2
V[0,0,0] = 0. #Set the DC component to 0, effective subtracts the mean from the solution
#Forces a unique solution to the periodic BC Poisson problem
return ifftvec(V)
def fftvec(vec):
"""
performs a fft on a vector with 3 components in the first index position
This is really just a wrapper for fft, fftn and their inverses
"""
try:
from anfft import fft, fftn
fft_type = 1
except:
# print "Could not import anfft, importing scipy instead."
#Update 9/18/2013 -- numpy with mkl is way faster than scipy
import mkl
mkl.set_num_threads(8)
from numpy.fft import fft, fftn
fft_type = 0
if force_gpu:
fft_type = 2 #set gpu fft's manually -- not sure what a automatic way would look like
from numpy import complex64, shape, array, empty
if vec.ndim > 2:
if vec.shape[0] == 3:
# "Vector": first index has size 3 so fft the other columns
if fft_type==1:
return array([fftn(i,measure=True) for i in vec]).astype(complex64)
# result = empty(vec.shape, dtype=complex64)
# result[0] = fftn(vec[0], measure=True).astype(complex64)
# result[1] = fftn(vec[1], measure=True).astype(complex64)
# result[2] = fftn(vec[2], measure=True).astype(complex64)
# return result
elif fft_type==0:
return fftn(vec, axes=range(1,vec.ndim)).astype(complex64)
elif fft_type==2:
# return array([gpu_fft(i) for i in vec.astype(complex64)])
result = empty(vec.shape, dtype=complex64)
result[0] = gpu_fft(vec[0].copy())
result[1] = gpu_fft(vec[1].copy())
result[2] = gpu_fft(vec[2].copy())
return result
else: # "Scalar", fft the whole thing
if fft_type==1:
return fftn(vec,measure=True).astype(complex64)
elif fft_type==0:
return fftn(vec).astype(complex64)
elif fft_type==2:
return gpu_fft(vec.copy())
elif vec.ndim == 1: #Not a vector, so use fft
if fft_type==1:
return fft(vec,measure = True).astype(complex64)
elif fft_type==0:
return fft(vec).astype(complex64)
elif fft_type==2:
return gpu_fft(vec.astype(complex64))
else:
#0th index is 3, so its a vector
#return fft(vec, axis=1).astype(complex64)
return array([fft(i) for i in vec])
def ifftvec(vec):
"""
performs a fft on a vector with 3 components in the last index position
This is a wrapper for ifft and ifftn
"""
try:
from anfft import ifft, ifftn
fft_type = 1
except:
# print "Could not import anfft, importing scipy instead."
#Update 9/18/2013 -- numpy with mkl is way faster than scipy
import mkl
mkl.set_num_threads(8)
from numpy.fft import ifft, ifftn
fft_type = 0
if force_gpu:
fft_type = 2 #set gpu fft's manually -- not sure what a automatic way would look like
from numpy import float32, real, array, empty, complex64
if vec.ndim > 2:
if vec.shape[0] == 3:
# "Vector": first index has size 3 so fft the other columns
if fft_type==1:
return array([ifftn(i,measure=True) for i in vec]).astype(float32)
# result = empty(vec.shape, dtype=float32)
# result[0] = real(ifftn(vec[0], measure=True)).astype(float32)
# result[1] = real(ifftn(vec[1], measure=True)).astype(float32)
# result[2] = real(ifftn(vec[2], measure=True)).astype(float32)
# return result
elif fft_type==0:
return ifftn(vec, axes=range(1,vec.ndim)).astype(float32)
elif fft_type==2:
# return array([gpu_ifft(i) for i in vec]).astype(float32)
result = empty(vec.shape, dtype=float32)
result[0] = gpu_ifft(vec[0].copy()).astype(float32)
result[1] = gpu_ifft(vec[1].copy()).astype(float32)
result[2] = gpu_ifft(vec[2].copy()).astype(float32)
return result
else: # "Scalar", fft the whole thing
if fft_type==1:
return ifftn(vec,measure=True).astype(float32)
elif fft_type==0:
return ifftn(vec).astype(float32)
elif fft_type==2:
return gpu_ifft(vec.copy()).astype(float32)
elif vec.ndim == 1: #Not a vector, so use fft
if fft_type==1:
return ifft(vec,measure = True).astype(float32)
elif fft_type==0:
return ifft(vec).astype(float32)
elif fft_type==2:
return gpu_ifft(vec).astype(float32)
else:
#0th index is 3, so its a vector
#return fft(vec, axis=1).astype(complex64)
return array([ifft(i) for i in vec]).astype(float32)
def gpu_fft(vec):
"""
Uses the pyopencl and pyfft libraries to perform an fft on the GPU
"""
from pyfft.cl import Plan as cl_plan
import pyopencl as cl
import pyopencl.array as cl_array
from numpy import complex64, shape, float32, complex128
print vec.shape
array_size = vec.shape
#Find the GPU's available
platform = cl.get_platforms()
my_gpu_devices = platform[0].get_devices(device_type=cl.device_type.GPU)
#Create a context using the GPU's found in the above step
ctx = cl.Context(devices=my_gpu_devices)
#Create queue using that context
queue = cl.CommandQueue(ctx)
#create a plan based on the size of the array
#Make a temporary copy of vec so that things don't get all messed up
plan = cl_plan(array_size, dtype=complex64, queue=queue)
# plan = cl_plan(array_size,queue=queue)
alloc = cl.tools.ImmediateAllocator(queue)
cl.tools.MemoryPool(alloc).stop_holding()
#temp = vec.copy().astype(complex64)
#gpu_data = cl_array.to_device(queue, temp)
vec = vec.astype(complex64)
cl.enqueue_barrier(queue)
gpu_data = cl_array.to_device(queue, vec, allocator = alloc, async = True)
gpu_data.queue.finish()
cl.enqueue_barrier(queue)
plan.execute(gpu_data.data)
cl.enqueue_barrier(queue)
ans = gpu_data.get()
gpu_data.data.release()
gpu_data.queue.finish()
queue.flush()
for i in range(20):
pass
return ans
def gpu_ifft(vec):
"""
Uses the pyopencl and pyfft libraries to perform an fft on the GPU
"""
from pyfft.cl import Plan as cl_plan
import pyopencl as cl
import pyopencl.array as cl_array
from numpy import complex64, shape, complex128, float32, real
array_size = vec.shape
#Find the GPU's available
platform = cl.get_platforms()
my_gpu_devices = platform[0].get_devices(device_type=cl.device_type.GPU)
#Create a context using the GPU's found in the above step
ctx = cl.Context(devices=my_gpu_devices)
#Create queue using that context
queue = cl.CommandQueue(ctx)
# plan = cl_plan(array_size,queue=queue)
#Make a temporary copy of vec so that things don't get all messed up
##temp = vec.copy().astype(complex64)
plan = cl_plan(array_size, dtype=complex64, queue=queue)
# plan = cl_plan(array_size,queue=queue)
alloc = cl.tools.ImmediateAllocator(queue)
cl.tools.MemoryPool(alloc).stop_holding()
##gpu_data = cl_array.to_device(queue, temp)
vec = vec.astype(complex64)
cl.enqueue_barrier(queue)
gpu_data = cl_array.to_device(queue, vec, allocator = alloc, async = True)
gpu_data.queue.finish()
cl.enqueue_barrier(queue)
plan.execute(gpu_data.data, inverse=True)
cl.enqueue_barrier(queue)
ans = gpu_data.get()
gpu_data.data.release()
gpu_data.queue.finish()
queue.flush()
for i in range(20):
pass
return ans
def power_spectrum(x):
"""
Calculates the power spectrum of a (nx,ny,nz) array as a function of kz
"""
from numpy import conjugate, shape
nx,ny,nz = x.shape
x_ = fftvec(x)
x_[0,0,0] = 0.
return sum(sum(x_*conjugate(x_),0),0)[:nz/2]/(nx*ny*nz)
def weighted_power_spectrum(x,kz):
"""
Calculates the power spectrum times kz
"""
from numpy import conjugate, shape
nx,ny,nz = x.shape
x_ = fftvec(x)
x_[0,0,0] = 0.
return sum(sum(x_*conjugate(x_),0),0)[:nz/2]/(nx*ny*nz)*kz[:nz/2]
def zaverage(a):
"""
Takes a 3D array and computes the average over the x-y plane
If the first index has size 3, its a vector so output will be a vector
"""
from numpy import mean
if a.shape[0] == 3:
return mean(mean(a, -2), -2)
else:
return mean(mean(a, 0), 0)
def lowpass(a, window='hamming', alpha=0.1, fc = 1./64.):
"""
Function which takes the num_ks smallest k-value positions in each dimension and filters the rest.
The input is expected to be of the form a[3,...] for a vector.
Alpha defines the sharpness of the filter window if hamming is chosen
fc is the cutoff frequency relative to the nyquist frequency
"""
from numpy import shape,ones,zeros,float32
#Does the filtering in 1 line
# -FFT
# -Window the data
# -IFFT
#Create a rectangular window
if(window=='rectangular'):
return ifftvec(create_filter(a.shape, fc,alpha, rect=True)*fftvec(a))
if(window=='hamming'):#Or create a "hamming" window
return ifftvec(create_filter(a.shape, fc, alpha)*fftvec(a))
def highpass(a, window='hamming', alpha=0.1, fc=1./64.):
"""
This function does the same sort of thing as lowpass, except it passes the high k components set by fc
"""
from numpy import shape,ones,float32
#Does the filtering in 1 line
# -FFT
# -Window the data
# -IFFT
#create_filter creates a lowpass window, so need to do a 1 - filter
#Create a rectangular window
if(window=='rectangular'):
return ifftvec((1.-create_filter(a.shape, fc, alpha,rect=True))*fftvec(a))
if(window=='hamming'):#Or create a "hamming" window
return ifftvec((1.-create_filter(a.shape, fc, alpha))*fftvec(a))
def tukey_filter(width, alpha):
"""
Creates a window with length width and sharpness alpha
1 is a cosine (Hamming)
0 is a rectangle/boxcar/brickwall (passing 0 will actually give a divide by zero, so don't do that)
"""
from numpy import arange, ones, cos, pi, float32
#create the x values to pass to the function
x = arange(width).astype(float32)
#Do some fancy slicing with numpy arrays to create a piecwise function
p1 = slice(None, int(alpha*(width-1)/2))
p2 = slice(int(alpha*(width-1)/2), int((width-1)*(1-alpha/2)))
p3 = slice( int((width-1)*(1-alpha/2)), int(width-1) )
#Set default values to 1
result = ones(width)
#Create the piecewise function
result[p1] = 0.5*(1.+cos(pi*(2.*x[p1]/alpha/(width-1)-1.)))
result[p2] = 1.
result[p3] = 0.5*(1.+cos(pi*(2.*x[p3]/alpha/(width-1)-alpha/2.+1.)))
if width%2 == 0:
result[:-width/2:-1] = result[:width/2-1] #mirror the window to work in k-space
else:
result[:-width/2:-1] = result[:width/2]
return result
def create_filter(axis_dimensions, fc, alpha, rect=False):
"""
Creates the 3D filter mask to be multiplied by the signal
"""
from numpy import append, insert, ones, zeros, hstack, float32
#If its a vector, only look at 1: indeces
if axis_dimensions[0] == 3:
ad = axis_dimensions[1:]
else:
ad = axis_dimensions
fcx = int(ad[0]/2*fc)
fcy = int(ad[1]/2*fc)
fcz = int(ad[2]/2*fc)
if(rect):
# filter = zeros(ad,dtype=float32)
# filter[:1,:,:]=1.
# filter[:,:4,:]=1.
# filter[:,:,:4]=1.
# filter[-1:,:,:]=1.
# filter[:,-4:,:]=1.
# filter[:,:,-4:]=1.
# return filter
f1 = zeros(ad[0])
f2 = zeros(ad[1])
f3 = zeros(ad[2])
f1[:2]=1.
f2[:8]=1.
f3[:8]=1.
f1[-2:]=1.
f2[-8:]=1.
f2[-8:]=1.
# f1 = zeros(ad[0]-fcx)
# f2 = zeros(ad[1]-fcy)
# f3 = zeros(ad[2]-fcz)
# f1 = hstack((ones(fcx/2),f1,ones(fcx/2)))
# f2 = hstack((ones(fcy/2),f2,ones(fcy/2)))
# f3 = hstack((ones(fcz/2),f3,ones(fcz/2)))
else:
#Create the 1D filters in each dimension
f1 = 1.-tukey_filter(ad[0]-fcx, alpha)
f2 = 1.-tukey_filter(ad[1]-fcy, alpha)
f3 = 1.-tukey_filter(ad[2]-fcz, alpha)
#Pad the ones on the ends up to the cutoff desired
f1 = hstack((ones((ad[0]-f1.size)/2),f1,ones((ad[0]-f1.size)/2)))
f2 = hstack((ones((ad[1]-f2.size)/2),f2,ones((ad[1]-f2.size)/2)))
f3 = hstack((ones((ad[2]-f3.size)/2),f3,ones((ad[2]-f3.size)/2)))
if f1.size != ad[0]:
f1 = insert(f1, ad[0]/2, 0.)
if f2.size != ad[1]:
f2 = insert(f2, ad[1]/2, 0.)
if f3.size != ad[2]:
f3 = insert(f3, ad[2]/2, 0.)
#This effectively does an outer product to create the array mask
f1, f2, f3 = ndgrid(f1,f2,f3)
return f1*f2*f3 #This is the actual outer product to make the mask
def dot_p(a, b):
"""
Custom dot product function for (3, nx, ny, nz) sized arrays
DOES NOT COMPLEX CONJUGATE
*** Beware *** No checking is done about the size of the input arrays, you've been warned
This should actually work for any array with 3 as the first index deonoting vector components.
So long as they are the same shape (or can broadcast)
"""
#Because of the way python-numpy arrays work, if the input are arrays, this is the sames as:
# b[0,...]*a[0,...] etc.
return sum(i*j for i,j in zip(a,b))
#return b[0]*a[0] + b[1]*a[1] + b[2]*a[2]
def crossp(a, b):
"""
Custom cross product routine for (3, nx, ny, nz) sized arrays
The same warnings as the dot_p function apply. Interestingly, I could also make this a wrapper for
numpy.cross(a, b, axis=0) as it does the same thing
"""
from numpy import array
return array([a[1]*b[2]-a[2]*b[1], a[2]*b[0]-a[0]*b[2], a[0]*b[1]-a[1]*b[0]])
def mag(x):
"""
Computes the vector magnitude
"""
from numpy import sqrt
return sqrt(sum(i**2 for i in x))
def LargeScale(x):
"""
Takes a lowpass of the data
"""
#return lowpass(x,window='rectangular',fc=8./64.)
#return lowpass(x,window = 'rectangular', fc=1./64.)
#return lowpass(x,window='hamming',alpha=0.001,fc=1./64.)
return lowpass(x,window='rectangular',alpha=0.1,fc=1./64.)
def delta(x):
"""
Takes effectively a highpass of the data
a = A - <A>
"""
#return x - LargeScale(x)
#return highpass(x,window='hamming',alpha=0.001,fc=1./64.)
return highpass(x,window='rectangular',alpha=0.1,fc=1./64.)
def dh_dt(files_in,dt,back=False):
"""
Takes a 5 point stencil time derivative of h (Note, small scale only)
"""
from numpy import array
if len(files_in) == 4:
#co = array([1./12./dt, -2./3./dt, +2./3./dt, -1./12./dt])
co = array([-3./10./dt, -1./10./dt, +1./10./dt, 3./10./dt])
else:
if back:
co = array([-1., 1.])/dt
else:
co = array([-1./2./dt, 1./2./dt])
dh = 0.
dH = 0.
for x,i in zip(files_in,range(len(files_in))):
H, h= MagneticHelicity(x,delt=True)
dh += co[i]*h
dH += co[i]*H
return dh, dH
def ndgrid(*args, **kwargs):
"""
n-dimensional gridding like Matlab's NDGRID
The input *args are an arbitrary number of numerical sequences,
e.g. lists, arrays, or tuples.
The i-th dimension of the i-th output argument
has copies of the i-th input argument.
Optional keyword argument:
same_dtype : If False (default), the result is an ndarray.
If True, the result is a lists of ndarrays, possibly with
different dtype. This can save space if some *args
have a smaller dtype than others.
Typical usage:
>>> x, y, z = [0, 1], [2, 3, 4], [5, 6, 7, 8]
>>> X, Y, Z = ndgrid(x, y, z) # unpacking the returned ndarray into X, Y, Z
Each of X, Y, Z has shape [len(v) for v in x, y, z].
>>> X.shape == Y.shape == Z.shape == (2, 3, 4)
True
>>> X
array([[[0, 0, 0, 0],
[0, 0, 0, 0],
[0, 0, 0, 0]],
[[1, 1, 1, 1],
[1, 1, 1, 1],
[1, 1, 1, 1]]])
>>> Y
array([[[2, 2, 2, 2],
[3, 3, 3, 3],
[4, 4, 4, 4]],
[[2, 2, 2, 2],
[3, 3, 3, 3],
[4, 4, 4, 4]]])
>>> Z
array([[[5, 6, 7, 8],
[5, 6, 7, 8],
[5, 6, 7, 8]],
[[5, 6, 7, 8],
[5, 6, 7, 8],
[5, 6, 7, 8]]])
With an unpacked argument list:
>>> V = [[0, 1], [2, 3, 4]]
>>> ndgrid(*V) # an array of two arrays with shape (2, 3)
array([[[0, 0, 0],
[1, 1, 1]],
[[2, 3, 4],
[2, 3, 4]]])
For input vectors of different data types, same_dtype=False makes ndgrid()
return a list of arrays with the respective dtype.
>>> ndgrid([0, 1], [1.0, 1.1, 1.2], same_dtype=False)
[array([[0, 0, 0], [1, 1, 1]]),
array([[ 1. , 1.1, 1.2], [ 1. , 1.1, 1.2]])]
Default is to return a single array.
>>> ndgrid([0, 1], [1.0, 1.1, 1.2])
array([[[ 0. , 0. , 0. ], [ 1. , 1. , 1. ]],
[[ 1. , 1.1, 1.2], [ 1. , 1.1, 1.2]]])
"""
from numpy import array, zeros, ones_like, append, shape
same_dtype = kwargs.get("same_dtype", True)
V = [array(v) for v in args] # ensure all input vectors are arrays
shape = [len(v) for v in args] # common shape of the outputs
result = []
for i, v in enumerate(V):
# reshape v so it can broadcast to the common shape
# http://docs.scipy.org/doc/numpy/user/basics.broadcasting.html
zero = zeros(shape, dtype=v.dtype)
thisshape = ones_like(shape)
thisshape[i] = shape[i]
result.append(zero + v.reshape(thisshape))
if same_dtype:
return array(result) # converts to a common dtype
else:
return result # keeps separate dtype for each output
### These functions are sort of kludges, they take time averages etc and save binary files to disk to conserve memory
# Function to take time averages and save data to disk
def gen_t_averages():
"""
Take in all the time slices and average them, this function needs to be edited to produce the right files
I think a glob.glob might be appropriate here...
"""
from numpy import array
#fp is the path to the directory where the time slices are kept
#fp = '/1/home/jackelb/Research/AthenaDumps/AthenaDumps/strat64z6/'
#fp = '/1/home/jackelb/Research/AthenaDumps/AthenaDumps/128/'
fp = '/1/home/jackelb/Research/AthenaDumps/AthenaDumps/strat128z4/'
#ts are the time stamps of the individual files in the syntax: _xxxx
#ts = array(['_1160', '_1164', '_1168', '_1172', '_1176', '_1180'])
#ts = array(['_0101','_0102','_0103','_0104'])
ts = array(['_1229','_1230','_1231','_1232'])
##ts = array(['_1180', '_1181', '_1182'])
#t_slice is the name of the time slice files with timestamp
#t_slice = array(['Strat.1160.vtk', 'Strat.1164.vtk', 'Strat.1168.vtk', 'Strat.1172.vtk',
# 'Strat.1176.vtk', 'Strat.1180.vtk'])
#t_slice = array(['Strat.0101.vtk', 'Strat.0102.vtk', 'Strat.0103.vtk', 'Strat.0104.vtk'])
t_slice = array(['Strat.1229.vtk', 'Strat.1230.vtk', 'Strat.1231.vtk', 'Strat.1232.vtk'])
##t_slice = array(['Strat.1180.vtk', 'Strat.1181.vtk', 'Strat.1182.vtk'])
#make the variable files
remake = True
if(remake==True):
for i in range(len(ts)):
make_variable_files(fp, t_slice[i], ts[i])
#make the time averages
qs = array(['B', 'U', 'E', 'J', 'H', 'Hc', 'H_t', 'JH', 'Potential'])
#ts = array(['_1160.npy', '_1164.npy', '_1168.npy', '_1172.npy', '_1176.npy', '_1180.npy'])
#ts = array(['_0101.npy','_0102.npy','_0103.npy','_0104.npy'])
ts = array(['_1229.npy','_1230.npy','_1231.npy','_1232.npy'])
##ts = array(['_1180.npy', '_1181.npy', '_1182.npy'])
for i in range(len(qs)):
time_average(fp, qs[i], ts)
def make_variable_files(file_prefix, time_stamp, file_suffix):
"""
Outputs numpy files for all the variables
"""
from numpy import save
file_in = file_prefix+time_stamp
print 'Reading from', file_in
N, D, B, U = read_data(file_in)
k = define_k(N, D)
b = B - delta(B)
u = U - delta(U)
print 'Writing', file_prefix + 'B' + file_suffix
save(file_prefix+'B'+file_suffix, (B, b))
print 'Writing', file_prefix + 'U' + file_suffix
save(file_prefix+'U'+file_suffix, (U, u))
#u = []
#b = []
E, e = EMF(file_in, U, B, delt=True)
print 'Writing', file_prefix + 'E' + file_suffix
save(file_prefix+'E'+file_suffix, (E, e))
J, jc = CurrentDensity(file_in, B, k, delt=True)
print 'Writing', file_prefix + 'Jc' + file_suffix
save(file_prefix+'J'+file_suffix, (J, jc))
H_t = dot_p( 2.*LargeScale(B), LargeScale(crossp(u, b)))
print 'Writing', file_prefix + 'H_t' + file_suffix
save(file_prefix+'H_t'+file_suffix, (H_t))
jc = []
b = []
H_t = []
e = []
u = []
Hc, hc = CurrentHelicity(file_in, J, B, k, delt=True)
print 'Writing', file_prefix + 'Hc' + file_suffix
save(file_prefix+'Hc'+file_suffix, (Hc, hc))
Hc = []
hc = []
Pot_4, pot_4 = Potential(file_in, J, E, k, delt=True)
print 'Writing', file_prefix + 'Potential' + file_suffix
save(file_prefix+'Potential'+file_suffix, (Pot_4, pot_4))
pot_4 = []
J = []
J_H, J_h, J_h_alt = MagneticHelicityFlux(file_in, Pot_4, E, delt=True, large=True)
print 'Writing', file_prefix + 'Jh' + file_suffix
save(file_prefix+'JH'+file_suffix, (J_H, J_h, J_h_alt))
J_H = []
J_h = []
J_h_alt
E = []
H, h = MagneticHelicity(file_in, Pot_4, B, delt=True)
print 'Writing', file_prefix + 'H' + file_suffix
save(file_prefix+'H'+file_suffix, (H, h))
return
def time_average(file_prefix, quantity, time_stamp):
"""
Function to take the time average of a set of data
"""
from numpy import zeros, float32, load, mean, save
if(quantity=='JH'):
print 'Loading data from', file_prefix+quantity
JH,Jh,Jh_alt = load(file_prefix+quantity+time_stamp[0])
JH = zeros(JH.shape + time_stamp.shape, dtype=float32)
Jh = zeros(JH.shape, dtype=float32)
Jh_alt = zeros(JH.shape, dtype=float32)
for i in range(len(time_stamp)):
JH[...,i], Jh[...,i], Jh_alt[...,i] = load(file_prefix+quantity+time_stamp[i])
save(file_prefix+quantity, (mean(JH, -1), mean(Jh, -1), mean(Jh_alt, -1)))
elif(quantity=='H_t'):
print 'Loading data from', file_prefix+quantity
H_t = load(file_prefix+quantity+time_stamp[0])
H_t = zeros(H_t.shape + time_stamp.shape, dtype=float32)
for i in range(len(time_stamp)):
H_t[..., i] = load(file_prefix+quantity+time_stamp[i])
save(file_prefix+quantity, mean(H_t, -1))
else:
#print 'Loading data from', file_prefix+quantity
Q, q = load(file_prefix+quantity+time_stamp[0])
Q = zeros(Q.shape+time_stamp.shape, dtype=float32)
q = zeros(q.shape+time_stamp.shape, dtype=float32)
for i in range(len(time_stamp)):
print 'Loading', file_prefix+quantity+time_stamp[i]
Q[..., i], q[..., i] = load(file_prefix+quantity+time_stamp[i])
save(file_prefix+quantity, (mean(Q, -1), mean(q, -1)))
##Plotting Functions
def plot_vec(x, y, titlear, x_label, y_label, filename):
"""
Function which plots a vector in 3 side by side plots
"""
from matplotlib.pyplot import figure, gcf, subplot, plot, title, xlabel, ylabel, tight_layout, savefig, close
figure
gcf().set_size_inches((8, 18.))
for ii in range(3):
subplot(3, 1, ii+1)
plot(x, y[ii], '+')
title(titlear[ii])
xlabel(x_label[ii])
ylabel(y_label[ii])
tight_layout()
savefig(filename)
close()
return
def plot_2vec(x, y1, y2, titles, xlabels, ylabels, filename):
"""
Function which plots the averages and lowpass filters
"""
from matplotlib.pyplot import figure, gcf, subplot, plot, title, xlabel, ylabel, tight_layout, savefig, close, gca
figure
gcf().set_size_inches((8.5, 11))
for ii in range(3):
subplot(3, 2, 2*ii+1)
plot(x, y1[ii], '+')
title(titles[ii])
xlabel(xlabels[ii])
ylabel(ylabels[ii])
xa, xb = gca().get_xlim()