More SciPy#
import numpy as np
import matplotlib.pyplot as plt
from scipy import optimize
Fitting#
Fitting is used to match a model to experimental data. E.g. we have N points of \((x_i, y_i)\) with associated errors, \(\sigma_i\), and we want to find a simply function that best represents the data.
Usually this means that we will need to define a metric, often called the residual, for how well our function matches the data, and then minimize this residual. Least-squares fitting is a popular formulation.
We want to fit our data to a function \(Y(x, \{a_j\})\), where \(a_j\) are model parameters we can adjust. We want to find the optimal \(a_j\) to minimize the distance of \(Y\) from our data:
Least-squares minimizes \(\chi^2\):
general linear least squares#
First we’ll make some experimental data (a quadratic with random fashion). We use the randn() function to provide Gaussian normalized errors.
def y_experiment2(a1, a2, a3, sigma, x):
""" return the experimental data in a quadratic + random fashion,
with a1, a2, a3 the coefficients of the quadratic and sigma is
the error. This will be poorly matched to a linear fit for
a3 != 0 """
N = len(x)
# randn gives samples from the "standard normal" distribution
r = np.random.randn(N)
y = a1 + a2*x + a3*x*x + sigma*r
return y
N = 40
sigma = 5.0*np.ones(N)
x = np.linspace(0, 100.0, N)
y = y_experiment2(2.0, 1.50, -0.02, sigma, x)
fig, ax = plt.subplots()
ax.scatter(x,y)
ax.errorbar(x, y, yerr=sigma, fmt="o")
<ErrorbarContainer object of 3 artists>
def resid(avec, x, y, sigma):
""" the residual function -- this is what will be minimized by the
scipy.optimize.leastsq() routine. avec is the parameters we
are optimizing -- they are packed in here, so we unpack to
begin. (x, y) are the data points
scipy.optimize.leastsq() minimizes:
x = arg min(sum(func(y)**2,axis=0))
y
so this should just be the distance from a point to the curve,
and it will square it and sum over the points
"""
a0, a1, a2 = avec
return (y - (a0 + a1*x + a2*x**2))/sigma
# initial guesses
a0, a1, a2 = 1, 1, 1
afit, flag = optimize.leastsq(resid, [a0, a1, a2], args=(x, y, sigma))
print(afit)
[ 1.28534202 1.52602147 -0.02045754]
ax.plot(x, afit[0] + afit[1]*x + afit[2]*x*x )
fig
\(\chi^2\)
chisq = sum(np.power(resid(afit, x, y, sigma),2))
normalization = len(x)-len(afit)
print(chisq/normalization)
1.0010973439853452
a nonlinear example#
our experimental data – an exponential
a0 = 2.5
a1 = 2./3.
sigma = 5.0
a0_orig, a1_orig = a0, a1
x = np.linspace(0.0, 4.0, 25)
y = a0*np.exp(a1*x) + sigma*np.random.randn(len(x))
fig, ax = plt.subplots()
ax.scatter(x,y)
ax.errorbar(x, y, yerr=sigma, fmt="o", label="_nolegend_")
<ErrorbarContainer object of 3 artists>
our function to minimize
def resid(avec, x, y):
""" the residual function -- this is what will be minimized by the
scipy.optimize.leastsq() routine. avec is the parameters we
are optimizing -- they are packed in here, so we unpack to
begin. (x, y) are the data points
scipy.optimize.leastsq() minimizes:
x = arg min(sum(func(y)**2,axis=0))
y
so this should just be the distance from a point to the curve,
and it will square it and sum over the points
"""
a0, a1 = avec
# note: if we wanted to deal with error bars, we would weight each
# residual accordingly
return y - a0*np.exp(a1*x)
a0, a1 = 1, 1
afit, flag = optimize.leastsq(resid, [a0, a1], args=(x, y))
print(flag)
print(afit)
1
[2.50331914 0.68493187]
ax.plot(x, afit[0]*np.exp(afit[1]*x),
label=r"$a_0 = $ %f; $a_1 = $ %f" % (afit[0], afit[1]))
ax.plot(x, a0_orig*np.exp(a1_orig*x), ":", label="original function")
ax.legend(numpoints=1, frameon=False)
fig
Note
What about uncertainties in both \(x\) and \(y\)? SciPy has an orthogonal distance regression implementation based on ODRPACK for this.
FFTs#
Fourier transforms convert a physical-space (or time series) representation of a function into frequency space. This provides an equivalent representation of the data with a new view.
The FFT and its inverse in NumPy use:
Both NumPy and SciPy have FFT routines that are similar. However, the NumPy version returns the data in a more convenient form.
Tip
It’s always best to start with something you understand—let’s do a simple sine wave. Since our function is real, we can use the rfft routines in NumPy—the understand that we are working with real data and they don’t return the negative frequency components.
Important
FFTs assume that you are periodic. If you include both endpoints of the domain in the points that comprise your sample then you will not match this assumption. Here we use endpoint=False with linspace()
def single_freq_sine(npts):
# a pure sine with no phase shift will result in pure imaginary
# signal
f_0 = 0.2
xmax = 10.0/f_0
xx = np.linspace(0.0, xmax, npts, endpoint=False)
f = np.sin(2.0*np.pi*f_0*xx)
return xx, f
To make our life easier, we’ll define a function that plots all the stages of the FFT process
def plot_FFT(xx, f):
npts = len(xx)
dx = xx[1] - xx[0]
# Forward transform: f(x) -> F(k)
fk = np.fft.rfft(f)
# Normalization -- the '2' here comes from the fact that we are
# neglecting the negative portion of the frequency space, since
# the FFT of a real function contains redundant information, so
# we are only dealing with 1/2 of the frequency space.
#
# technically, we should only scale the 0 bin by N, since k=0 is
# not duplicated -- we won't worry about that for these plots
norm = 2.0 / npts
fk = fk * norm
fk_r = fk.real
fk_i = fk.imag
# rfftfreq returns the frequencies as 0, 1/N, 2/N, 3/N, ...
k = np.fft.rfftfreq(npts)
# to make these dimensional, we need to divide by dx.
kfreq = k / dx
# Inverse transform: F(k) -> f(x) -- without the normalization
fkinv = np.fft.irfft(fk/norm)
# plots
fig, ax = plt.subplots(nrows=4, ncols=1)
ax[0].plot(xx, f)
ax[0].set_xlabel("x")
ax[0].set_ylabel("f(x)")
ax[1].plot(kfreq, fk_r, label=r"Re($\mathcal{F}$)")
ax[1].plot(kfreq, fk_i, ls=":", label=r"Im($\mathcal{F}$)")
ax[1].set_xlabel(r"$\nu_k$")
ax[1].set_ylabel("F(k)")
ax[1].legend(fontsize="small", frameon=False)
ax[2].plot(kfreq, np.abs(fk))
ax[2].set_xlabel(r"$\nu_k$")
ax[2].set_ylabel(r"|F(k)|")
ax[3].plot(xx, fkinv.real)
ax[3].set_xlabel(r"$\nu_k$")
ax[3].set_ylabel(r"inverse F(k)")
f = plt.gcf()
f.set_size_inches(10,8)
plt.tight_layout()
npts = 128
xx, f = single_freq_sine(npts)
plot_FFT(xx, f)
A cosine is shifted in phase by pi/2
def single_freq_cosine(npts):
# a pure cosine with no phase shift will result in pure real
# signal
f_0 = 0.2
xmax = 10.0/f_0
xx = np.linspace(0.0, xmax, npts, endpoint=False)
f = np.cos(2.0*np.pi*f_0*xx)
return xx, f
xx, f = single_freq_cosine(npts)
plot_FFT(xx, f)
Now let’s look at a sine with a pi/4 phase shift
def single_freq_sine_plus_shift(npts):
# a pure sine with no phase shift will result in pure imaginary
# signal
f_0 = 0.2
xmax = 10.0/f_0
xx = np.linspace(0.0, xmax, npts, endpoint=False)
f = np.sin(2.0*np.pi*f_0*xx + np.pi/4)
return xx, f
xx, f = single_freq_sine_plus_shift(npts)
plot_FFT(xx, f)
A frequency filter#
we’ll setup a simple two-frequency sine wave and filter a component
def two_freq_sine(npts):
# a pure sine with no phase shift will result in pure imaginary
# signal
f_0 = 0.2
f_1 = 0.5
xmax = 10.0/f_0
# we call with endpoint=False -- if we include the endpoint, then for
# a periodic function, the first and last point are identical -- this
# shows up as a signal in the FFT.
xx = np.linspace(0.0, xmax, npts, endpoint=False)
f = 0.5*(np.sin(2.0*np.pi*f_0*xx) + np.sin(2.0*np.pi*f_1*xx))
return xx, f
npts = 256
xx, f = two_freq_sine(npts)
fig, ax = plt.subplots()
ax.plot(xx, f)
[<matplotlib.lines.Line2D at 0x7fcc94dc7dd0>]
we’ll take the transform: f(x) -> F(k)
# normalization factor: the 2 here comes from the fact that we neglect
# the negative portion of frequency space because our input function
# is real
norm = 2.0/npts
fk = norm*np.fft.rfft(f)
ofk_r = fk.real.copy()
ofk_i = fk.imag.copy()
# get the frequencies
k = np.fft.rfftfreq(len(xx))
# since we don't include the endpoint in xx, to normalize things, we need
# max(xx) + dx to get the true length of the domain
#
# This makes the frequencies essentially multiples of 1/dx
kfreq = k*npts/(max(xx) + xx[1])
fig, ax = plt.subplots()
ax.plot(kfreq, fk.real, label="real")
ax.plot(kfreq, fk.imag, ":", label="imaginary")
ax.legend(frameon=False)
<matplotlib.legend.Legend at 0x7fcc94d0e350>
Filter out the higher frequencies
fk[kfreq > 0.4] = 0.0
# element 0 of fk is the DC component
fk_r = fk.real
fk_i = fk.imag
# Inverse transform: F(k) -> f(x)
fkinv = np.fft.irfft(fk/norm)
fig, ax = plt.subplots()
ax.plot(xx, fkinv.real)
[<matplotlib.lines.Line2D at 0x7fcc94d85b50>]
Linear Algebra#
general manipulations of matrices#
you can use regular NumPy arrays or you can use a special matrix class that offers some short cuts
a = np.array([[1.0, 2.0], [3.0, 4.0]])
print(a)
print(a.transpose())
print(a.T)
[[1. 2.]
[3. 4.]]
[[1. 3.]
[2. 4.]]
[[1. 3.]
[2. 4.]]
ainv = np.linalg.inv(a)
print(ainv)
[[-2. 1. ]
[ 1.5 -0.5]]
a @ ainv
array([[1.0000000e+00, 0.0000000e+00],
[8.8817842e-16, 1.0000000e+00]])
the eye() function will generate an identity matrix (as will the identity())
print(np.eye(2))
print(np.identity(2))
[[1. 0.]
[0. 1.]]
[[1. 0.]
[0. 1.]]
Linear systems#
we can solve \({\bf A}{\bf x} = {\bf b}\) easily.
Note
Linear system solvers don’t usually compute the inverse first and then multiply by it. It is much cheaper to solve the system directly (e.g., via Gaussian elimination) than to first compute the inverse.
b = np.array([5, 7])
x = np.linalg.solve(a, b)
print(x)
[-3. 4.]
The matrix class#
A = np.matrix('1.0 2.0; 3.0 4.0')
print(A)
print(A.T)
[[1. 2.]
[3. 4.]]
[[1. 3.]
[2. 4.]]
X = np.matrix('5.0 7.0')
Y = X.T
print(A*Y)
[[19.]
[43.]]
print(A.I*Y)
[[-3.]
[ 4.]]
tridiagonal matrix solve#
Here we’ll solve the equation:
with \(g(x) = \sin(x)\), and the domain \(x \in [0, 2\pi]\), with boundary conditions \(f(0) = f(2\pi) = 0\). The solution is simply \(f(x) = -\sin(x)\).
We’ll use a grid of \(N\) points with \(x_0\) on the left boundary and \(x_{N-1}\) on the right boundary.
We difference our equation as:
We keep the boundary points fixed, so we only need to solve for the \(N-2\) interior points. Near the boundaries, our difference is:
and
We can write the system of equations for solving for the \(N-2\) interior points as:
Then we just solve \({\bf A}{\bf x} = {\bf b}\)
Note
SciPy has banded solvers that work with banded matrices like we have above. They will be much more efficient than using a solver based on a dense matrix
import scipy.linalg as linalg
# our grid -- including endpoints
N = 100
x = np.linspace(0.0, 2.0*np.pi, N, endpoint=True)
dx = x[1] - x[0]
# our source
g = np.sin(x)
# our matrix will be tridiagonal, with [1, -2, 1] on the diagonals
# we only solve for the N-2 interior points
# diagonal
d = -2 * np.ones(N-2)
# upper -- note that the upper diagonal has 1 less element than the
# main diagonal. The SciPy banded solver wants the matrix in the
# form:
#
# * a01 a12 a23 a34 a45 <- upper diagonal
# a00 a11 a22 a33 a44 a55 <- diagonal
# a10 a21 a32 a43 a54 * <- lower diagonal
#
u = np.ones(N-2)
u[0] = 0.0
# lower
l = np.ones(N-2)
l[N-3] = 0.0
# put the upper, diagonal, and lower parts together as a banded matrix
A = np.matrix([u, d, l])
# solve A sol = dx**2 g for the inner N-2 points
sol = linalg.solve_banded((1,1), A, dx**2*g[1:N-1])
fig, ax = plt.subplots()
ax.plot(x[1:N-1], sol)
[<matplotlib.lines.Line2D at 0x7fcc94bd5b50>]
