I have an algorith that seeks to multiply two functions and integrate the result. One is a small normal distribution around 1.0, with a small standard deviation of abouty .1; the other is also a normal, but much larger, with mean 100,000 and stdev 15,000.
The code looks like so:
def integrand(x, z, mu, sigma) :
# goal is to return return f_x(x)*f_y(z/x)*1/abs(x)
# return normal(x, mu, sigma) * normal(z/x, 100000, 15000)/abs(x)
return normal(z/x, mu, sigma) * normal(x, 100000, 15000)/abs(x)
pResult = quad(integrand, -10000000,10000000,
args=(_z, MU, SIGMA),
points = [1.0, 2.0, 100000.0],
epsabs = 1, epsrel = .01)
This is a formula for multiplying random variables, Z = XY. It would seem that I could swap where the z/x goes in the integrand, but in trying to see which way runs faster (by commenting out one of the two return statements in integrand()) I was surprised to get different results (one is 114,221.4 and the other is 116,174.2). Any idea why?
Also, when I cycle through a wide range of z values and plot P(z) vs z, the graphs look different, One looks right (like a normal distribution - using the first return statement) and the other looks like a top-hat with soft corners.
The math for this algorithm: https://en.wikipedia.org/wiki/Product_distribution
Scaling matters, as I noted in the answer to your previous question, and recommended to use points to help quad locate relatively small features.
You rescale the function but keep the same interval of integration. Assuming the function essentially "fits" in the interval (the tails outside of the interval are negligible), the difference is due to the algorithm being able or unable to locate the small feature of the function (the narrow Gaussian) within the interval of integration. The more narrow is the function support, the more likely is quad to get integration wrong.
I also recommend putting accuracy as the top priority; speed comes after that. It's easy to write a function that returns "0" quickly.
Related
I would like to implement a function in python (using numpy) that takes a mathematical function (for ex. p(x) = e^(-x) like below) as input and generates random numbers, that are distributed according to that mathematical-function's probability distribution. And I need to plot them, so we can see the distribution.
I need actually exactly a random number generator function for exactly the following 2 mathematical functions as input, but if it could take other functions, why not:
1) p(x) = e^(-x)
2) g(x) = (1/sqrt(2*pi)) * e^(-(x^2)/2)
Does anyone have any idea how this is doable in python?
For simple distributions like the ones you need, or if you have an easy to invert in closed form CDF, you can find plenty of samplers in NumPy as correctly pointed out in Olivier's answer.
For arbitrary distributions you could use Markov-Chain Montecarlo sampling methods.
The simplest and maybe easier to understand variant of these algorithms is Metropolis sampling.
The basic idea goes like this:
start from a random point x and take a random step xnew = x + delta
evaluate the desired probability distribution in the starting point p(x) and in the new one p(xnew)
if the new point is more probable p(xnew)/p(x) >= 1 accept the move
if the new point is less probable randomly decide whether to accept or reject depending on how probable1 the new point is
new step from this point and repeat the cycle
It can be shown, see e.g. Sokal2, that points sampled with this method follow the acceptance probability distribution.
An extensive implementation of Montecarlo methods in Python can be found in the PyMC3 package.
Example implementation
Here's a toy example just to show you the basic idea, not meant in any way as a reference implementation. Please refer to mature packages for any serious work.
def uniform_proposal(x, delta=2.0):
return np.random.uniform(x - delta, x + delta)
def metropolis_sampler(p, nsamples, proposal=uniform_proposal):
x = 1 # start somewhere
for i in range(nsamples):
trial = proposal(x) # random neighbour from the proposal distribution
acceptance = p(trial)/p(x)
# accept the move conditionally
if np.random.uniform() < acceptance:
x = trial
yield x
Let's see if it works with some simple distributions
Gaussian mixture
def gaussian(x, mu, sigma):
return 1./sigma/np.sqrt(2*np.pi)*np.exp(-((x-mu)**2)/2./sigma/sigma)
p = lambda x: gaussian(x, 1, 0.3) + gaussian(x, -1, 0.1) + gaussian(x, 3, 0.2)
samples = list(metropolis_sampler(p, 100000))
Cauchy
def cauchy(x, mu, gamma):
return 1./(np.pi*gamma*(1.+((x-mu)/gamma)**2))
p = lambda x: cauchy(x, -2, 0.5)
samples = list(metropolis_sampler(p, 100000))
Arbitrary functions
You don't really have to sample from proper probability distributions. You might just have to enforce a limited domain where to sample your random steps3
p = lambda x: np.sqrt(x)
samples = list(metropolis_sampler(p, 100000, domain=(0, 10)))
p = lambda x: (np.sin(x)/x)**2
samples = list(metropolis_sampler(p, 100000, domain=(-4*np.pi, 4*np.pi)))
Conclusions
There is still way too much to say, about proposal distributions, convergence, correlation, efficiency, applications, Bayesian formalism, other MCMC samplers, etc.
I don't think this is the proper place and there is plenty of much better material than what I could write here available online.
The idea here is to favor exploration where the probability is higher but still look at low probability regions as they might lead to other peaks. Fundamental is the choice of the proposal distribution, i.e. how you pick new points to explore. Too small steps might constrain you to a limited area of your distribution, too big could lead to a very inefficient exploration.
Physics oriented. Bayesian formalism (Metropolis-Hastings) is preferred these days but IMHO it's a little harder to grasp for beginners. There are plenty of tutorials available online, see e.g. this one from Duke university.
Implementation not shown not to add too much confusion, but it's straightforward you just have to wrap trial steps at the domain edges or make the desired function go to zero outside the domain.
NumPy offers a wide range of probability distributions.
The first function is an exponential distribution with parameter 1.
np.random.exponential(1)
The second one is a normal distribution with mean 0 and variance 1.
np.random.normal(0, 1)
Note that in both case, the arguments are optional as these are the default values for these distributions.
As a sidenote, you can also find those distributions in the random module as random.expovariate and random.gauss respectively.
More general distributions
While NumPy will likely cover all your needs, remember that you can always compute the inverse cumulative distribution function of your distribution and input values from a uniform distribution.
inverse_cdf(np.random.uniform())
By example if NumPy did not provide the exponential distribution, you could do this.
def exponential():
return -np.log(-np.random.uniform())
If you encounter distributions which CDF is not easy to compute, then consider filippo's great answer.
I have this set of experimental data:
x_data = np.array([0, 2, 5, 10, 15, 30, 60, 120])
y_data = np.array([1.00, 0.71, 0.41, 0.31, 0.29, 0.36, 0.26, 0.35])
t = np.linspace(min(x_data), max(x_data), 151)
scatter plot
I want to fit them with a curve that follows an exponential behaviour for t < t_lim and a linear behaviour for t > t_lim, where t_lim is a value that i can set as i want. I want to use curve_fit to find the best fit. I would like to find the best fit meeting these two conditions:
The end point of the first behaviour (exponential) must be the starting point of the second behaviour (linear): in other words, I don't want the jump discontinuity in the middle.
I would like the second behaviour (linear) to be descending.
I solved in this way:
t_lim = 15
def y(t, k, m, q):
return np.concatenate((np.exp(-k*t)[t<t_lim], (m*t + q)[t>=t_lim]))
popt, pcov = curve_fit(y, x_data, y_data, p0=[0.5, -0.005, 0.005])
y_model = y(t, k_opt, m_opt, q_opt)
I obtain this kind of curve:
chart_plot
I don't know how to tell python to find the best values of m, k, q that meet the two conditions (no jump discontinuity, and m < 0)
Instead of trying to add these conditions as explicit constraints, I'd go about modifying the form of y so that these conditions are always satisfied.
For example, try replacing m with -m**2. That way, the coefficient in the linear part will always be negative.
For the continuity condition, how about this: For an exponential with a given decay factor and a linear curve with a given slope which are supposed to meet at a given t_lim there's only exactly one value for q that will satisfy that condition. You can explicitly compute that value and just plug that in.
Basically, q won't be a fit parameter anymore; instead, inside of y, you'd compute the correct q value based on k, m, t_lim.
This post is not a direct answer to the question. This is a preliminary study.
First : Fitting to a simple exponential function with only a constant (without decreasing or increasing linear part) :
The result is not bad considering the wide scatter on the right part.
Second : Fitting to an exponential function with a linear function (without taking account of the expected decreasing on the right).
The slope of the linear part is very low : 0.000361
But the slope is positive which is not as wanted.
Since the scatter is very large one suspects that the slope of the linear function might be governed mainly by the scatter. In order to check this hypothesis one make the same fitting calculus whitout one point. Taking only the seven first points (that is forgetting the eighth point) the result is :
Now the slope is negative as wanted. But this is an untruthful result.
Of course if some technical reason implies that the slope is necessarily negative one could use a picewise function made of an exponenlial and a linear function. But what is the credibility of such a model ?
This doesn't answer to the question. Neverthelss I hope that this inspection will be of interest.
For information :
The usual nonlinear regression methods are often non convergent in case of large scatter due to the difficulty to set initial values of the parameters sufficienly close to the unknown correct values. In order to avoid the difficulty the above fittings where made with a non usual method which doesn't requires "guessed" initial value. For the principle refer to : https://fr.scribd.com/doc/14674814/Regressions-et-equations-integrales
In the referenced document the case of the function exponential and linear isn't fully treated. In order to overcome this deficiency the method is shown below with the numerical calculus (MathsCAD).
If more accuracy is needed use a nonlinear regression software with the values of p,a,b,c found above as initial values to start the iterative calculus.
There is a function which determine the intensity of the Fraunhofer diffraction pattern of a circular aperture... (more information)
Integral of the function in distance x= [-3.8317 , 3.8317] must be about 83.8% ( If assume that I0 is 100) and when you increase the distance to [-13.33 , 13.33] it should be about 95%.
But when I use integral in python, the answer is wrong.. I don't know what's going wrong in my code :(
from scipy.integrate import quad
from scipy import special as sp
I0=100.0
dist=3.8317
I= quad(lambda x:( I0*((2*sp.j1(x)/x)**2)) , -dist, dist)[0]
print I
Result of the integral can't be bigger than 100 (I0) because this is the diffraction of I0 ... I don't know.. may be scaling... may be the method! :(
The problem seems to be in the function's behaviour near zero. If the function is plotted, it looks smooth:
However, scipy.integrate.quad complains about round-off errors, which is very strange with this beautiful curve. However, the function is not defined at 0 (of course, you are dividing by zero!), hence the integration does not go well.
You may use a simpler integration method or do something about your function. You may also be able to integrate it to very close to zero from both sides. However, with these numbers the integral does not look right when looking at your results.
However, I think I have a hunch of what your problem is. As far as I remember, the integral you have shown is actually the intensity (power/area) of Fraunhofer diffraction as a function of distance from the center. If you want to integrate the total power within some radius, you will have to do it in two dimensions.
By simple area integration rules you should multiply your function by 2 pi r before integrating (or x instead of r in your case). Then it becomes:
f = lambda(r): r*(sp.j1(r)/r)**2
or
f = lambda(r): sp.j1(r)**2/r
or even better:
f = lambda(r): r * (sp.j0(r) + sp.jn(2,r))
The last form is best as it does not suffer from any singularities. It is based on Jaime's comment to the original answer (see the comment below this answer!).
(Note that I omitted a couple of constants.) Now you can integrate it from zero to infinity (no negative radii):
fullpower = quad(f, 1e-9, np.inf)[0]
Then you can integrate from some other radius and normalize by the full intensity:
pwr = quad(f, 1e-9, 3.8317)[0] / fullpower
And you get 0.839 (which is quite close to 84 %). If you try the farther radius (13.33):
pwr = quad(f, 1e-9, 13.33)
which gives 0.954.
It should be noted that we introduce a small error by starting the integration from 1e-9 instead of 0. The magnitude of the error can be estimated by trying different values for the starting point. The integration result changes very little between 1e-9 and 1e-12, so they seem to be safe. Of course, you could use, e.g., 1e-30, but then there may be numerical instability in the division. (In this case there isn't, but in general singularities are numerically evil.)
Let us do one thing still:
import matplotlib.pyplot as plt
import numpy as np
x = linspace(0.01, 20, 1000)
intg = np.array([ quad(f, 1e-9, xx)[0] for xx in x])
plt.plot(x, intg/fullpower)
plt.grid('on')
plt.show()
And this is what we get:
At least this looks right, the dark fringes of the Airy disk are clearly visible.
What comes to the last part of the question: I0 defines the maximum intensity (the units may be, e.g. W/m2), whereas the integral gives total power (if the intensity is in W/m2, the total power is in W). Setting the maximum intensity to 100 does not guarantee anything about the total power. That is why it is important to calculate the total power.
There actually exists a closed form equation for the total power radiated onto a circular area:
P(x) = P0 ( 1 - J0(x)^2 - J1(x)^2 ),
where P0 is the total power.
Note that you also can get a closed form solution for your integration using Sympy:
import sympy as sy
sy.init_printing() # LaTeX like pretty printing in IPython
x,d = sy.symbols("x,d", real=True)
I0=100
dist=3.8317
f = I0*((2*sy.besselj(1,x)/x)**2) # the integrand
F = f.integrate((x, -d, d)) # symbolic integration
print(F.evalf(subs={d:dist})) # numeric evalution
F evaluates to:
1600*d*besselj(0, Abs(d))**2/3 + 1600*d*besselj(1, Abs(d))**2/3 - 800*besselj(1, Abs(d))**2/(3*d)
with besselj(0,r) corresponding to sp.j0(r).
They might be a singularity in the integration algorithm when doing the jacobian at x = 0. You can exclude this points from the integration with "points":
f = lambda x:( I0*((2*sp.j1(x)/x)**2))
I = quad(f, -dist, dist, points = [0])
I get then the following result (is this your desired result?)
331.4990321315221
I spent some time these days on a problem. I have a set of data:
y = f(t), where y is very small concentration (10^-7), and t is in second. t varies from 0 to around 12000.
The measurements follow an established model:
y = Vs * t - ((Vs - Vi) * (1 - np.exp(-k * t)) / k)
And I need to find Vs, Vi, and k. So I used curve_fit, which returns the best fitting parameters, and I plotted the curve.
And then I used a similar model:
y = (Vs * t/3600 - ((Vs - Vi) * (1 - np.exp(-k * t/3600)) / k)) * 10**7
By doing that, t is a number of hour, and y is a number between 0 and about 10. The parameters returned are of course different. But when I plot each curve, here is what I get:
http://i.imgur.com/XLa4LtL.png
The green fit is the first model, the blue one with the "normalized" model. And the red dots are the experimental values.
The fitting curves are different. I think it's not expected, and I don't understand why. Are the calculations more accurate if the numbers are "reasonnable" ?
The docstring for optimize.curve_fit says,
p0 : None, scalar, or M-length sequence
Initial guess for the parameters. If None, then the initial
values will all be 1 (if the number of parameters for the function
can be determined using introspection, otherwise a ValueError
is raised).
Thus, to begin with, the initial guess for the parameters is by default 1.
Moreover, curve fitting algorithms have to sample the function for various values of the parameters. The "various values" are initially chosen with an initial step size on the order of 1. The algorithm will work better if your data varies somewhat smoothly with changes in the parameter values that on the order of 1.
If the function varies wildly with parameter changes on the order of 1, then the algorithm may tend to miss the optimum parameter values.
Note that even if the algorithm uses an adaptive step size when it tweaks the parameter values, if the initial tweak is so far off the mark as to produce a big residual, and if tweaking in some other direction happens to produce a smaller residual, then the algorithm may wander off in the wrong direction and miss the local minimum. It may find some other (undesired) local minimum, or simply fail to converge. So using an algorithm with an adaptive step size won't necessarily save you.
The moral of the story is that scaling your data can improve the algorithm's chances of of finding the desired minimum.
Numerical algorithms in general all tend to work better when applied to data whose magnitude is on the order of 1. This bias enters into the algorithm in numerous ways. For instance, optimize.curve_fit relies on optimize.leastsq, and the call signature for optimize.leastsq is:
def leastsq(func, x0, args=(), Dfun=None, full_output=0,
col_deriv=0, ftol=1.49012e-8, xtol=1.49012e-8,
gtol=0.0, maxfev=0, epsfcn=None, factor=100, diag=None):
Thus, by default, the tolerances ftol and xtol are on the order of 1e-8. If finding the optimum parameter values require much smaller tolerances, then these hard-coded default numbers will cause optimize.curve_fit to miss the optimize parameter values.
To make this more concrete, suppose you were trying to minimize f(x) = 1e-100*x**2. The factor of 1e-100 squashes the y-values so much that a wide range of x-values (the parameter values mentioned above) will fit within the tolerance of 1e-8. So, with un-ideal scaling, leastsq will not do a good job of finding the minimum.
Another reason to use floats on the order of 1 is because there are many more (IEEE754) floats in the interval [-1,1] than there are far away from 1. For example,
import struct
def floats_between(x, y):
"""
http://stackoverflow.com/a/3587987/190597 (jsbueno)
"""
a = struct.pack("<dd", x, y)
b = struct.unpack("<qq", a)
return b[1] - b[0]
In [26]: floats_between(0,1) / float(floats_between(1e6,1e7))
Out[26]: 311.4397707054894
This shows there are over 300 times as many floats representing numbers between 0 and 1 than there are in the interval [1e6, 1e7].
Thus, all else being equal, you'll typically get a more accurate answer if working with small numbers than very large numbers.
I would imagine it has more to do with the initial parameter estimates you are passing to curve fit. If you are not passing any I believe they all default to 1. Normalizing your data makes those initial estimates closer to the truth. If you don't want to use normalized data just pass the initial estimates yourself and give them reasonable values.
Others have already mentioned that you probably need to have a good starting guess for your fit. In cases like this is, I usually try to find some quick and dirty tricks to get at least a ballpark estimate of the parameters. In your case, for large t, the exponential decays pretty quickly to zero, so for large t, you have
y == Vs * t - (Vs - Vi) / k
Doing a first-order linear fit like
[slope1, offset1] = polyfit(t[t > 2000], y[t > 2000], 1)
you will get slope1 == Vs and offset1 == (Vi - Vs) / k.
Subtracting this straight line from all the points you have, you get the exponential
residual == y - slope1 * t - offset1 == (Vs - Vi) * exp(-t * k)
Taking the log of both sides, you get
log(residual) == log(Vs - Vi) - t * k
So doing a second fit
[slope2, offset2] = polyfit(t, log(y - slope1 * t - offset1), 1)
will give you slope2 == -k and offset2 == log(Vs - Vi), which should be solvable for Vi since you already know Vs. You might have to limit the second fit to small values of t, otherwise you might be taking the log of negative numbers. Collect all the parameters you obtained with these fits and use them as the starting points for your curve_fit.
Finally, you might want to look into doing some sort of weighted fit. The information about the exponential part of your curve is contained in just the first few points, so maybe you should give those a higher weight. Doing this in a statistically correct way is not trivial.
I'm trying to interpolate some data for the purpose of plotting. For instance, given N data points, I'd like to be able to generate a "smooth" plot, made up of 10*N or so interpolated data points.
My approach is to generate an N-by-10*N matrix and compute the inner product the original vector and the matrix I generated, yielding a 1-by-10*N vector. I've already worked out the math I'd like to use for the interpolation, but my code is pretty slow. I'm pretty new to Python, so I'm hopeful that some of the experts here can give me some ideas of ways I can try to speed up my code.
I think part of the problem is that generating the matrix requires 10*N^2 calls to the following function:
def sinc(x):
import math
try:
return math.sin(math.pi * x) / (math.pi * x)
except ZeroDivisionError:
return 1.0
(This comes from sampling theory. Essentially, I'm attempting to recreate a signal from its samples, and upsample it to a higher frequency.)
The matrix is generated by the following:
def resampleMatrix(Tso, Tsf, o, f):
from numpy import array as npar
retval = []
for i in range(f):
retval.append([sinc((Tsf*i - Tso*j)/Tso) for j in range(o)])
return npar(retval)
I'm considering breaking up the task into smaller pieces because I don't like the idea of an N^2 matrix sitting in memory. I could probably make 'resampleMatrix' into a generator function and do the inner product row-by-row, but I don't think that will speed up my code much until I start paging stuff in and out of memory.
Thanks in advance for your suggestions!
This is upsampling. See Help with resampling/upsampling for some example solutions.
A fast way to do this (for offline data, like your plotting application) is to use FFTs. This is what SciPy's native resample() function does. It assumes a periodic signal, though, so it's not exactly the same. See this reference:
Here’s the second issue regarding time-domain real signal interpolation, and it’s a big deal indeed. This exact interpolation algorithm provides correct results only if the original x(n) sequence is periodic within its full time interval.
Your function assumes the signal's samples are all 0 outside of the defined range, so the two methods will diverge away from the center point. If you pad the signal with lots of zeros first, it will produce a very close result. There are several more zeros past the edge of the plot not shown here:
Cubic interpolation won't be correct for resampling purposes. This example is an extreme case (near the sampling frequency), but as you can see, cubic interpolation isn't even close. For lower frequencies it should be pretty accurate.
If you want to interpolate data in a quite general and fast way, splines or polynomials are very useful. Scipy has the scipy.interpolate module, which is very useful. You can find many examples in the official pages.
Your question isn't entirely clear; you're trying to optimize the code you posted, right?
Re-writing sinc like this should speed it up considerably. This implementation avoids checking that the math module is imported on every call, doesn't do attribute access three times, and replaces exception handling with a conditional expression:
from math import sin, pi
def sinc(x):
return (sin(pi * x) / (pi * x)) if x != 0 else 1.0
You could also try avoiding creating the matrix twice (and holding it twice in parallel in memory) by creating a numpy.array directly (not from a list of lists):
def resampleMatrix(Tso, Tsf, o, f):
retval = numpy.zeros((f, o))
for i in xrange(f):
for j in xrange(o):
retval[i][j] = sinc((Tsf*i - Tso*j)/Tso)
return retval
(replace xrange with range on Python 3.0 and above)
Finally, you can create rows with numpy.arange as well as calling numpy.sinc on each row or even on the entire matrix:
def resampleMatrix(Tso, Tsf, o, f):
retval = numpy.zeros((f, o))
for i in xrange(f):
retval[i] = numpy.arange(Tsf*i / Tso, Tsf*i / Tso - o, -1.0)
return numpy.sinc(retval)
This should be significantly faster than your original implementation. Try different combinations of these ideas and test their performance, see which works out the best!
I'm not quite sure what you're trying to do, but there are some speedups you can do to create the matrix. Braincore's suggestion to use numpy.sinc is a first step, but the second is to realize that numpy functions want to work on numpy arrays, where they can do loops at C speen, and can do it faster than on individual elements.
def resampleMatrix(Tso, Tsf, o, f):
retval = numpy.sinc((Tsi*numpy.arange(i)[:,numpy.newaxis]
-Tso*numpy.arange(j)[numpy.newaxis,:])/Tso)
return retval
The trick is that by indexing the aranges with the numpy.newaxis, numpy converts the array with shape i to one with shape i x 1, and the array with shape j, to shape 1 x j. At the subtraction step, numpy will "broadcast" the each input to act as a i x j shaped array and the do the subtraction. ("Broadcast" is numpy's term, reflecting the fact no additional copy is made to stretch the i x 1 to i x j.)
Now the numpy.sinc can iterate over all the elements in compiled code, much quicker than any for-loop you could write.
(There's an additional speed-up available if you do the division before the subtraction, especially since inthe latter the division cancels the multiplication.)
The only drawback is that you now pay for an extra Nx10*N array to hold the difference. This might be a dealbreaker if N is large and memory is an issue.
Otherwise, you should be able to write this using numpy.convolve. From what little I just learned about sinc-interpolation, I'd say you want something like numpy.convolve(orig,numpy.sinc(numpy.arange(j)),mode="same"). But I'm probably wrong about the specifics.
If your only interest is to 'generate a "smooth" plot' I would just go with a simple polynomial spline curve fit:
For any two adjacent data points the coefficients of a third degree polynomial function can be computed from the coordinates of those data points and the two additional points to their left and right (disregarding boundary points.) This will generate points on a nice smooth curve with a continuous first dirivitive. There's a straight forward formula for converting 4 coordinates to 4 polynomial coefficients but I don't want to deprive you of the fun of looking it up ;o).
Here's a minimal example of 1d interpolation with scipy -- not as much fun as reinventing, but.
The plot looks like sinc, which is no coincidence:
try google spline resample "approximate sinc".
(Presumably less local / more taps ⇒ better approximation,
but I have no idea how local UnivariateSplines are.)
""" interpolate with scipy.interpolate.UnivariateSpline """
from __future__ import division
import numpy as np
from scipy.interpolate import UnivariateSpline
import pylab as pl
N = 10
H = 8
x = np.arange(N+1)
xup = np.arange( 0, N, 1/H )
y = np.zeros(N+1); y[N//2] = 100
interpolator = UnivariateSpline( x, y, k=3, s=0 ) # s=0 interpolates
yup = interpolator( xup )
np.set_printoptions( 1, threshold=100, suppress=True ) # .1f
print "yup:", yup
pl.plot( x, y, "green", xup, yup, "blue" )
pl.show()
Added feb 2010: see also basic-spline-interpolation-in-a-few-lines-of-numpy
Small improvement. Use the built-in numpy.sinc(x) function which runs in compiled C code.
Possible larger improvement: Can you do the interpolation on the fly (as the plotting occurs)? Or are you tied to a plotting library that only accepts a matrix?
I recommend that you check your algorithm, as it is a non-trivial problem. Specifically, I suggest you gain access to the article "Function Plotting Using Conic Splines" (IEEE Computer Graphics and Applications) by Hu and Pavlidis (1991). Their algorithm implementation allows for adaptive sampling of the function, such that the rendering time is smaller than with regularly spaced approaches.
The abstract follows:
A method is presented whereby, given a
mathematical description of a
function, a conic spline approximating
the plot of the function is produced.
Conic arcs were selected as the
primitive curves because there are
simple incremental plotting algorithms
for conics already included in some
device drivers, and there are simple
algorithms for local approximations by
conics. A split-and-merge algorithm
for choosing the knots adaptively,
according to shape analysis of the
original function based on its
first-order derivatives, is
introduced.