Visualizing Attractors#

datashaderpanelhvplotholoviewsparamnumbabokeh
Published: September 17, 2018 · Modified: November 26, 2024


An attractor is a set of values to which a numerical system tends to evolve. An attractor is called a strange attractor if the resulting pattern has a fractal structure. This notebook shows how to calculate and plot two-dimensional attractors of a variety of types, using code and parameters primarily from Lázaro Alonso, François Pacull, Jason Rampe, Paul Bourke, and James A. Bednar.

Clifford Attractors#

For example, a Clifford Attractor is a strange attractor defined by two iterative equations that determine the x,y locations of discrete steps in the path of a particle across a 2D space, given a starting point (x0,y0) and the values of four parameters (a,b,c,d):

(1)#\[\begin{equation} x_{n +1} = \sin(a y_{n}) + c \cos(a x_{n}) \end{equation}\]
(2)#\[\begin{equation} y_{n +1} = \sin(b x_{n}) + d \cos(b y_{n}) \end{equation}\]

At each time step, the equations define the location for the following time step, and the accumulated locations show the areas of the 2D plane most commonly visited by the imaginary particle.

It’s easy to calculate these values in Python using Numba. First, we define the iterative attractor equation:

import numpy as np, pandas as pd
from numba import jit
from math import sin, cos, sqrt, fabs

@jit
def Clifford(x, y, a, b, c, d, *o):
    return sin(a * y) + c * cos(a * x), \
           sin(b * x) + d * cos(b * y)

We then evaluate this equation 10 million times, creating a set of x,y coordinates visited. The @jit here and above is optional, but it makes the code 50x faster.

n=10_000_000

@jit
def trajectory_coords(fn, x0, y0, a, b=0, c=0, d=0, e=0, f=0, n=n):
    x, y = np.zeros(n), np.zeros(n)
    x[0], y[0] = x0, y0
    for i in np.arange(n-1):
        x[i+1], y[i+1] = fn(x[i], y[i], a, b, c, d, e, f)
    return x,y

def trajectory(fn, x0, y0, a, b=0, c=0, d=0, e=0, f=0, n=n):
    x, y = trajectory_coords(fn, x0, y0, a, b, c, d, e, f, n)
    return pd.DataFrame(dict(x=x,y=y))
%%time
df = trajectory(Clifford, 0, 0, -1.3, -1.3, -1.8, -1.9)
CPU times: user 1.08 s, sys: 80.4 ms, total: 1.16 s
Wall time: 1.16 s
df.tail()
x y
9999995 1.857884 1.395837
9999996 0.375264 -0.205512
9999997 -1.326024 -2.301316
9999998 0.423711 2.867012
9999999 -0.981134 1.060115

We can now aggregate these 10,000,000 continuous coordinates into a discrete 2D rectangular grid with Datashader, counting each time a point fell into that grid cell:

import datashader as ds
/home/runner/work/examples/examples/attractors/envs/default/lib/python3.11/site-packages/dask/dataframe/__init__.py:31: FutureWarning: 
Dask dataframe query planning is disabled because dask-expr is not installed.

You can install it with `pip install dask[dataframe]` or `conda install dask`.
This will raise in a future version.

  warnings.warn(msg, FutureWarning)
%%time

cvs = ds.Canvas(plot_width = 700, plot_height = 700)
agg = cvs.points(df, 'x', 'y')
print(agg.values[190:195,190:195],"\n")
[[ 37  41  26  24  24]
 [ 28  30  42  27  26]
 [111  53  29  37  28]
 [145 177 113  63  44]
 [ 78  94 136 140  96]] 

CPU times: user 391 ms, sys: 7.91 ms, total: 399 ms
Wall time: 398 ms

A small portion of that grid is shown above, but it’s difficult to see the grid’s structure from the numerical values. To see the entire array at once, we can turn each grid cell into a pixel, using a greyscale value from white to black:

ds.transfer_functions.Image.border=0

ds.tf.shade(agg, cmap = ["white", "black"])

As you can see, the most-visited areas of the plane have an interesting structure for this set of parameters. To explore further, let’s wrap up the above aggregation and shading commands into a function so we can apply them more easily:

from datashader.colors import inferno, viridis

def dsplot(fn, vals, n=n, cmap=viridis, label=True):
    """Return a Datashader image by collecting `n` trajectory points for the given attractor `fn`"""
    lab = ("{}, "*(len(vals)-1)+" {}").format(*vals) if label else None
    df  = trajectory(fn, *vals, n=n)
    cvs = ds.Canvas(plot_width = 300, plot_height = 300)
    agg = cvs.points(df, 'x', 'y')
    img = ds.tf.shade(agg, cmap=cmap, name=lab)
    return img

And let’s load some colormaps that we can use for subsequent plots:

from colorcet import palette

palette["viridis"]=viridis
palette["inferno"]=inferno

We can now use these colormaps with a pre-selected set of Clifford attractor parameter values (stored in a separate YAML-format text file) to show a wide variety of trajectories that these equations can form:

import yaml
vals = yaml.load(open("data/strange_attractors.yml","r"), Loader=yaml.FullLoader)

def args(name):
    """Return a list of available argument lists for the given type of attractor"""
    return [v[1:] for v in vals if v[0]==name]

def plot(fn, vals=None, **kw):
    """Plot the given attractor `fn` once per provided set of arguments."""
    vargs=args(fn.__name__) if vals is None else vals
    return ds.tf.Images(*[dsplot(fn, v[1:], cmap=palette[v[0]][::-1], **kw) for v in vargs]).cols(4)
plot(Clifford)
0, 0, -1.3, -1.3, -1.8, -1.9

0, 0, -1.4, 1.6, 1.0, 0.7

0, 0, 1.7, 1.7, 0.6, 1.2

0, 0, 1.7, 0.7, 1.4, 2.0

0, 0, -1.7, 1.8, -1.9, -0.4

0, 0, 1.1, -1.32, -1.03, 1.54

0, 0, 0.77, 1.99, -1.31, -1.45

0, 0, -1.9, -1.9, -1.9, -1.0

0, 0, 0.75, 1.34, -1.93, 1.0

0, 0, -1.32, -1.65, 0.74, 1.81

0, 0, -1.6, 1.6, 0.7, -1.0

0, 0, -1.7, 1.5, -0.5, 0.7

Here the values shown are the arguments for the first call to Clifford(x, y, a, b, c, d), with each subsequent call using the x,y location of the previous call.

Randomly sampling the parameter space typically yields much less dramatic patterns, such as all trajectory locations being on a small number of points:

import numpy.random
numpy.random.seed(21)
num = 4

rvals=np.c_[np.zeros((num,2)), numpy.random.random((num,4))*4-2]
plot(Clifford, vals=[["kbc"]+list(rvals[i]) for i in range(len(rvals))], label=True)
0.0, 0.0, -1.8051004767634908, -0.8435613608407326, 0.8838653873249194, -1.9135350003362008

0.0, 0.0, -1.176308938930244, -1.7969069732184928, -0.7909124241415326, 0.6556411784987999

0.0, 0.0, -0.7675424270524847, 0.33436510487439497, -1.7217161815495978, 1.4696179359723534

0.0, 0.0, -1.467037922993009, -1.2875013537620066, -0.01628180069537688, 1.4547985782328943

If you wish, Datashader could easily be used to filter out such uninteresting examples, by applying a criterion to the aggregate array before shading and showing only those that remain (e.g. rejecting those where 80% of the pixel bins are empty).

De Jong attractors#

A variety of other sets of attractor equations have been proposed, such as these from Peter de Jong:

@jit
def De_Jong(x, y, a, b, c, d, *o):
    return sin(a * y) - cos(b * x), \
           sin(c * x) - cos(d * y)

plot(De_Jong)
0, 0, -1.244, -1.251, -1.815, -1.908

0, 0, 1.7, 1.7, 0.6, 1.2

0, 0, 1.4, -2.3, 2.4, -2.1

0, 0, -2.7, -0.09, -0.86, -2.2

0, 0, -0.827, -1.637, 1.659, -0.943

0, 0, -2.24, 0.43, -0.65, -2.43

0, 0, 2.01, -2.53, 1.61, -0.33

0, 0, 1.4, 1.56, 1.4, -6.56

Svensson attractors#

From Johnny Svensson:

@jit
def Svensson(x, y, a, b, c, d, *o):
    return d * sin(a * x) - sin(b * y), \
           c * cos(a * x) + cos(b * y)

plot(Svensson)
0, 0, 1.5, -1.8, 1.6, 0.9

0, 0, -1.78, 1.29, -0.09, -1.18

0, 0, -0.91, -1.29, -1.97, -1.56

0, 0, 1.4, 1.56, 1.4, -6.56

Bedhead Attractor#

From Ivan Emrich and Jason Rampe:

@jit
def Bedhead(x, y, a, b, *o):
    return sin(x*y/b)*y + cos(a*x-y), \
           x + sin(y)/b

plot(Bedhead)
1, 1, -0.81, -0.92

1, 1, -0.64, 0.76

1, 1, 0.06, 0.98

1, 1, -0.67, 0.83

Fractal Dream Attractor#

From Clifford A. Pickover’s book “Chaos In Wonderland”, with parameters from Jason Rampe:

@jit
def Fractal_Dream(x, y, a, b, c, d, *o):
    return sin(y*b)+c*sin(x*b), \
           sin(x*a)+d*sin(y*a)

plot(Fractal_Dream)
0.1, 0.1, -0.966918, 2.879879, 0.765145, 0.744728

0.1, 0.1, -2.8276, 1.2813, 1.9655, 0.597

0.1, 0.1, -1.1554, -2.3419, -1.9799, 2.1828

0.1, 0.1, -1.9956, -1.4528, -2.6206, 0.8517

Hopalong attractors#

From Barry Martin, here with code for two variants from François Pacull:

@jit
def Hopalong1(x, y, a, b, c, *o):
    return y - sqrt(fabs(b * x - c)) * np.sign(x), \
           a - x
@jit
def Hopalong2(x, y, a, b, c, *o):
    return y - 1.0 - sqrt(fabs(b * x - 1.0 - c)) * np.sign(x - 1.0), \
           a - x - 1.0

plot(Hopalong1)
0, 0, 2.0, 1.0, 0.0

0, 0, -11.0, 0.05, 0.5

0, 0, 2.0, 0.05, 2.0

0, 0, 1.1, 0.5, 1.0

plot(Hopalong2)
0, 0, 7.17, 8.44, 2.56

0, 0, 7.8, 0.13, 8.15

0, 0, 9.7, 1.6, 7.9

Gumowski-Mira Attractor#

From I. Gumowski and C. Mira, with code and parameters from Jason Rampe and Lázaro Alonso:

@jit
def G(x, mu):
    return mu * x + 2 * (1 - mu) * x**2 / (1.0 + x**2)

@jit
def Gumowski_Mira(x, y, a, b, mu, *o):
    xn = y + a*(1 - b*y**2)*y  +  G(x, mu)
    yn = -x + G(xn, mu)
    return xn, yn

plot(Gumowski_Mira)
0.1, 0.1, 0.0, 0.5, -0.75

0, 1, 0.008, 0.05, -0.496

0.1, 0.1, 0.0, 0.5, -0.7509

0, 1, 0.0, 0.5, -0.22

0, 1, 0.008, 0.05, -0.9

0, 1, 0.008, 0.05, -0.45

0.1, 0.1, 0.008, 0.05, 0.16

0, 0.5, 0.008, 0.05, -0.7

0.5, 0, 0.0, 0.05, -0.2

0.5, 0.5, 0.0, 0.05, -0.22

0, 0.5, 0.0, 0.05, -0.31

0, 0.5, 0.0, 0.05, -0.55

0.5, 0.5, 0.0, 0.05, -0.23

0.5, 0.5, 0.009, 0.05, 0.32

0.1, 0.1, 0.0, 0.5, -0.65

0.0, 0.5, 0.0, 0, -0.578

0.0, 0.5, 0.0, 0, -0.604

0.0, 0.5, 0.0, 0, 0.228

0.0, 0.5, 0.0, 0, -0.002

0.0, 0.5, 0.0, 0, -0.623

Symmetric Icon Attractor#

The Hopalong and Gumowski-Mira equations often result in symmetric patterns, but a different approach is to force the patterns to be symmetric, which is often pleasing. Examples from “Symmetry in Chaos” by Michael Field and Martin Golubitsky, with code and parameters from Jason Rampe:

@jit
def Symmetric_Icon(x, y, a, b, g, om, l, d, *o):
    zzbar = x*x + y*y
    p = a*zzbar + l
    zreal, zimag = x, y

    for i in range(1, d-1):
        za, zb = zreal * x - zimag * y, zimag * x + zreal * y
        zreal, zimag = za, zb

    zn = x*zreal - y*zimag
    p += b*zn

    return p*x + g*zreal - om*y, p*y - g*zimag + om*x

plot(Symmetric_Icon)
0.01, 0.01, 1.8, 0.0, 1.0, 0.1, -1.93, 5

0.01, 0.01, 5.0, -1.0, 1.0, 0.188, -2.5, 5

0.01, 0.01, -1.0, 0.1, -0.82, 0.12, 1.56, 3

0.01, 0.01, 1.806, 0.0, 1.0, 0.0, -1.806, 5

0.01, 0.01, 10.0, -12.0, 1.0, 0.0, -2.195, 3

0.01, 0.01, -2.5, 0.0, 0.9, 0.0, 2.5, 3

0.01, 0.01, 3.0, -16.79, 1.0, 0.0, -2.05, 9

0.01, 0.01, 5.0, 1.5, 1.0, 0.0, -2.7, 6

0.01, 0.01, 1.0, -0.1, 0.167, 0.0, -2.08, 7

0.01, 0.01, 2.32, 0.0, 0.75, 0.0, -2.32, 5

0.01, 0.01, -2.0, 0.0, -0.5, 0.0, 2.6, 5

0.01, 0.01, 2.0, 0.2, 0.1, 0.0, -2.34, 5

0.01, 0.01, 2.0, 0.0, 1.0, 0.1, -1.86, 4

0.01, 0.01, -1.0, 0.1, -0.82, 0.0, 1.56, 3

0.01, 0.01, -1.0, 0.03, -0.8, 0.0, 1.455, 3

0.01, 0.01, -2.5, -0.1, 0.9, -0.15, 2.39, 16

Interactive plotting#

If you are running a live Python process, you can use Datashader with hvPlot to zoom in and see the individual steps in any of these calculations:

import hvplot.pandas # noqa

df = trajectory(Clifford, *(args("Clifford")[5][1:]))
df.hvplot.points('x', 'y', rasterize=True, dynspread=True, cnorm='eq_hist',
                 width=400,height=400, colorbar=False)

Each time you zoom in in a live process, the data will be reaggregated, which should take a small fraction of a second for 10 million points. Eventually, once you zoom in enough you should see individual data points, as we are not connecting the points into a trajectory here.

You can also try “connecting the dots”, which will reveal how the particle jumps discretely from one region of the space to another:

df.hvplot.paths('x', 'y', rasterize=True, dynspread=True, cnorm='eq_hist',
                  width=400, height=400, colorbar=False)

Again, if you zoom in on a live server, the plot will update so that you can see the individual traces involved.

On the live server, you can also explore to find your own parameter values that generate interesting patterns:

import holoviews as hv
from holoviews.operation.datashader import rasterize, dynspread
hv.extension('bokeh')

def hv_clif(a,b,c,d,x0=0,y0=0,n=n):
    return hv.Points(trajectory(Clifford, x0, y0, a, b, c, d, n))

x0,y0,a,b,c,d = args("Clifford")[6][1:]

dm = hv.DynamicMap(hv_clif, kdims=['a', 'b', 'c', 'd'])
dm = dm.redim.range(a=(-2.0, 2.0), b=(-2.0,2.0), c=(-2.0,2.0), d=(-2.0,2.0))
dm = dm.redim.default(a=a, b=b, c=c, d=d)

dynspread(rasterize(dm)).opts(cmap='kgy_r', cnorm='eq_hist', width=500,height=500)

Although many of the regions of this four-dimensional parameter space generate uninteresting trajectories such as single points, you can find interesting regions by starting with one of the a,b,c,d tuples of values in previous plots, then click on one slider and use the left and right arrow keys to see how the plot changes as that parameter changes. See also this Panel-based attractor dashboard.

This web page was generated from a Jupyter notebook and not all interactivity will work on this website.