# The plasma dispersion function¶

Let’s import some basics (and PlasmaPy!)

import numpy as np
import matplotlib.pyplot as plt
import plasmapy

help(plasmapy.mathematics.plasma_dispersion_func)


Out:

Help on function plasma_dispersion_func in module plasmapy.mathematics.mathematics:

plasma_dispersion_func(zeta: Union[complex, int, float, numpy.ndarray, astropy.units.quantity.Quantity]) -> Union[complex, float, numpy.ndarray, astropy.units.quantity.Quantity]
Calculate the plasma dispersion function.

Parameters
----------
zeta : complex, int, float, ~numpy.ndarray, or ~astropy.units.Quantity
Argument of plasma dispersion function.

Returns
-------
Z : complex, float, or ~numpy.ndarray
Value of plasma dispersion function.

Raises
------
TypeError
If the argument is of an invalid type.

~astropy.units.UnitsError
If the argument is a ~astropy.units.Quantity but is not
dimensionless.

ValueError
If the argument is not entirely finite.

--------
plasma_dispersion_func_deriv

Notes
-----
The plasma dispersion function is defined as:

.. math::
Z(\zeta) = \pi^{-0.5} \int_{-\infty}^{+\infty}
\frac{e^{-x^2}}{x-\zeta} dx

where the argument is a complex number [fried.conte-1961]_.

In plasma wave theory, the plasma dispersion function appears
frequently when the background medium has a Maxwellian
distribution function.  The argument of this function then refers
to the ratio of a wave's phase velocity to a thermal velocity.

References
----------
.. [fried.conte-1961] Fried, Burton D. and Samuel D. Conte. 1961.
The Plasma Dispersion Function: The Hilbert Transformation of the
Gaussian. Academic Press (New York and London).

Examples
--------
>>> plasma_dispersion_func(0)
1.7724538509055159j
>>> plasma_dispersion_func(1j)
0.757872156141312j
>>> plasma_dispersion_func(-1.52+0.47j)
(0.6088888957234254+0.33494583882874024j)


We’ll now make some sample data to visualize the dispersion function:

x = np.linspace(-1, 1, 1000)
X, Y = np.meshgrid(x, x)
Z = X + 1j * Y
print(Z.shape)


Out:

(1000, 1000)


Before we start plotting, let’s make a visualization function first:

def plot_complex(X, Y, Z, N=50):
fig, (real_axis, imag_axis) = plt.subplots(1, 2)
real_axis.contourf(X, Y, Z.real, N)
imag_axis.contourf(X, Y, Z.imag, N)
real_axis.set_title("Real values")
imag_axis.set_title("Imaginary values")
for ax in [real_axis, imag_axis]:
ax.set_xlabel("Real values")
ax.set_ylabel("Imaginary values")
fig.tight_layout()

plot_complex(X, Y, Z) We can now apply our visualization function to our simple dispersion relation

# sphinx_gallery_thumbnail_number = 2
F = plasmapy.mathematics.plasma_dispersion_func(Z)
plot_complex(X, Y, F) So this is going to be a hack and I’m not 100% sure the dispersion function is quite what I think it is, but let’s find the area where the dispersion function has a lesser than zero real part because I think it may be important (brb reading Fried and Conte):

plot_complex(X, Y, F.real < 0) We can also visualize the derivative:

F = plasmapy.mathematics.plasma_dispersion_func_deriv(Z)
plot_complex(X, Y, F) Plotting the same function on a larger area:

x = np.linspace(-2, 2, 2000)
X, Y = np.meshgrid(x, x)
Z = X + 1j * Y
print(Z.shape)


Out:

(2000, 2000)

F = plasmapy.mathematics.plasma_dispersion_func(Z)
plot_complex(X, Y, F, 100) Now we examine the derivative of the dispersion function as a function of the phase velocity of an electromagnetic wave propagating through the plasma. This is recreating figure 5.1 in: J. Sheffield, D. Froula, S. H. Glenzer, and N. C. Luhmann Jr, Plasma scattering of electromagnetic radiation: theory and measurement techniques. Chapter 5 Pg 106 (Academic press, 2010).

xs = np.linspace(0, 4, 100)
ws = (-1 / 2) * plasmapy.mathematics.plasma_dispersion_func_deriv(xs)
wRe = np.real(ws)
wIm = np.imag(ws)

plt.plot(xs, wRe, label="Re")
plt.plot(xs, wIm, label="Im")
plt.axis([0, 4, -0.3, 1])
plt.legend(loc='upper right',
frameon=False,
labelspacing=0.001,
fontsize=14, 