pyshtools defines three major classes that simplify access to the underlying SHTOOLS functions:
The underlying data are stored in internal subclasses in different formats (such as kind = 'real'
or 'complex'
and grid = 'DH'
or 'GLQ'
). In this tutorial, we will demonstrate several aspects related to the SHCoeffs
and SHGrid
classes.
In [1]:
from __future__ import print_function # only necessary if using Python 2.x
%matplotlib inline
import matplotlib.pyplot as plt
import numpy as np
import pyshtools
In [2]:
pyshtools.utils.figstyle(rel_width=0.75)
%config InlineBackend.figure_format = 'retina' # if you are not using a retina display, comment this line
The spherical harmonic coefficient class SHCoeffs
can be initialized directly from a numpy array that holds the spherical harmonic coefficient data. Spherical harmonic coefficients are stored as a numpy array of dimension (2, lmax+1, lmax+1), where the first column corresponds to the cosine [0] and sine [1] components, the second column
corresponds to the spherical harmonic degree l
, and the third column corresponds to the angular order m
. We will first create a numpy array of coefficients that are equal to zero, with the exception of the l=5
, m=2
harmonic.
In [3]:
lmax = 200
coeffs = np.zeros((2, lmax+1, lmax+1))
coeffs[0, 5, 2] = 1.
To initialize a new class instance, we make use of the constructor method from_array()
:
In [4]:
coeffs_l5m2 = pyshtools.SHCoeffs.from_array(coeffs)
When initializing a new class instance, the default is to assume that the input coefficients are 4$\pi$ normalized excluding the Condon-Shortley phase. This normalization convention can be overridden by setting the optional parameter normalization
, which takes values of '4pi'
, 'ortho'
, 'schmidt'
, or 'unnorm'
, along with the parameter csphase
, which can be 1 (to exclude the Condon-Shortley phase) or -1 (to include it). The SHCoeffs
class contains many methods, and here we use plot_spectrum()
to plot the power spectrum:
In [5]:
fig, ax = coeffs_l5m2.plot_spectrum(xscale='log', yscale='lin', show=False) # show=False is used to avoid a warning when plotting in inline mode
To plot the function that corresponds to the coefficients, we first need to expand it on a grid, which can be accomplished using the expand()
method:
In [6]:
grid_l5m2 = coeffs_l5m2.expand(grid='DH2')
This returns a new SHGrid
class instance. The resolution of the grid is determined automatically to correspond to the maximum degree of the spherical harmonic coefficients in order to ensure good sampling. The optional parameter grid
can be 'DH2'
for a Driscoll and Healy sampled grid with nlon = 2 * nlat, 'DH'
for a Driscol and Healy sampled grid with nlon = nlat, or 'GLQ'
for a grid used with the Gauss-Legendre quadrature expansion routines. Once the grid is created, it can be plotted using the built-in method plot()
.
In [7]:
fig, ax = grid_l5m2.plot(show=False)
Another constructor for the SHCoeffs
class is the from_random()
method. It takes a power spectrum (power per degree l of the coefficients) and generates coefficients that are independent normal distributed random variables with the provided expected power spectrum. This corresponds to a stationary and isotropic random model on the surface of the sphere whose autocorrelation function is given by the spherical harmonic addition theorem.
We initialize coefficients here with a scale-free power spectrum that has equal band power beyond the scale length that defines the size of the largest model features. The particular property of this model is that it is invariant under zoom operations.
In [8]:
a = 20 # scale length
degrees = np.arange(lmax+1, dtype=np.float)
power = 1. / (1. + (degrees / a) ** 2) ** 0.5
coeffs_global = pyshtools.SHCoeffs.from_random(power)
fig, ax = coeffs_global.plot_spectrum(unit='per_dlogl', xscale='log', show=False)
fig2, ax2 = coeffs_global.expand(grid='DH2').plot(show=False)
Spherical harmonic coefficients can be expressed in a different coordinate system very efficiently. Importantly, the power per degree spectrum is invariant under rotation.
The rotations are specified by the three Euler angles alpha
, beta
, and gamma
. There are two different conventions for specifying these angles, and the rotations can furthermore be viewed as either a rotation of the coordinate system or a rotation of the physical body. pyshtools by default uses the "y-convention" and rotates the coordinate system with the following three successive operations
alpha
,beta
, andgamma
.To rotate the physical body instead of the coordinate system, it is only necessary to set the optional parameter body
equal to True. To use the x convention, where the second rotation is with respect to the x axis, set the optional parameter convention
equal to 'x'
.
In the following example, we use the constructor from_zeros()
, and then use the method set_coeffs()
to initialize a single zonal spherical harmonic coefficient. We then rotate the physical body whose symmetry axis passess through the north pole to 30 degrees east longitude on the equator.
In [9]:
coeffs_l5m0 = pyshtools.SHCoeffs.from_zeros(lmax)
coeffs_l5m0.set_coeffs(1., 5, 0)
alpha = 30. # rotation around the initial z-axis
beta = 90. # rotation around the new y-axis
gamma = 0. # rotation around the new z-axis
coeffs_l5m0_rot = coeffs_l5m0.rotate(alpha, beta, gamma, body=True, degrees=True)
grid_l5m0_rot = coeffs_l5m0_rot.expand(grid='DH2')
fig, ax = grid_l5m0_rot.plot(show=False)
In [10]:
grid_new = (2. * grid_l5m0_rot + grid_l5m2**2 - grid_l5m2 * grid_l5m2) / 2.0
grid_new.plot(show=False)
coeffs = grid_new.expand()
fig, ax = coeffs.plot_spectrum(xscale='log', show=False)