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lines changed Original file line number Diff line number Diff line change 1111# This example demonstrates how to use the
1212# :py:func:`~pvlib.spectrum.average_photon_energy` function to calculate the
1313# Average Photon Energy (APE, :math:`\overline{E_\gamma}`) of spectral
14- # irradiance distributions. This example uses spectral irradiance simulated
14+ # irradiance distributions. This example uses spectral irradiance simulated
1515# using :py:func:`~pvlib.spectrum.spectrl2`, but the same method is
1616# applicable to spectral irradiance from any source.
1717# More information on the SPECTRL2 model can be found in [1]_.
2323# To demonstrate this functionality, first we will simulate some spectra
2424# using :py:func:`~pvlib.spectrum.spectrl2`. In this example, we will simulate
2525# spectra following a similar method to that which is followed in the
26- # `Modelling Spectral Irradiance
27- # <https://pvlib-python.readthedocs.io/en/stable/gallery/spectrum/plot_spectrl2_fig51A.html>`_
28- # example, which reproduces a figure from [4]_. The first step is to
29- # import the required packages and define some basic system parameters
30- # and meteorological conditions.
26+ # :ref:`sphx_glr_gallery_spectrum_plot_spectrl2_fig51A.py` example, which
27+ # reproduces a figure from [4]_. The first step is to import the required
28+ # packages and define some basic system parameters and meteorological
29+ # conditions.
3130
3231# %%
3332import pandas as pd
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