Merge remote-tracking branch 'upstream/main' into remove-basic-pvgis-outputformat

Author: AdamRJensen

docs/sphinx/source/conf.py

@@ -66,7 +66,7 @@
 intersphinx_mapping = {
     'python': ('https://docs.python.org/3/', None),
     'numpy': ('https://numpy.org/doc/stable/', None),
-    'scipy': ('https://docs.scipy.org/doc/scipy/reference/', None),
+    'scipy': ('https://docs.scipy.org/doc/scipy/', None),
     'pandas': ('https://pandas.pydata.org/pandas-docs/stable', None),
     'matplotlib': ('https://matplotlib.org/stable', None),
 }

docs/sphinx/source/reference/iotools.rst

@@ -26,6 +26,11 @@ of sources and file formats relevant to solar energy modeling.
    iotools.read_crn
    iotools.read_solrad
    iotools.get_solrad
+   iotools.get_nsrdb_psm4_aggregated
+   iotools.get_nsrdb_psm4_tmy
+   iotools.get_nsrdb_psm4_conus
+   iotools.get_nsrdb_psm4_full_disc
+   iotools.read_nsrdb_psm4
    iotools.get_psm3
    iotools.read_psm3
    iotools.parse_psm3

docs/sphinx/source/reference/pv_modeling/parameters.rst

@@ -12,6 +12,7 @@ Functions for fitting single diode models
     ivtools.sdm.fit_cec_sam
     ivtools.sdm.fit_desoto
     ivtools.sdm.fit_pvsyst_sandia
+    ivtools.sdm.fit_pvsyst_iec61853_sandia_2025
     ivtools.sdm.fit_desoto_sandia
 
 Functions for fitting the single diode equation

docs/sphinx/source/user_guide/faq.rst renamed to docs/sphinx/source/user_guide/extras/faq.rst

@@ -133,7 +133,7 @@ Follow these steps to obtain the library using git/GitHub:
    This button is circled in the image below. Remember the system path that
    you clone the library to.
 
-.. image:: ../_images/clonebutton.png
+.. image:: ../../_images/clonebutton.png
 
 Please see GitHub's
 `Forking Projects <https://guides.github.com/activities/forking/>`_,

docs/sphinx/source/user_guide/nomenclature.rst renamed to docs/sphinx/source/user_guide/extras/nomenclature.rst

@@ -9,26 +9,26 @@ This user guide is an overview and explains some of the key features of pvlib.
 .. toctree::
    :caption: Getting started
    :maxdepth: 2
-   
-   package_overview
-   installation
-   introtutorial
-   
+
+   getting_started/package_overview
+   getting_started/installation
+   getting_started/introtutorial
+
 .. toctree::
-   :caption: Modeling topics
    :maxdepth: 2
-   
-   pvsystem
-   modelchain
-   timetimezones
-   bifacial
-   clearsky
-   weather_data
-   singlediode
+   :caption: Modeling topics
+
+   modeling_topics/pvsystem
+   modeling_topics/modelchain
+   modeling_topics/timetimezones
+   modeling_topics/bifacial
+   modeling_topics/clearsky
+   modeling_topics/weather_data
+   modeling_topics/singlediode
 
 .. toctree::
-   :caption: Extras
    :maxdepth: 2
+   :caption: Extras
 
-   nomenclature
-   faq
+   extras/nomenclature
+   extras/faq

docs/sphinx/source/user_guide/installation.rst renamed to docs/sphinx/source/user_guide/getting_started/installation.rst

@@ -80,7 +80,7 @@ The model operates in the following steps:
    determines the fraction of ground-reflected irradiance that reaches the row
    surface.
 4. Find the fraction of the row surface that is shaded from direct irradiance.
-   Only sky and ground-reflected irradiance reach the the shaded fraction of
+   Only sky and ground-reflected irradiance reach the shaded fraction of
    the row surface.
 5. For the front and rear surfaces, apply the incidence angle modifier to
    the direct irradiance and sum the diffuse sky, diffuse ground, and direct