ANN: pvlib-0.9.1 released

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Dear Pythonistas and solar power enthusiasts,

On behalf of the maintainers, we're happy to announce a new release of
pvlib python:
software for simulating performance of photovoltaic solar energy systems.

*See what's new for v0.9.1:*
* https://pvlib-python.readthedocs.io/en/stable/whatsnew.html

*Releases are available from PyPI and the conda-forge channel:*
* https://pypi.org/project/pvlib/
* https://anaconda.org/conda-forge/pvlib-python

*Read the Documentation:*
* https://pvlib-python.readthedocs.io/en/stable/index.html

*Report issues & contribute:*
* https://github.com/pvlib/pvlib-python

*Highlights:*
** *Beautifully updated documentation theme that is easier to browse and
navigate. Please share your feedback!
* Implementation of pvlib.temperature.prilliman
<https://pvlib-python.readthedocs.io/en/stable/reference/generated/pvlib.temperature.prilliman.html#pvlib.temperature.prilliman>,
a transient weighted moving-average temperature model by Prilliman, *et al.*,
to calculate back of module temperature from high-frequency sub-hourly
irradiance input to account for different characteristic timescales between
heat transfer and power conversion.
* New infinite sheds model for either bifacial or monofacial modules, that
calculates row-to-row shading and view factors for sky and ground reflected
diffuse irradiance. Use pvlib.bifacial.infinite_sheds.get_irradiance
<https://pvlib-python.readthedocs.io/en/stable/reference/generated/pvlib.bifacial.infinite_sheds.get_irradiance.html#pvlib.bifacial.infinite_sheds.get_irradiance>
to calculate the plane of array irradiance, all its components on both
front and back sides, and the total from both sides.

*The maintainers thank you for using pvlib python!*

-- 
Mark Mikofski, PhD (2005)
*Fiat Lux*

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<div dir=3D"ltr">Dear Pythonistas and solar power enthusiasts,<div><br></di=
v><div>On behalf of the maintainers, we&#39;re happy to announce a new rele=
ase of=C2=A0<span class=3D"gmail-il">pvlib</span>=C2=A0python: software for=
 simulating performance of photovoltaic solar energy systems.</div><div><br=
></div><div><b>See what&#39;s new for=C2=A0v0.9.1:</b></div><div>*=C2=A0<a =
href=3D"https://pvlib-python.readthedocs.io/en/stable/whatsnew.html" target=
=3D"_blank">https://<span class=3D"gmail-il">pvlib</span>-python.readthedoc=
s.io/en/stable/whatsnew.html</a><br></div><div><br></div><div><b>Releases a=
re available from PyPI and the conda-forge channel:</b></div><div>*=C2=A0<a=
 href=3D"https://pypi.org/project/pvlib/" target=3D"_blank">https://pypi.or=
g/project/<span class=3D"gmail-il">pvlib</span>/</a></div><div>*=C2=A0<a hr=
ef=3D"https://anaconda.org/conda-forge/pvlib-python" target=3D"_blank">http=
s://anaconda.org/conda-forge/<span class=3D"gmail-il">pvlib</span>-python</=
a></div><div><br></div><div><b>Read the Documentation:</b></div><div>*=C2=
=A0<a href=3D"https://pvlib-python.readthedocs.io/en/stable/index.html" tar=
get=3D"_blank">https://<span class=3D"gmail-il">pvlib</span>-python.readthe=
docs.io/en/stable/index.html</a><br></div><div><br></div><div><b>Report iss=
ues &amp; contribute:</b></div><div>*=C2=A0<a href=3D"https://github.com/pv=
lib/pvlib-python" target=3D"_blank">https://github.com/<span class=3D"gmail=
-il">pvlib</span>/<span class=3D"gmail-il">pvlib</span>-python</a><br></div=
><div><div><br></div><div><b>Highlights:</b></div><div><b>*=C2=A0</b>Beauti=
fully updated documentation theme that is easier to browse and navigate. Pl=
ease share your feedback!</div><div>* Implementation of <a href=3D"https://=
pvlib-python.readthedocs.io/en/stable/reference/generated/pvlib.temperature=
.prilliman.html#pvlib.temperature.prilliman">pvlib.temperature.prilliman</a=
>, a transient weighted moving-average temperature model by Prilliman, <i>e=
t al.</i>, to calculate back of module temperature from high-frequency sub-=
hourly irradiance input to account for different characteristic timescales =
between heat transfer and power conversion.</div><div>*=C2=A0New infinite s=
heds model for either bifacial or monofacial modules, that calculates row-t=
o-row shading and view factors for sky and ground reflected diffuse irradia=
nce. Use <a href=3D"https://pvlib-python.readthedocs.io/en/stable/reference=
/generated/pvlib.bifacial.infinite_sheds.get_irradiance.html#pvlib.bifacial=
.infinite_sheds.get_irradiance">pvlib.bifacial.infinite_sheds.get_irradianc=
e</a> to calculate=C2=A0the plane of array irradiance, all its components o=
n both front and back sides, and the total from both sides.</div><div><br><=
/div><div><b>The maintainers thank=C2=A0you for using=C2=A0<span class=3D"g=
mail-il">pvlib</span>=C2=A0python!</b></div></div><div><br></div>-- <br><di=
v dir=3D"ltr" class=3D"gmail_signature" data-smartmail=3D"gmail_signature">=
<div dir=3D"ltr"><div><div><span style=3D"font-size:12.8px">Mark Mikofski, =
PhD (2005)</span><br></div><div><span style=3D"font-size:12.8px"><i>Fiat Lu=
x</i></span><br></div></div></div></div></div>

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