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Co-authored-by: Adam R. Jensen <39184289+AdamRJensen@users.noreply.github.com>
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docs/examples/irradiance-decomposition/plot_diffuse_fraction.py

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# correlations, which include additional variables such as airmass. These
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# methods seem to reduce DNI spikes over 1000 [W/m^2].
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#
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# .. _TMY3: https://docs.nlr.gov/docs/fy08osti/43156.pdf
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# .. _NSRDB: https://docs.nlr.gov/docs/fy12osti/54824.pdf
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# .. _TMY3: https://doi.org/10.2172/928611
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# .. _NSRDB: https://doi.org/10.2172/1054832

docs/examples/spectrum/average_photon_energy.py

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from scipy.integrate import trapezoid
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from pvlib import spectrum, solarposition, irradiance, atmosphere
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lat, lon = 39.742, -105.18 # NLR SRRL location
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lat, lon = 39.742, -105.18 # SRRL location
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surface_tilt = 25
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surface_azimuth = 180 # south-facing system
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pressure = 81190 # at 1828 metres AMSL, roughly

docs/tutorials/tmy_to_power.ipynb

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{
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"cell_type": "markdown",
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"metadata": {},
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"source": "Next, we will assume that the SAPM model is representative of the real world performance so that we can use scipy's optimization routine to derive simulated PVUSA coefficients. You will need to install scipy to run these functions.\n\nHere's one PVUSA reference:\n\nhttps://docs.nlr.gov/docs/fy09osti/45376.pdf\n"
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"source": "Next, we will assume that the SAPM model is representative of the real world performance so that we can use scipy's optimization routine to derive simulated PVUSA coefficients. You will need to install scipy to run these functions.\n\nHere's one PVUSA reference:\n\nhttps://www.osti.gov/biblio/951223\n"
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},
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{
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"cell_type": "code",

pvlib/bifacial/infinite_sheds.py

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@@ -166,7 +166,7 @@ def _shaded_fraction(solar_zenith, solar_azimuth, surface_tilt,
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:doi:`10.1109/PVSC40753.2019.8980572`.
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.. [2] Kevin Anderson and Mark Mikofski, "Slope-Aware Backtracking for
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Single-Axis Trackers", Technical Report NREL/TP-5K00-76626, July 2020.
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https://www.nlr.gov/docs/fy20osti/76626.pdf
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:doi:`10.2172/1660126`
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"""
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tan_phi = utils._solar_projection_tangent(
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solar_zenith, solar_azimuth, surface_azimuth)

pvlib/clearsky.py

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.. [3] `Bird Clear Sky Model <http://www.nlr.gov/grid/solar-resource/
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clearsky.html>`_
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.. [4] `SERI/TR-642-761 <https://www.nlr.gov/docs/legosti/old/761.pdf>`_
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.. [4] SERI/TR-642-761 :doi:`10.2172/6510849`
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.. [5] `Error Reports <http://www.nlr.gov/grid/solar-resource/
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clearsky-error-reports.html>`_

pvlib/inverter.py

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@@ -388,7 +388,7 @@ def pvwatts(pdc, pdc0, eta_inv_nom=0.96, eta_inv_ref=0.9637):
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References
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----------
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.. [1] A. P. Dobos, "PVWatts Version 5 Manual", NLR, Golden, CO, USA,
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.. [1] A. P. Dobos, "PVWatts Version 5 Manual", NREL, Golden, CO, USA,
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Technical Report NREL/TP-6A20-62641, 2014, :doi:`10.2172/1158421`.
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"""
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pvlib/irradiance.py

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Engineers, 2005. :doi:`10.1061/9780784408056`
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.. [6] I. Reda, A. Andreas, "Solar position algorithm for solar
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radiation applications" NLR Golden, CO, USA. NREL/TP-560-34302,
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radiation applications" NREL Golden, CO, USA. NREL/TP-560-34302,
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Revised 2008. :doi:`10.2172/15003974`
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"""
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pvlib/pvsystem.py

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@@ -2963,7 +2963,7 @@ def pvwatts_dc(effective_irradiance, temp_cell, pdc0, gamma_pdc, temp_ref=25.,
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Module Performance," In Proc. 33rd IEEE Photovoltaic Specialists
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Conference (PVSC), San Diego, CA, USA, 2008, pp. 1-6,
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:doi:`10.1109/PVSC.2008.4922586`.
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https://docs.nlr.gov/docs/fy08osti/42511.pdf
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Pre-print: :doi:`10.1109/PVSC.2008.4922586`
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""" # noqa: E501
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pdc = (effective_irradiance * 0.001 * pdc0 *

pvlib/shading.py

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@@ -88,7 +88,7 @@ def masking_angle(surface_tilt, gcr, slant_height):
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:doi:`10.1016/0379-6787(84)90017-6`
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.. [2] Gilman, P. et al., (2018). "SAM Photovoltaic Model Technical
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Reference Update", NREL Technical Report NREL/TP-6A20-67399.
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Available at https://www.nlr.gov/docs/fy18osti/67399.pdf
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:doi:`10.2172/1429291`
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"""
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# The original equation (8 in [1]) requires pitch and collector width,
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# but it's easy to non-dimensionalize it to make it a function of GCR
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:doi:`10.1016/0379-6787(84)90017-6`
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.. [2] Gilman, P. et al., (2018). "SAM Photovoltaic Model Technical
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Reference Update", NREL Technical Report NREL/TP-6A20-67399.
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Available at https://www.nlr.gov/docs/fy18osti/67399.pdf
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:doi:`10.2172/1429291`
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"""
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return 1 - cosd(masking_angle/2)**2
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@@ -304,7 +304,7 @@ def projected_solar_zenith_angle(solar_zenith, solar_azimuth,
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References
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----------
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.. [1] K. Anderson and M. Mikofski, 'Slope-Aware Backtracking for
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Single-Axis Trackers', National Laboratory of the Rockies (NLR), Golden,
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Single-Axis Trackers', National Renewable Energy Lab. (NREL), Golden,
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CO (United States);
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NREL/TP-5K00-76626, Jul. 2020. :doi:`10.2172/1660126`.
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pvlib/snow.py

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Uses of the Townsend Snow Model. In "Photovoltaic Reliability
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Workshop (PVRW) 2023 Proceedings: Posters.", ed. Silverman,
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T. J. Dec. 2023. NREL/CP-5900-87918.
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Available at: https://www.nlr.gov/docs/fy25osti/90585.pdf
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:doi:`10.2172/1429291`
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.. [3] Townsend, T. (2013). Predicting PV Energy Loss Caused by Snow.
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Solar Power International, Chicago IL.
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:doi:`10.13140/RG.2.2.14299.68647`

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