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Sandia View Factor Model Implementation

Page • Sandia has coded a view factor model that estimates back-side irradiance across a row of bifacial modules, accounting for the row’s shadow on the ground and assuming an isotropic model for sky diffuse irradiance. Figure 1 and Figure 2 show the modeled variation in back-side irradiance by cell at noon...

Sandia’s Ephemeris Model

Page • Sandia National Laboratories has developed a function that approximates the position of the sun quite accurately.  This function, along with Matlab source code, is available as part of the PV_LIB Toolbox.  The function is pvl_ephemeris.  The calculation is based on an internal course, Engineering Astronomy, developed by Grover Hughes, and...

Shading, Soiling, and Reflection Losses

Page • Here, irradiance incident on the array (calculated in the previous step) is further reduced by shading, soiling, and reflection losses.  Various modeling approaches have been developed to account for these reductions.  They will be examined in detail in the following sections.

Simple Sandia Sky Diffuse Model

Page • This empirical model for diffuse sky irradiance was developed at Sandia National Laboratories by David King and has been found to work quite well at the Sandia facility (better, in fact, than any of the other models that have been compared). The model determines the diffuse irradiance from the sky ($$E_{d}$$) tilted...

Single Axis Tracking

Page • Single axis tracking simply means there is one axis of rotation. The axis can be horizontal (most common), tilted, or even vertical. A horizontal single axis tracker is the most common configuration.  The axis of rotation is horizontal, usually orientated North-South with the modules facing toward the East in the...

Single Diode Equivalent Circuit Models

Page • Equivalent circuit models define the entire I-V curve of a cell, module, or array as a continuous function for a given set of operating conditions. One basic equivalent circuit model in common use is the single diode model, which is derived from physical principles (e.g., Gray, 2011) and represented by the...

Solar Position Algorithm (SPA)

Page • Reda and Andreas 2008 from the National Renewable Energy Laboratory published a sun position algorithm with a reported uncertainty of +/- 0.0003 degrees.  The report is available from NREL at this link.  NREL has developed an implementation of the algorithm in C.  License information is available at this link.

Solar Variability Zones

Page • Matthew Lave, Robert J. Broderick, Matthew J. Reno, Solar variability zones: Satellite-derived zones that represent high-frequency ground variability, Solar Energy, Volume 151, 15 July 2017, Pages 119-128, ISSN 0038-092X. Abstract: To determine the impact of solar variability to electric grid operations, appropriate samples of solar variability must be used, but determining appropriate variability...

Spectral Content

Page • The spectral content of sunlight is influenced by a number of atmospheric factors, including the amount of water vapor and other aerosols in the atmosphere.  The figure below compares spectra at the top of the atmosphere, from a theoretical blackbody at 5,250 deg C, and for typical sunlight at sea...

Spectral Mismatch Models

Page • Spectral mismatch models are part of the translation from broadband plane-of-array (POA) irradiance to effective irradiance. Generally, the translation takes the form $$E_e=M\times\{IAM_B\times E_b + E_{diff}\} \times SF$$ where $$M$$ is the spectral mismatch modifier, $$IAM_B$$ is the reflection losses for the beam irradiance $$E_b$$  (i.e., $$DNI\times\cos(AOI)$$) , $$E_{diff}$$ is the diffuse POA irradiance and $$SF$$ is the soiling factor.  Models...

Spectral Response

Page • PV devices are characterized by their response to light in a reference spectrum.  When a device is tested in a lab or outdoors, the spectrum of the light source may not be the same as that of the reference spectrum.  The effect of this difference on performance is typically quantified by...

Sun Position

Page • The position of the sun relative to an observer on the surface of the Earth is an important input needed to model PV system performance.  The convention used to describe solar position includes: Zenith angle ($$\Theta_{Z}$$)Azimuth angle ($$\Theta_{A}$$))Solar elevation angle () is equal to $$90^o-\Theta_{Z}$$ The figure below shows how...

temp downloads

Page • Large-Scale PV Plant Performance Benchmarking (9563 downloads ) Latest Developments in Solar Irradiance Measurement (10906 downloads ) Latest Developments in Solar Irradiance Measurement (11589 downloads ) Latest developments in solar irradiance measurement; improving measurement accuracy, improving data availability (10694 downloads ) LCOE Reduction Through Proactively Optimized PV System Monitoring (10704...

Tools

Page • Originally developed at Sandia National Laboratories, this open-source PV performance modeling library is the gold-standard source for published models and algorithms. It is currently maintained by a diverse team of PV system experts. Source code is available on GitHub. Please see the Installation page for installation help. For examples of how to...

Two-Axis Tracking

Page • Two-axis tracking allows the array to be pointed normal to the Sun in order to maximize the irradiance hitting the array.  This results in an angle of incidence equal to zero. At Sandia National Laboratories, we have a two-axis tracker that we use to characterize PV modules, shown below. There are...

View Factor Models

Page • View factor models are used for radiative transfer calculations of the amount of radiation leaving one surface (A) that reaches a second surface (B). The view factor $$F_{A\rightarrow B}$$ is the fraction of the radiation from surface A that hits surface B. In the context of bifacial PV arrays, the surface B...

Wavelet Variability Model

Page • This is a help file for the pvl_WVM MatLab code. It contains links to examples and some FAQs. Click here to Download pvl_WVM Matlab Code Contents: What the WVM doesWVM Code Syntax and Required InputsExamplesDetermining the Cloud SpeedConvert WVM Smoothed Irradiance to Power OutputReferencesBSD License What the WVM does The WVM models the...

Weather and Design

Page • Obtaining irradiance and weather data is typically the first step in setting up and running a PV performance model.  Historical data is typically used to predict output of proposed systems, while real or near-real time data is used to model the output expected from an operating system to validate that...

Weather Data Sources for Performance Modeling

Page • Obtaining high quality weather and irradiance data for performance modeling studies is one of the most important steps in PV performance modeling, since the uncertainty in the irradiance data usually accounts a large amount of the total uncertainty.  The modeler usually starts with historical data that has been compiled especially...

Weather Observations

Page • Weather or atmospheric observations can be made to improve the performance of some models. Some weather measurements have small variations and can be approximated based upon location (e.g. atmospheric pressure can be estimated from site elevation). Others, such as air temperature, which have greater variation and play a strong role...

Wind Speed and Direction

Page • Wind speed is measured with an anemometer.  The most common type is a the cup-type anemometer, shown on the right side of the picture below.  The number of rotations per time interval is used to calculate the wind speed.  The vane on the left is used to measure the direction...

Workshops

Page • Upcoming Workshops 2025 European PVPMC Workshop - Ayia Napa, Cyprus (29-30 October 2025) Call for Abstracts is closed. Check back soon for program and registration information. Co-hosted by EPL Technology Frontiers Ltd, Phaethon Centre of Excellence at the University of Cyprus, and Sandia National Laboratories this workshop will cover all...

Workshops & Publications

Page • Workshops– Past and Future workshops, including links to presentationsIEA PVPS Task 13 Reports - Reports from this international R&D organization related to PV performance and reliability.Sandia Reports - Listing of PV related SAND reports

WVM Discrete Point Example

Page • This example uses May 18th, 2014 irradiance data collected at Sandia National Laboratories in Livermore, CA to demonstrate use of the wavelet variability model (WVM). Contents load datadefine variablesrun WVMplot the WVM results load data This file contains two vectors: “GHI” which is the GHI measurements, and “dt” which is...
Results 126–150 of 151