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SolarPosition.jl

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SolarPosition.jl provides a simple, unified interface to a collection of validated solar position algorithms written in pure, performant julia.

Solar positioning algorithms are commonly used to calculate the solar zenith and azimuth angles, which are essential for various applications where the sun is important, such as:

  • Solar energy systems
  • Building design
  • Climate studies
  • Astronomy

Acknowledgement

This package is based on the work done by readers in the field of solar photovoltaics in the packages solposx and pvlib-python. In particular the positioning and refraction methods have been adapted from solposx, while the SPA algorithm and the deltat calculation are ported from pvlib-python. These packages also provide validation data necessary to ensure correctness of the algorithm implementations.

Example Usage

using SolarPosition, Dates

# define observer location (latitude, longitude, altitude in meters)
obs = Observer(52.35888, 4.88185, 100.0)  # Van Gogh Museum, Amsterdam

# a few hours of timestamps
times = collect(DateTime(2023, 6, 21, 10):Hour(1):DateTime(2023, 6, 21, 15));

# compute solar positions for all timestamps
positions = solar_position(obs, times)
6-element StructArray(::Vector{Float64}, ::Vector{Float64}, ::Vector{Float64}) with eltype SolPos{Float64}:
 SolPos(azimuth=136.1908215897601°, elevation=55.13208390809107°, zenith=34.86791609190893°)
 SolPos(azimuth=160.3753655770986°, elevation=59.974081481305134°, zenith=30.025918518694862°)
 SolPos(azimuth=188.3992597996431°, elevation=60.87918930278924°, zenith=29.120810697210757°)
 SolPos(azimuth=214.62987222053295°, elevation=57.493462259959394°, zenith=32.5065377400406°)
 SolPos(azimuth=235.5258846451899°, elevation=50.992647293443966°, zenith=39.007352706556034°)
 SolPos(azimuth=251.77304757136397°, elevation=42.790197455865076°, zenith=47.209802544134924°)

Solar positioning algorithms

Here we provide an overview of the solar positioning algorithms currently implemented in SolarPosition.jl. Each algorithm is described with its reference paper, claimed accuracy and implementation status.

AlgorithmReferenceAccuracyDefault RefractionStatus
PSABlanco-Muriel et al.±0.0083°None
NOAAGlobal Monitoring Laboratory±0.0167°HUGHES
WalravenWalraven, 1978±0.0100°None
USNOU.S. Naval Observatory±0.0500°None
SPAReda & Andreas, 2004±0.0003°Built-in

Refraction correction algorithms

Atmospheric refraction correction algorithms available in SolarPosition.jl.

AlgorithmReferenceAtmospheric ParametersStatus
HUGHESHughes, 1985Pressure, Temperature
ARCHERArcher et al., 1980None
BENNETTBennett, 1982Pressure, Temperature
MICHALSKYMichalsky, 1988None
SG2Blanc & Wald, 2012Pressure, Temperature
SPARefractionReda & Andreas, 2004Pressure, Temperature

How to Cite

If you use SolarPosition.jl in your work, please cite using the reference given in CITATION.cff.

Contributing

If you want to make contributions of any kind, please first that a look into our contributing guide directly on GitHub or the contributing page on the website