Solar position algorithm for solar radiation applications
By I. Reda, A. Andreas. 2004
1,319 citations recorded by the source corpus.
Subfields: Artificial Intelligence, Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/06e2d210ff6aadd7eea14aca39a1be21e1b00dbe
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In Artificial Intelligence
In Astronomy and Astrophysics
Citations in the corpus
- A worldwide cost-based design and optimization of tilted bifacial solar farms (2018, methodology): “The solar path can be acquired/simulated by using the NREL’s solar position algorithm [33] which has been implemented in Sandia PV modeling library (PVLib) [34].”
- The Sun’s apparent position and the optimal tilt angle of a solar collector in the northern hemisphere (2009, methodology): “Using the Julian date system, Reda and Andreas (2004) proposed a step by step procedure for calculating the solar azimuth and zenith angles in the period from the year � 2000 to 6000, with an uncertainty of only ±0.0003.”
- Quality control of global solar radiation using sunshine duration hours (2009, methodology): “To compute God and N, the reader is referred to Reda and Andreas [9].”
- Optimization and performance of bifacial solar modules: A global perspective (2017, methodology): “use the NREL's solar position algorithm [24] implemented in the Sandia PV modeling library [25] to simulate the solar path—specifically, the solar zenith ( θZ ) and azimuth ( γS ) angles at any arbitrary time and geographic location.”
- Torsion-balance tests of the weak equivalence principle (2012, methodology): “0003 ̋ in the azimuth and zenith angles [104].”
- Very short term irradiance forecasting using the lasso (2015, methodology): “We use the53 solar positioning algorithm developed by Reda and Andreas (2008) for extraterrestrial irradiance calculation.54 Finally, we include a zenith angle filter of 80◦.55 1.2.”
- Global horizontal irradiance clear sky models : implementation and analysis. (2012, methodology): “The most recent Solar Position Algorithm (SPA) developed by NREL in 2004 calculates the solar position with very low uncertainty based on location, date, and time inputs for the years -2000–6000 [9].”