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Rethinking solar resource assessments in the context of global dimming and brightening

: Müller, B.; Wild, M.; Driesse, A.; Behrens, K.

Preprint urn:nbn:de:0011-n-2799055 (522 KByte PDF)
MD5 Fingerprint: 65b871c2c7296b02046e36a93b09b4a8
Created on: 25.4.2014

Solar energy 99 (2014), pp.272-282
ISSN: 0038-092X
ISSN: 0375-9865
Journal Article, Electronic Publication
Fraunhofer ISE ()
Photovoltaische Module; Systeme und Zuverlässigkeit; Energieeffiziente Gebäude; Photovoltaische Module und Kraftwerke; Solarthermie; Systemintegration und Netze – Strom; Wärme; Gas; Energieeffiziente Leistungselektronik; Energiesystemanalyse; Lichttechnik; Kühlung und Klimatisierung von Gebäuden; Gebrauchsdauer von Modulen und Materialien; Photovoltaische Kraftwerke; Bauwerksintegrierte Photovoltaik; Thermische Solaranlagen; Solarthermische Kraftwerke; Betriebsführung von Energieversorgungssystemen; Autonome Stromversorgungen und Inselnetze; Kraftwerkseinsatzplanung und Betriebsstrategien; Nationale und regionale Energieversorgungskonzepte; Modellierung von Energieversorgungsszenarien; radiation; irradiance; resource assessment; dimming and brightening

Solar resource assessments use solar radiation data from past observations to estimate the average annual solar radiation over the expected lifetime for a solar energy system. However, solar radiation at the Earth’s surface is not stable over time but undergoes significant long-term variations often referred to as “global dimming and brightening”. This study analyzes the effect of these long-term trends on solar resource assessments. Based on long-term measurement records in Germany, it is found that the additional uncertainty of solar resource assessments caused by long-term trends in solar radiation is about 3% on the horizontal plane and even higher for tilted or tracked planes. These additional uncertainties are not included in most uncertainty calculations for solar resource assessments up to now. Furthermore, for the measurement stations analyzed, the current irradiance level is about 5% above the long-term average of the years 1951–2010. Since the direction of future trends in solar radiation is not known, different possibilities to estimate the future solar resource are compared. In view of long-term trends that could extend beyond the period of past observations and beyond the projected lifetime of a solar energy application, a paradigm shift is proposed: instead of using the longest possible period to calculate an average value, only the 10 most recent years should be used as the estimator for future solar irradiance.