An approach for generating synthetic fine temporal resolution solar radiation time series from hourly gridded datasets

A tool has been developed to statistically increase the temporal resolution of solar irradiance time series. Fine temporal resolution time series are an important input into the planning process for solar power plants, and lead to increased understanding of the likely short-term variability of solar...

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Main Authors: Matthew Perry, Alberto Troccoli
Format: Article
Language:English
Published: Borntraeger 2017-06-01
Series:Meteorologische Zeitschrift
Subjects:
Online Access:http://dx.doi.org/10.1127/metz/2016/0746
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spelling doaj-3c8725582375427fa15b5ffb7c8b5bb72020-11-24T23:07:10ZengBorntraegerMeteorologische Zeitschrift0941-29482017-06-0126326527610.1127/metz/2016/074687148An approach for generating synthetic fine temporal resolution solar radiation time series from hourly gridded datasetsMatthew PerryAlberto TroccoliA tool has been developed to statistically increase the temporal resolution of solar irradiance time series. Fine temporal resolution time series are an important input into the planning process for solar power plants, and lead to increased understanding of the likely short-term variability of solar energy. The approach makes use of the spatial variability of hourly gridded datasets around a location of interest to make inferences about the temporal variability within the hour. The unique characteristics of solar irradiance data are modelled by classifying each hour into a typical weather situation. Low variability situations are modelled using an autoregressive process which is applied to ramps of clear-sky index. High variability situations are modelled as a transition between states of clear sky conditions and different levels of cloud opacity. The methods have been calibrated to Australian conditions using 1 min data from four ground stations for a 10 year period. These stations, together with an independent dataset, have also been used to verify the quality of the results using a number of relevant metrics. The results show that the method generates realistic fine resolution synthetic time series. The synthetic time series correlate well with observed data on monthly and annual timescales as they are constrained to the nearest grid-point value on each hour. The probability distributions of the synthetic and observed global irradiance data are similar, with Kolmogorov-Smirnov test statistic less than 0.04 at each station. The tool could be useful for the estimation of solar power output for integration studies.http://dx.doi.org/10.1127/metz/2016/0746solar irradiancesolar powersynthetictime seriesspatial variabilityfine temporal resolution
collection DOAJ
language English
format Article
sources DOAJ
author Matthew Perry
Alberto Troccoli
spellingShingle Matthew Perry
Alberto Troccoli
An approach for generating synthetic fine temporal resolution solar radiation time series from hourly gridded datasets
Meteorologische Zeitschrift
solar irradiance
solar power
synthetic
time series
spatial variability
fine temporal resolution
author_facet Matthew Perry
Alberto Troccoli
author_sort Matthew Perry
title An approach for generating synthetic fine temporal resolution solar radiation time series from hourly gridded datasets
title_short An approach for generating synthetic fine temporal resolution solar radiation time series from hourly gridded datasets
title_full An approach for generating synthetic fine temporal resolution solar radiation time series from hourly gridded datasets
title_fullStr An approach for generating synthetic fine temporal resolution solar radiation time series from hourly gridded datasets
title_full_unstemmed An approach for generating synthetic fine temporal resolution solar radiation time series from hourly gridded datasets
title_sort approach for generating synthetic fine temporal resolution solar radiation time series from hourly gridded datasets
publisher Borntraeger
series Meteorologische Zeitschrift
issn 0941-2948
publishDate 2017-06-01
description A tool has been developed to statistically increase the temporal resolution of solar irradiance time series. Fine temporal resolution time series are an important input into the planning process for solar power plants, and lead to increased understanding of the likely short-term variability of solar energy. The approach makes use of the spatial variability of hourly gridded datasets around a location of interest to make inferences about the temporal variability within the hour. The unique characteristics of solar irradiance data are modelled by classifying each hour into a typical weather situation. Low variability situations are modelled using an autoregressive process which is applied to ramps of clear-sky index. High variability situations are modelled as a transition between states of clear sky conditions and different levels of cloud opacity. The methods have been calibrated to Australian conditions using 1 min data from four ground stations for a 10 year period. These stations, together with an independent dataset, have also been used to verify the quality of the results using a number of relevant metrics. The results show that the method generates realistic fine resolution synthetic time series. The synthetic time series correlate well with observed data on monthly and annual timescales as they are constrained to the nearest grid-point value on each hour. The probability distributions of the synthetic and observed global irradiance data are similar, with Kolmogorov-Smirnov test statistic less than 0.04 at each station. The tool could be useful for the estimation of solar power output for integration studies.
topic solar irradiance
solar power
synthetic
time series
spatial variability
fine temporal resolution
url http://dx.doi.org/10.1127/metz/2016/0746
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