Intra-Hour Cloud Tracking Based on Probability Hypothesis Density Filtering

IEEE Swift variations in the cloud cover may cause significant power output fluctuations in solar power systems, jeopardizing power quality. Forecasting the power output with a very short horizon below 30 seconds can be seen as a cloud cover forecasting problem solved by processing images from a sky...

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Main Authors: Barbieri, F., Rifflart, C., Vo, Ba Tuong, Rajakaruna, Sumedha, Ghosh, A.
Format: Journal Article
Published: The Institute of Electrical and Electronic Engineers (IEEE) 2017
Online Access:http://hdl.handle.net/20.500.11937/58574
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author Barbieri, F.
Rifflart, C.
Vo, Ba Tuong
Rajakaruna, Sumedha
Ghosh, A.
author_facet Barbieri, F.
Rifflart, C.
Vo, Ba Tuong
Rajakaruna, Sumedha
Ghosh, A.
author_sort Barbieri, F.
building Curtin Institutional Repository
collection Online Access
description IEEE Swift variations in the cloud cover may cause significant power output fluctuations in solar power systems, jeopardizing power quality. Forecasting the power output with a very short horizon below 30 seconds can be seen as a cloud cover forecasting problem solved by processing images from a sky camera. After a pre-processing stage that identifies clouds with a criterion based on the red-green blue (RGB) values of each pixel, a Probability Hypothesis Density (PHD) filter or a more advanced Cardinalized Probability Hypothesis Density (CPHD) filter can be used to an unknown and varying number of clouds. The time when cumulus clouds will shade the sun can be forecasted with an absolute precision 6 seconds ahead and with an acceptable accuracy 27 seconds ahead. It has been found that both filters are equally well-suited for a real-time online nowcasting application. They also have the potential to deal with noise and the swift dynamics and high variability of clouds.
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institution Curtin University Malaysia
institution_category Local University
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publishDate 2017
publisher The Institute of Electrical and Electronic Engineers (IEEE)
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spelling curtin-20.500.11937-585742017-11-24T05:46:58Z Intra-Hour Cloud Tracking Based on Probability Hypothesis Density Filtering Barbieri, F. Rifflart, C. Vo, Ba Tuong Rajakaruna, Sumedha Ghosh, A. IEEE Swift variations in the cloud cover may cause significant power output fluctuations in solar power systems, jeopardizing power quality. Forecasting the power output with a very short horizon below 30 seconds can be seen as a cloud cover forecasting problem solved by processing images from a sky camera. After a pre-processing stage that identifies clouds with a criterion based on the red-green blue (RGB) values of each pixel, a Probability Hypothesis Density (PHD) filter or a more advanced Cardinalized Probability Hypothesis Density (CPHD) filter can be used to an unknown and varying number of clouds. The time when cumulus clouds will shade the sun can be forecasted with an absolute precision 6 seconds ahead and with an acceptable accuracy 27 seconds ahead. It has been found that both filters are equally well-suited for a real-time online nowcasting application. They also have the potential to deal with noise and the swift dynamics and high variability of clouds. 2017 Journal Article http://hdl.handle.net/20.500.11937/58574 10.1109/TSTE.2017.2733258 The Institute of Electrical and Electronic Engineers (IEEE) restricted
spellingShingle Barbieri, F.
Rifflart, C.
Vo, Ba Tuong
Rajakaruna, Sumedha
Ghosh, A.
Intra-Hour Cloud Tracking Based on Probability Hypothesis Density Filtering
title Intra-Hour Cloud Tracking Based on Probability Hypothesis Density Filtering
title_full Intra-Hour Cloud Tracking Based on Probability Hypothesis Density Filtering
title_fullStr Intra-Hour Cloud Tracking Based on Probability Hypothesis Density Filtering
title_full_unstemmed Intra-Hour Cloud Tracking Based on Probability Hypothesis Density Filtering
title_short Intra-Hour Cloud Tracking Based on Probability Hypothesis Density Filtering
title_sort intra-hour cloud tracking based on probability hypothesis density filtering
url http://hdl.handle.net/20.500.11937/58574