Cloud motion and stability estimation for intra-hour solar forecasting

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Cloud motion and stability estimation for intra-hour solar forecasting. / Chow, Chi Wai; Belongie, Serge; Kleissl, Jan.

I: Solar Energy, Bind 115, 01.06.2015, s. 645-655.

Publikation: Bidrag til tidsskriftTidsskriftartikelForskningfagfællebedømt

Harvard

Chow, CW, Belongie, S & Kleissl, J 2015, 'Cloud motion and stability estimation for intra-hour solar forecasting', Solar Energy, bind 115, s. 645-655. https://doi.org/10.1016/j.solener.2015.03.030

APA

Chow, C. W., Belongie, S., & Kleissl, J. (2015). Cloud motion and stability estimation for intra-hour solar forecasting. Solar Energy, 115, 645-655. https://doi.org/10.1016/j.solener.2015.03.030

Vancouver

Chow CW, Belongie S, Kleissl J. Cloud motion and stability estimation for intra-hour solar forecasting. Solar Energy. 2015 jun. 1;115:645-655. https://doi.org/10.1016/j.solener.2015.03.030

Author

Chow, Chi Wai ; Belongie, Serge ; Kleissl, Jan. / Cloud motion and stability estimation for intra-hour solar forecasting. I: Solar Energy. 2015 ; Bind 115. s. 645-655.

Bibtex

@article{3f9f7ee110934f0884025755a35d45c0,
title = "Cloud motion and stability estimation for intra-hour solar forecasting",
abstract = "Techniques for estimating cloud motion and stability for intra-hour forecasting using a ground-based sky imaging system are presented. A variational optical flow (VOF) technique was used to determine the sub-pixel accuracy of cloud motion for every pixel. Cloud locations up to 15. min ahead were forecasted by inverse mapping of the cloud map. A month of image data captured by a sky imager at UC San Diego was analyzed to compare the accuracy of VOF forecast with cross-correlation method (CCM) and image persistence method. The VOF forecast with a fixed smoothness parameter was found to be superior to image persistence forecast for all forecast horizons for almost all days and outperform CCM forecast with an average error reduction of 39%, 21%, 19%, and 19% for 0, 5, 10, and 15. min forecasts respectively. Optimum forecasts may be achieved with forecast-horizon-dependent smoothness parameters. In addition, cloud stability and forecast confidence was evaluated by correlating point trajectories with forecast error. Point trajectories were obtained by tracking sub-sampled pixels using optical flow field. Point trajectory length in mintues was shown to increase with decreasing forecast error and provide valuable information for cloud forecast confidence at forecast issue time.",
keywords = "Cloud motion tracking, Cloud stability, Sky imager, Solar forecast",
author = "Chow, {Chi Wai} and Serge Belongie and Jan Kleissl",
note = "Publisher Copyright: {\textcopyright} 2015 Elsevier Ltd.",
year = "2015",
month = jun,
day = "1",
doi = "10.1016/j.solener.2015.03.030",
language = "English",
volume = "115",
pages = "645--655",
journal = "Solar Energy",
issn = "0038-092X",
publisher = "Elsevier Limited",

}

RIS

TY - JOUR

T1 - Cloud motion and stability estimation for intra-hour solar forecasting

AU - Chow, Chi Wai

AU - Belongie, Serge

AU - Kleissl, Jan

N1 - Publisher Copyright: © 2015 Elsevier Ltd.

PY - 2015/6/1

Y1 - 2015/6/1

N2 - Techniques for estimating cloud motion and stability for intra-hour forecasting using a ground-based sky imaging system are presented. A variational optical flow (VOF) technique was used to determine the sub-pixel accuracy of cloud motion for every pixel. Cloud locations up to 15. min ahead were forecasted by inverse mapping of the cloud map. A month of image data captured by a sky imager at UC San Diego was analyzed to compare the accuracy of VOF forecast with cross-correlation method (CCM) and image persistence method. The VOF forecast with a fixed smoothness parameter was found to be superior to image persistence forecast for all forecast horizons for almost all days and outperform CCM forecast with an average error reduction of 39%, 21%, 19%, and 19% for 0, 5, 10, and 15. min forecasts respectively. Optimum forecasts may be achieved with forecast-horizon-dependent smoothness parameters. In addition, cloud stability and forecast confidence was evaluated by correlating point trajectories with forecast error. Point trajectories were obtained by tracking sub-sampled pixels using optical flow field. Point trajectory length in mintues was shown to increase with decreasing forecast error and provide valuable information for cloud forecast confidence at forecast issue time.

AB - Techniques for estimating cloud motion and stability for intra-hour forecasting using a ground-based sky imaging system are presented. A variational optical flow (VOF) technique was used to determine the sub-pixel accuracy of cloud motion for every pixel. Cloud locations up to 15. min ahead were forecasted by inverse mapping of the cloud map. A month of image data captured by a sky imager at UC San Diego was analyzed to compare the accuracy of VOF forecast with cross-correlation method (CCM) and image persistence method. The VOF forecast with a fixed smoothness parameter was found to be superior to image persistence forecast for all forecast horizons for almost all days and outperform CCM forecast with an average error reduction of 39%, 21%, 19%, and 19% for 0, 5, 10, and 15. min forecasts respectively. Optimum forecasts may be achieved with forecast-horizon-dependent smoothness parameters. In addition, cloud stability and forecast confidence was evaluated by correlating point trajectories with forecast error. Point trajectories were obtained by tracking sub-sampled pixels using optical flow field. Point trajectory length in mintues was shown to increase with decreasing forecast error and provide valuable information for cloud forecast confidence at forecast issue time.

KW - Cloud motion tracking

KW - Cloud stability

KW - Sky imager

KW - Solar forecast

UR - http://www.scopus.com/inward/record.url?scp=84926040320&partnerID=8YFLogxK

U2 - 10.1016/j.solener.2015.03.030

DO - 10.1016/j.solener.2015.03.030

M3 - Journal article

AN - SCOPUS:84926040320

VL - 115

SP - 645

EP - 655

JO - Solar Energy

JF - Solar Energy

SN - 0038-092X

ER -

ID: 301829678