Wind Energy Resources at Antarctic Stations Based on ERA5

The harsh scientific research environment of Antarctic stations demands a reliable energy supply; however, traditional methods not only pose a challenge in supply but also harm the environment. Antarctic energy supply has become a new choice for energy development in Antarctica due to its abundant w...

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Published in:Atmosphere
Main Authors: Kaishan Wang, Di Wu, Jinping Wu, Shuang Li, Xinye Zhao, Chongwei Zheng, Yue Yu, Kai Wu
Format: Article in Journal/Newspaper
Language:English
Published: MDPI AG 2023
Subjects:
Online Access:https://doi.org/10.3390/atmos14121732
https://doaj.org/article/0daa62b092714bfd8cffba56707d1411
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spelling ftdoajarticles:oai:doaj.org/article:0daa62b092714bfd8cffba56707d1411 2024-01-21T10:01:51+01:00 Wind Energy Resources at Antarctic Stations Based on ERA5 Kaishan Wang Di Wu Jinping Wu Shuang Li Xinye Zhao Chongwei Zheng Yue Yu Kai Wu 2023-11-01T00:00:00Z https://doi.org/10.3390/atmos14121732 https://doaj.org/article/0daa62b092714bfd8cffba56707d1411 EN eng MDPI AG https://www.mdpi.com/2073-4433/14/12/1732 https://doaj.org/toc/2073-4433 doi:10.3390/atmos14121732 2073-4433 https://doaj.org/article/0daa62b092714bfd8cffba56707d1411 Atmosphere, Vol 14, Iss 12, p 1732 (2023) Antarctic wind energy Antarctic station ERA5 Meteorology. Climatology QC851-999 article 2023 ftdoajarticles https://doi.org/10.3390/atmos14121732 2023-12-24T01:38:07Z The harsh scientific research environment of Antarctic stations demands a reliable energy supply; however, traditional methods not only pose a challenge in supply but also harm the environment. Antarctic energy supply has become a new choice for energy development in Antarctica due to its abundant wind energy resources. Using ERA5 10 m wind field reanalysis data, we compared and analyzed the correlation (r) and Root Mean Square Error (RMSE) between some observation stations and reanalysis data, with correlations above 0.67 and root mean square error below 2.3. This indicates that the accuracy of the ERA5 data is suitable for resource assessment at stations in Antarctica. We assessed the wind energy potential of the Great Wall, Zhongshan, Kunlun and Taishan Stations. The results show that the annual distribution and long-term trend of wind energy at Taishan Station are the best, followed by the Great Wall, Zhongshan and Kunlun Stations. Taishan Station has stable wind direction and abundant wind energy, the average wind power density is 800 W/m 2 , with an annual growth trend of 2.02 W/m 2 ·yr −1 . The effective wind speed occurrence and energy level occurrence are generally above 90% and the coefficient of variation is generally below 0.8. The dominant direction of wind energy is northeast and the wind direction is stable, which is conducive to the development and utilization of wind energy. Article in Journal/Newspaper Antarc* Antarctic Antarctica Directory of Open Access Journals: DOAJ Articles Antarctic Zhongshan ENVELOPE(76.371,76.371,-69.373,-69.373) Atmosphere 14 12 1732
institution Open Polar
collection Directory of Open Access Journals: DOAJ Articles
op_collection_id ftdoajarticles
language English
topic Antarctic
wind energy
Antarctic station
ERA5
Meteorology. Climatology
QC851-999
spellingShingle Antarctic
wind energy
Antarctic station
ERA5
Meteorology. Climatology
QC851-999
Kaishan Wang
Di Wu
Jinping Wu
Shuang Li
Xinye Zhao
Chongwei Zheng
Yue Yu
Kai Wu
Wind Energy Resources at Antarctic Stations Based on ERA5
topic_facet Antarctic
wind energy
Antarctic station
ERA5
Meteorology. Climatology
QC851-999
description The harsh scientific research environment of Antarctic stations demands a reliable energy supply; however, traditional methods not only pose a challenge in supply but also harm the environment. Antarctic energy supply has become a new choice for energy development in Antarctica due to its abundant wind energy resources. Using ERA5 10 m wind field reanalysis data, we compared and analyzed the correlation (r) and Root Mean Square Error (RMSE) between some observation stations and reanalysis data, with correlations above 0.67 and root mean square error below 2.3. This indicates that the accuracy of the ERA5 data is suitable for resource assessment at stations in Antarctica. We assessed the wind energy potential of the Great Wall, Zhongshan, Kunlun and Taishan Stations. The results show that the annual distribution and long-term trend of wind energy at Taishan Station are the best, followed by the Great Wall, Zhongshan and Kunlun Stations. Taishan Station has stable wind direction and abundant wind energy, the average wind power density is 800 W/m 2 , with an annual growth trend of 2.02 W/m 2 ·yr −1 . The effective wind speed occurrence and energy level occurrence are generally above 90% and the coefficient of variation is generally below 0.8. The dominant direction of wind energy is northeast and the wind direction is stable, which is conducive to the development and utilization of wind energy.
format Article in Journal/Newspaper
author Kaishan Wang
Di Wu
Jinping Wu
Shuang Li
Xinye Zhao
Chongwei Zheng
Yue Yu
Kai Wu
author_facet Kaishan Wang
Di Wu
Jinping Wu
Shuang Li
Xinye Zhao
Chongwei Zheng
Yue Yu
Kai Wu
author_sort Kaishan Wang
title Wind Energy Resources at Antarctic Stations Based on ERA5
title_short Wind Energy Resources at Antarctic Stations Based on ERA5
title_full Wind Energy Resources at Antarctic Stations Based on ERA5
title_fullStr Wind Energy Resources at Antarctic Stations Based on ERA5
title_full_unstemmed Wind Energy Resources at Antarctic Stations Based on ERA5
title_sort wind energy resources at antarctic stations based on era5
publisher MDPI AG
publishDate 2023
url https://doi.org/10.3390/atmos14121732
https://doaj.org/article/0daa62b092714bfd8cffba56707d1411
long_lat ENVELOPE(76.371,76.371,-69.373,-69.373)
geographic Antarctic
Zhongshan
geographic_facet Antarctic
Zhongshan
genre Antarc*
Antarctic
Antarctica
genre_facet Antarc*
Antarctic
Antarctica
op_source Atmosphere, Vol 14, Iss 12, p 1732 (2023)
op_relation https://www.mdpi.com/2073-4433/14/12/1732
https://doaj.org/toc/2073-4433
doi:10.3390/atmos14121732
2073-4433
https://doaj.org/article/0daa62b092714bfd8cffba56707d1411
op_doi https://doi.org/10.3390/atmos14121732
container_title Atmosphere
container_volume 14
container_issue 12
container_start_page 1732
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