Determination of nighttime VTEC average in the Klobuchar ionospheric delay model
The Klobuchar model has been widely used to correct the ionospheric delay in applications. However, the NVTEC (Nighttime Vertical Total Electron Content) of the Klobuchar model employs an empirical constant of 9 TECU (Total Electron Content Unit) at L1 frequency. In this paper, the rationality and r...
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2018-03-01
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doaj-39545b694c8843db84dfa635109c1fba2021-02-02T07:11:04ZengKeAi Communications Co., Ltd.Geodesy and Geodynamics1674-98472018-03-0192175182Determination of nighttime VTEC average in the Klobuchar ionospheric delay modelWeili Zhou0Shuli Song1Qinming Chen2Na Cheng3Hui Xie4Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, 200030, China; University of Chinese Academy of Sciences, Beijing, 100049, China; Corresponding author.Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, 200030, ChinaShanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, 200030, ChinaShanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, 200030, China; University of Chinese Academy of Sciences, Beijing, 100049, ChinaShanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, 200030, China; University of Chinese Academy of Sciences, Beijing, 100049, ChinaThe Klobuchar model has been widely used to correct the ionospheric delay in applications. However, the NVTEC (Nighttime Vertical Total Electron Content) of the Klobuchar model employs an empirical constant of 9 TECU (Total Electron Content Unit) at L1 frequency. In this paper, the rationality and reliability of the nighttime constant setting are investigated using the GIM (Global Ionosphere Map) product of the IGS (International GNSS Service) from 1998 to 2015. Our study indicates that the suitable time span of NVTEC average in nighttime should be between 20:00 and 06:00 LT (local time). The NVTEC is highly correlated with seasons, having positive extremes in spring and autumn and negative extremes in summer through the mean values in all latitudes. In addition to seasonal dependence, solar activity in the solar cycle 23 strongly influences NVTEC as well and leads to its variation within a range between 25 and 30 TECU in spring and autumn at solar maximum, which is about 1.5 times greater than that in summer and winter. The NVTEC also has a dependence on the latitude at solar maximum, with the mean value from 30 TECU in low latitudinal regions to 15 TECU in high latitudinal regions. Therefore, these results demonstrate that the nighttime VTEC has much greater deviations from the imperial constant in the Klobuchar model, and the newly estimated constant is expected to bring improvement to the predictability of the Klobuchar ionospheric delay model in nighttime. Keywords: Klobuchar model, Ionospheric correction, Nighttime VTEC, Global ionosphere maphttp://www.sciencedirect.com/science/article/pii/S1674984716301872 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Weili Zhou Shuli Song Qinming Chen Na Cheng Hui Xie |
spellingShingle |
Weili Zhou Shuli Song Qinming Chen Na Cheng Hui Xie Determination of nighttime VTEC average in the Klobuchar ionospheric delay model Geodesy and Geodynamics |
author_facet |
Weili Zhou Shuli Song Qinming Chen Na Cheng Hui Xie |
author_sort |
Weili Zhou |
title |
Determination of nighttime VTEC average in the Klobuchar ionospheric delay model |
title_short |
Determination of nighttime VTEC average in the Klobuchar ionospheric delay model |
title_full |
Determination of nighttime VTEC average in the Klobuchar ionospheric delay model |
title_fullStr |
Determination of nighttime VTEC average in the Klobuchar ionospheric delay model |
title_full_unstemmed |
Determination of nighttime VTEC average in the Klobuchar ionospheric delay model |
title_sort |
determination of nighttime vtec average in the klobuchar ionospheric delay model |
publisher |
KeAi Communications Co., Ltd. |
series |
Geodesy and Geodynamics |
issn |
1674-9847 |
publishDate |
2018-03-01 |
description |
The Klobuchar model has been widely used to correct the ionospheric delay in applications. However, the NVTEC (Nighttime Vertical Total Electron Content) of the Klobuchar model employs an empirical constant of 9 TECU (Total Electron Content Unit) at L1 frequency. In this paper, the rationality and reliability of the nighttime constant setting are investigated using the GIM (Global Ionosphere Map) product of the IGS (International GNSS Service) from 1998 to 2015. Our study indicates that the suitable time span of NVTEC average in nighttime should be between 20:00 and 06:00 LT (local time). The NVTEC is highly correlated with seasons, having positive extremes in spring and autumn and negative extremes in summer through the mean values in all latitudes. In addition to seasonal dependence, solar activity in the solar cycle 23 strongly influences NVTEC as well and leads to its variation within a range between 25 and 30 TECU in spring and autumn at solar maximum, which is about 1.5 times greater than that in summer and winter. The NVTEC also has a dependence on the latitude at solar maximum, with the mean value from 30 TECU in low latitudinal regions to 15 TECU in high latitudinal regions. Therefore, these results demonstrate that the nighttime VTEC has much greater deviations from the imperial constant in the Klobuchar model, and the newly estimated constant is expected to bring improvement to the predictability of the Klobuchar ionospheric delay model in nighttime. Keywords: Klobuchar model, Ionospheric correction, Nighttime VTEC, Global ionosphere map |
url |
http://www.sciencedirect.com/science/article/pii/S1674984716301872 |
work_keys_str_mv |
AT weilizhou determinationofnighttimevtecaverageintheklobucharionosphericdelaymodel AT shulisong determinationofnighttimevtecaverageintheklobucharionosphericdelaymodel AT qinmingchen determinationofnighttimevtecaverageintheklobucharionosphericdelaymodel AT nacheng determinationofnighttimevtecaverageintheklobucharionosphericdelaymodel AT huixie determinationofnighttimevtecaverageintheklobucharionosphericdelaymodel |
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1724299874904571904 |