Validation of the IRI-2020 model for the topside-plasmasphere using GNSS TEC measurements

IF 2.8 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Advances in Space Research Pub Date : 2025-03-01 Epub Date: 2024-07-08 DOI:10.1016/j.asr.2024.07.009
Nina Servan-Schreiber , Malini Aggarwal , Yuyang Huang , Minwook Kang , Abdalla Shaker , Dieter Bilitza
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Abstract

The 2020 update of the International Reference Ionosphere (IRI) model introduces a new topside option, COR2, for the formulation of its electron density profile, as well as two plasmaspheric extension options based on the GCPM model of Gallagher et al. (2000) and the IMAGE/RPI model of Ozhogin et al. (2012). We validate the COR2-Gallagher and COR2-Ozhogin topside-plasmasphere options of IRI-2020 using GNSS VTEC measurements and compare them to the NeQuick model used as the default option in IRI-2016. VTEC data from a total of 21 GNSS ground-based receivers are compared to predictions of the IRI model, ranging from low (< 30°) to middle (30°-60°) magnetic latitudes, during high (year 2014; F10.7140 sfu) and low (year 2019; F10.770 sfu) solar activity. Peak plasma frequency (foF2) data from co-located digisondes are ingested into the model to ensure the relevance of the comparison. The three topside-plasmasphere options perform equally well at mid-latitudes (RMSE3 TECU). At low latitudes, the NeQuick option (RMSE9 TECU) performs better than both the COR2-Gallagher and COR2-Ozhogin options (RMSE > 10 TECU). For all options, the modeled VTEC is consistently overestimated during the autumn/winter daytime at mid-latitudes regardless of solar activity, and throughout the day at low latitudes during low solar activity.
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利用全球导航卫星系统 TEC 测量结果验证 IRI-2020 顶侧等离子体模型
2020年更新的国际参考电离层(IRI)模型引入了一个新的上层选项COR2,用于制定其电子密度曲线,以及基于Gallagher等人(2000)的GCPM模型和Ozhogin等人(2012)的IMAGE/RPI模型的两个等离子体扩展选项。我们使用GNSS VTEC测量值验证了IRI-2020的COR2-Gallagher和COR2-Ozhogin顶面等离子层选项,并将其与作为IRI-2016默认选项的NeQuick模型进行了比较。来自21个GNSS地面接收器的VTEC数据与IRI模型的预测进行了比较,范围从低(<;磁极高纬度(2014年)至中纬度(30°-60°);F10.7 ~ 140 sfu)和低(2019年;F10.7 ~ 70 sfu)太阳活动。在模型中输入了来自同一位置的双轴仪的峰值等离子体频率(foF2)数据,以确保比较的相关性。在中纬度地区,三种上层等离子体层方案的表现同样良好(RMSE ~ 3 TECU)。在低纬度地区,NeQuick选项(RMSE ~ 9 TECU)的性能优于COR2-Gallagher和COR2-Ozhogin选项(RMSE >;10特)。对于所有选项,无论太阳活动如何,模拟的VTEC在中纬度地区秋冬白天始终被高估,在太阳活动不活跃的低纬度地区全天都被高估。
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来源期刊
Advances in Space Research
Advances in Space Research 地学天文-地球科学综合
CiteScore
5.20
自引率
11.50%
发文量
800
审稿时长
5.8 months
期刊介绍: The COSPAR publication Advances in Space Research (ASR) is an open journal covering all areas of space research including: space studies of the Earth''s surface, meteorology, climate, the Earth-Moon system, planets and small bodies of the solar system, upper atmospheres, ionospheres and magnetospheres of the Earth and planets including reference atmospheres, space plasmas in the solar system, astrophysics from space, materials sciences in space, fundamental physics in space, space debris, space weather, Earth observations of space phenomena, etc. NB: Please note that manuscripts related to life sciences as related to space are no more accepted for submission to Advances in Space Research. Such manuscripts should now be submitted to the new COSPAR Journal Life Sciences in Space Research (LSSR). All submissions are reviewed by two scientists in the field. COSPAR is an interdisciplinary scientific organization concerned with the progress of space research on an international scale. Operating under the rules of ICSU, COSPAR ignores political considerations and considers all questions solely from the scientific viewpoint.
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