Overestimation of the Bottom-Side Ionospheric TEC in the IRI Model Over Low Latitude Regions

IF 2.9 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS
K. Venkatesh, H. Kava, D. Pallamraju, Gopi K. Seemala
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Abstract

It is known that the ionospheric Total Electron Content (TEC) variations estimated by the IRI model show large differences from observed values over the low latitudes. While studies on the topside ionospheric contributions to the errors in the modeled TEC by the IRI are under active consideration, there have been no studies on the role of the contribution of the bottom-side ionosphere. As ionosondes provide the true information on the bottom-side TEC, in this work a comparative study has been carried out in discerning the role of various parameters that go into the estimates of bottom-side density profiles and electron content in the IRI model (TECb_iri). The digisonde measurements over a low latitude location, Ahmedabad, India are used to estimate the bottom-side electron content (TECb_digi) during 2015 and 2018. It is found that the TECb_iri is overestimated during day time irrespective of the season and solar activity. The maximum differences in TECb_digi are noted during equinoctial months and high solar activity period. Among the F-layer peak and profile parameters, the model differences in the bottom-side thickness (B0) are found to be consistent with the differences in the TECb_iri. The agreements and discrepancies between TECb_iri and TECb_digi, under the influence of complex electrodynamic processes and solar flux are discussed. This study provides crucial information required to delineate the contributions of different empirical parameters in the IRI to address the discrepancies that exist in the bottom-side ionospheric modeling over low latitudes.

IRI模式对低纬度地区电离层底部TEC的高估
众所周知,IRI模式估计的电离层总电子含量(TEC)变化在低纬度地区与观测值有很大差异。虽然目前正在积极研究上部电离层对IRI模拟的TEC误差的贡献,但还没有关于底部电离层贡献作用的研究。由于离子探空仪提供了关于底侧TEC的真实信息,因此在这项工作中进行了一项比较研究,以确定各种参数在IRI模型(TECb_iri)中对底侧密度剖面和电子含量的估计中的作用。在印度艾哈迈达巴德低纬度地区的digisonde测量用于估计2015年和2018年的底部电子含量(TECb_digi)。发现无论季节和太阳活动如何,白天的TECb_iri都被高估了。在分点月和太阳活动高峰期,TECb_digi差异最大。在f层峰型参数和剖面参数中,底部厚度(B0)的模型差异与TECb_iri的模型差异一致。讨论了在复杂电动力过程和太阳通量的影响下,TECb_iri和TECb_digi的一致性和差异性。该研究提供了描述IRI中不同经验参数的贡献所需的关键信息,以解决低纬度地区底部电离层模拟中存在的差异。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Journal of Geophysical Research: Space Physics
Journal of Geophysical Research: Space Physics Earth and Planetary Sciences-Geophysics
CiteScore
5.30
自引率
35.70%
发文量
570
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