论文标题

在地磁活动期间,用GNSS和Navic在印度纵向部门上的电离层模型的比较研究

Comparative studies of Ionospheric models with GNSS and NavIC over the Indian Longitudinal sector during geomagnetic activities

论文作者

Chakraborty, Sumanjit, Datta, Abhirup, Ray, Sarbani, Ayyagari, Deepthi, Paul, Ashik

论文摘要

本文介绍了全球电离层模型最新版本的性能的风暴时间比较分析:国际参考层(IRI)2016,NEQUICK 2(NEQ)和IRI扩展到Plasmasphere(IRI-P)2017,涉及与印度星座(NAVIC)和全球导航卫星系统(GNSSSSSSSSSSSSSSSERIVER ELECTER ELECTIRES ELECTIRED ELECTIRED ELECTIRED INOSERINED INOSERINED INOSPERISED INOSPERISED INOSPERIND INOSPERISED INOSPERNONCER)有关(NAVIC)2017。该分析是在2017年9月至2018年9月至2018年9月9日的不同地磁风暴条件下进行的,在太阳周期的下降阶段。位于磁性赤道附近的异常波峰和磁赤道和班加罗尔之间的海得拉巴已被分析。除IRI-P外,这些模型通常在暴风雨期间高估了,除了IRI-P之外,该模型与2017年9月7日(在2017年9月的强烈风暴期间)从Anomaly Crest周围的车站观察到的增强型(约为3-5 TECU)。其他两个模型未观察到显着匹配。 IRI-P的这种匹配归因于等离子体的贡献以及将测得的TEC值吸收到该模型中的能力。在本研究中,据我们所知,经验模型的首次比较TEC与来自磁性赤道的IGS观测值与IGS观测值与超越rest的位置相结合的navic和gnss测量是在地面磁性干扰条件下进行的。由于导体卫星处于较高的海拔高度(约36000公里),因此将航海数据纳入现有模型可以给印度次大陆提供更好的电离层预测。

This paper presents the storm time comparative analysis of the performances of latest versions of global ionospheric models: International Reference Ionosphere (IRI) 2016, NeQuick 2 (NeQ) and the IRI extended to Plasmasphere (IRI-P) 2017 with respect to Navigation with Indian Constellation (NavIC) and Global Navigation Satellite System (GNSS) derived ionospheric Total Electron Content (TEC). The analysis is carried out under varying geomagnetic storm conditions during September 2017-November 2018, falling in the declining phase of solar cycle 24. TEC data from Indore, located near the northern crest of the Equatorial Ionization Anomaly (EIA) along with data obtained from the International GNSS Service (IGS) stations at Lucknow, located beyond the anomaly crest; Hyderabad, located between anomaly crest and magnetic equator and Bangalore, located near the magnetic equator have been analysed. The models generally overestimated during the storm periods with the exception of IRI-P, which matched (with an offset of about 3-5 TECU) with the enhancement observed on September 7, 2017 (during the strong storm of September 2017), from stations around the anomaly crest. No significant match was observed by the other two models. This match of IRI-P is attributed to the plasmaspheric contribution as well as the capability of assimilating measured TEC values into this model. In the present study, to the best of our knowledge, first comparisons of the empirical model derived TEC with NavIC and GNSS measurements from an anomaly crest location, combined with the IGS observations from the magnetic equator to locations beyond the anomaly crest, are conducted during geomagnetically disturbed conditions. Since NavIC satellites are at higher altitudes(~ 36000 km), the inclusion of NavIC data to the existing model could give better ionospheric predictions over the Indian subcontinent.

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