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Statistics of GPS TEC at the northern EIA crest region of the Indian subcontinent during the solar cycle 24 (2013-2018): comparison with IRI-2016 and IRI-2012 models

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Abstract

In this study the statistics of ionospheric total electron content (TEC), derived from a GSV4004B dual-frequency Global Positioning System (GPS) receiver at Agartala station (23.450°N, 91.150°E) located in northern equatorial ionization anomaly (EIA) crest region of the Indian subcontinent, is reported with a performance analysis of IRI-2016 and IRI-2012 models during the ascending, maxima, declining and minima phases (2013-2018) of the solar cycle 24. Variations of model total electron content, as obtained from the IRI-2016 and IRI-2012 for the three options of topside electron density namely NeQuick, IRI 2001 and IRI 01-corr, are compared with the observed total electron content during different periods of interest viz. monthly, seasonal, annual and the correlations with solar activity parameters viz. sunspot number (SSN), 10.7 cm solar radio flux (F10.7), solar EUV flux, are also investigated. All the three options of IRI-2016 and IRI-2012 models show an earlier occurrence of diurnal maximum total electron content, as compared to the observed diurnal maximum GPS total electron content, throughout all the months during the complete period of observation. As the solar activity decreases (from 2015 to 2018), the model starts underestimating GPS total electron content, which becomes significantly high during the very low solar activity period of 2017-18 for all the months. IRI-2016 model underestimates the GPS total electron content before the hours of diurnal maximum and overestimates after the hours of diurnal maximum in the years from 2013-2018. IRI-2012 model underestimates the GPS total electron content before the hours of diurnal maximum and overestimates after the hours of diurnal maximum in the years from 2013-17 but overestimate during the whole day in the year of 2018. Overestimation by IRI-2012 is much more than that by IRI-2016 in the year of 2018. Predictions given by IRI-2016 are better than that given by IRI-2012 for our region. The seasonal mean maximum total electron content values are highest during the spring equinox months and lowest during the winter months except the year of 2014 and 2013. The correlation analysis, between the GPS total electron content and solar indices, show that the correlation coefficient is higher for the solar EUV flux, as compared to the sunspot number (SSN) and 10.7 cm solar radio flux (F10.7).

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Acknowledgements

The authors gratefully acknowledge the Department of Physics, Tripura University for providing infrastructure to carry out the research. The authors are thankful to NASA for providing open access of the IRI-2016 and IRI-2012 model data (https://ccmc.gsfc.nasa.gov/modelweb/models/iri2016_vitmo.php and https://ccmc.gsfc.nasa.gov/modelweb/models/iri2012_vitmo.php), Sunspot number or SSN data (omniweb.gsfc.nasa.gov/form/dx1.html) and to NOAA for the 10.7 cm solar radio flux or F10.7 data (www.ngdc.noaa.gov/stp/space-weather/solar-data). The authors are thankful to Solar and Heliospheric Observatory (SOHO) for solar EUV flux data (dornsifecms.usc.edu/space-sciences-center/download-sem-data/). The authors are also thankful to World Data Center for Geomagnetism, Kyoto (wdc.kugi.kyoto-u.ac.jp/dstdir/) for providing international quiet and disturbed day’s data and to Global UltraViolet Imager onboard TIMED/GUVI satellites (guvitimed.jhuapl.edu/guvi-galleryl3on2) for global [O/N2] maps. The authors are grateful to DST FIST, Govt. of India for funding the research through the DST FIST fund (Ref. No SR/FST/PSI-191/2014). The authors are also grateful to UGC, Govt. of India for financial support to carry out this research through the financial assistance under the UGC – SAP program 2016 (Ref. No. F.530/23/DRS-I/2018 (SAP-I)).

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  1. Iswarchandra Vidyasagar College, Belonia, Tripura, India

    Arup Patari

  2. Department of Physics, Tripura University, Agartala, India

    Bapan Paul & Anirban Guha

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  1. Arup Patari
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Patari, A., Paul, B. & Guha, A. Statistics of GPS TEC at the northern EIA crest region of the Indian subcontinent during the solar cycle 24 (2013-2018): comparison with IRI-2016 and IRI-2012 models. Astrophys Space Sci 366, 46 (2021). https://doi.org/10.1007/s10509-021-03950-6

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