Abstract

The Empirical Canadian High Arctic Ionospheric Model (E-CHAIM) is a new empirical model of high latitude ionospheric electron density. While the introductory studies regarding E-CHAIM include validations, E-CHAIM’s topside model was notably excluded from independent validation using datasets not included in the model fitting. In this study, we undertake such a validation using in situ electron density observations from the Defense Meteorological Satellite Program (DMSP) constellation of satellites and the Challenging Mini-satellite Payload (CHAMP) mission. Through this validation, we show that E-CHAIM generally outperforms the International Reference Ionosphere (IRI) at DMSP orbit (~830 km altitude), with RMS errors of 8.3–9.8 × 109 e/m3 versus the IRI’s 1.2–1.3 × 1010 e/m3. E-CHAIM’s improvement over the IRI is consistent at all latitudes but is particularly noted in sub-auroral regions and is mainly limited to summer and equinox periods. At CHAMP orbit, E-CHAIM and the IRI are found to perform largely comparably, with E-CHAIM outperforming the IRI only marginally with RMS errors of 7.11 × 1010 e/m3 versus the IRI’s 7.48 × 1010 e/m3. This improvement is found to be largely constrained to sub-auroral latitudes with both models performing comparably at higher latitudes. An observed tendency for the IRI to overestimate electron density in the near-peak (at CHAMP orbit) and underestimate electron density at higher altitudes (DMSP orbit) appears to be consistent with previous work, which identified this pattern to result from shortcomings in the NeQuick topside function curvature at high latitudes.

Highlights

  • The Empirical Canadian High Arctic Ionospheric Model (E-CHAIM) is a relatively new empirical representation of high latitude (>50° N geomagnetic latitude) electron density (Themens et al, 2017a, 2018)

  • It is here demonstrated that E-CHAIM performs well in its representation of topside electron density and, at high altitudes, represents a noted improvement over the International Reference Ionosphere (IRI)

  • The IRI demonstrates a notable tendency to underestimate summer and equinox electron density, at high solar activity where it underestimates monthly averaged electron density by as much as 60%. For these same equinox and summer periods at high altitudes, E-CHAIM performs substantially better than the IRI with errors within 25%

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Summary

Introduction

The Empirical Canadian High Arctic Ionospheric Model (E-CHAIM) is a relatively new empirical representation of high latitude (>50° N geomagnetic latitude) electron density (Themens et al, 2017a, 2018). Due to a limited dataset and the desire to use all available topside electron density profiles for the fitting of the model, independent validation of the E-CHAIM topside has not yet been undertaken. While the above changes were demonstrated to provide a significant improvement with respect to the fitting dataset, further validation against independent datasets is necessary For this purpose, we have here gathered over a decade of in situ electron density observations from the Defense Meteorological Satellite Program (DMSP) constellation of satellites and the Challenging Mini-satellite Payload (CHAMP) mission. We have here gathered over a decade of in situ electron density observations from the Defense Meteorological Satellite Program (DMSP) constellation of satellites and the Challenging Mini-satellite Payload (CHAMP) mission These instruments have been used previously to evaluate the performance of other empirical models, like the IRI and NeQuick, on global scales.

DMSP in situ electron density
CHAMP in situ electron density
E-CHAIM
Overall comparison
Morning and evening seasonal and solar cycle variations
Validation of E-CHAIM using CHAMP
CHAMP validation
Findings
Discussion
Conclusions
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