The height-dependent delayed ionospheric response to solar EUV - data comparison

<p>For comparison with the observational results a TIE-GCM v2.0 model run in the 2.5 &times; 2.5 configuration is calculated. In order to converge to stable initial condition the model runs for 30 days prior to the final simulation starting at 28 March 2019. This initial run is configured with default parameters. The final run from 27 April 2019 to 24 May 2019 uses the default configuration of TIE-GCM with the Heelis Electric Convection Field Model (Heelis et al., 1982) as the high-latitude potential model. The input forcing is used from the NASA/GSFC&rsquo;s OMNI data set</p> <p>Secondary files:</p> <p>117 - 122: <a href="https://zenodo.org/record/6004534">https://zenodo.org/record/6004534</a></p> <p>123 - 128: <a href="https://zenodo.org/record/6006516">https://zenodo.org/record/6006516</a></p> <p>129 - 134: <a href="https://zenodo.org/record/6009777">https://zenodo.org/record/6009777</a></p> <p>135 - 140: <a href="https://zenodo.org/record/6014195">https://zenodo.org/record/6014195</a></p> <p>141 - 143: <a href="https://zenodo.org/record/6014201">https://zenodo.org/record/6014201</a></p> <p>&nbsp;</p>