The height-dependent delayed ionospheric response to solar EUV - data comparison - secondary files 141 - 143

<strong>Secondary files for doy 141 - 143</strong> For comparison with the observational results a TIE-GCM v2.0 model run in the 2.5 × 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’s OMNI data set<strong>年积日（DOY）141至143的辅助文件</strong> 为与观测结果开展对比，本研究以2.5×2.5的分辨率配置运行了TIE-GCM v2.0模型。为使模型收敛至稳定初始状态，在2019年3月28日启动的最终模拟前，模型先行运行了30天，该预运行阶段采用默认参数配置。2019年4月27日至2019年5月24日的最终模拟运行采用TIE-GCM默认配置，并以希利斯电对流场模型（Heelis Electric Convection Field Model，Heelis等，1982）作为高纬度电势模型。模拟所需的输入强迫场数据取自NASA/GSFC的OMNI数据集。