The height-dependent delayed ionospheric response to solar EUV - data comparison - secondary files 129 - 134

<strong>Secondary files for doy 129 - 134</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129至134的辅助文件</strong> 为与观测结果开展对比，本研究采用2.5×2.5配置的TIE-GCM v2.0模式开展模拟计算。为使模式收敛至稳定初始状态，在2019年3月28日启动最终模拟前，模式先行运行30天以完成预热。该预热运行采用默认参数配置。2019年4月27日至2019年5月24日的最终模拟运行，采用TIE-GCM的默认配置，并以希利斯电场对流模型（Heelis Electric Convection Field Model，Heelis等，1982）作为高纬度电势模型。模拟所需的强迫场输入数据取自NASA/GSFC的OMNI数据集。