Fig. 11From: Statistical study of medium-scale traveling ionospheric disturbances in low-latitude ionosphere using an automatic algorithmComparison between the propagation directions of MSTIDs and the AGWs derived from WACCM. The gray lines are the MSTID propagation direction during 2013–2015, and the blue line represents the averaged value during 2013–2015, while the dashed line indicates the MSTIDs are rarely detected. The red line with stars displays the corresponding WACCM resultsBack to article page