“…Especially in the low‐latitude ionosphere, the vertical plasma drift velocities ( E × B drifts) that are so critical in defining the structure and variability of the EIA depend crucially on the solar tides (England et al, , ; Maute et al, ; Millward et al, ; Tarpley, , ). A variety of nonmigrating tides, especially nonmigrating diurnal eastward propagating wave number 2 and 3 (DE2 and DE3, respectively), contribute to the plasma zonal structure (Hagan et al, ; England , ; Kil et al, ; McDonald et al, ) near the equator. The DE3 tide has been linked to the wave‐4 pattern in the EIA when viewed at a constant local time (e.g., Immel et al, ), whereas DE2 is a contributor to the wave‐3 pattern that typically emerges in the boreal winter months (Forbes et al, ; Kil et al, ; Pancheva & Mukhtarov, ), although other tides (e.g., DW4, DE2, and SW5) play a role (McDonald et al, ).…”