“…Model simulations show that primary GWs excited by deep convection can propagate well into the thermosphere, where they break or dissipate (Vadas & Liu, , ; Vadas & Crowley, ). This process creates intermittent, localized body forces which excite secondary GWs having λ H ∼100–1,000 s km (Vadas & Crowley, ); these secondary GWs then propagate to much higher altitudes and create significant variability in the neutral wind (Vadas & Crowley, ). Additionally, these secondary GWs enhance the variability of the ionosphere by creating medium to large‐scale traveling ionospheric disturbances via ion drag (Azeem et al, ; Nicolls et al, ; Vadas & Crowley, ; Vadas & Nicolls, ).…”