“…Now, we will restrict ourselves with the searching the global and resonant atmosphere modes among these determined by the solution of Dispersion Equation (A16), as it is noted in the text of our paper (see Section 3 in particular). This is important due to the global character of the sources (such as global terminator and X-ray flares), with the influence of these on the ionosphere being studied in the present paper; note that the global Lamb modes of the atmosphere are also excited effectively by the seismogenic sources, which are considered in the present paper as well, in accordance with [ 20 , 21 ]. To consider the roots of interest of the relation (A16), note that, in the absence of any sources in the system (A14), the roots of Equation (A16) coincide with the roots of the equation The coefficients included in the dispersion equation in the form (A17) determine the polarization relations for AGWs: From the dispersion equation presented in (A17), we present the characteristics of the global evanescent or reactive Lamb waves (see Equation ( 9 ), Section 3 ) and Brunt–Väisälä oscillations (Equation ( 10 ), Section 3 ) [ 20 , 55 , 56 , 57 , 58 , 59 ].…”