Penetration of internal gravity waveguide modes into the upper atmosphere

Penetration of internal gravity waveguide modes into the upper atmosphere

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The paper describes internal gravity waveguide modes, using dissipative solutions above the source.We compare such a description with an accurate approach smok rpm c coils and a WKB approximation for dissipationless equations.For waveguide disturbances, dispersion relations calculated by any method are shown to be close to each other and to be in good agreement with observed characteristics of traveling ionospheric disturbances.Unlike other methods, dissipative solutions above the source allow us to adequately describe the spatial structure of disturbances vlone stop snitching shirt in the upper atmosphere.