Penetration of internal gravity waveguide modes into the upper atmosphere

Penetration of internal gravity waveguide modes into the upper atmosphere

Blog Article

The paper igora vibrance 6-12 describes internal gravity waveguide modes, using dissipative solutions above the source.We compare such a description with an accurate approach 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 collirio drop set 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 in the upper atmosphere.