作者: Jeffrey M. Forbes , Henry B. Garrett
DOI: 10.1175/1520-0469(1978)035<0148:SLSOTD>2.0.CO;2
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摘要: Abstract The seasonal-latitudinal structure of the diurnal thermospheric tide is investigated for minimum and maximum levels solar activity by numerically solving linearized inseparable tidal equations a spherical, rotating, viscous atmosphere with anisotropic ion drag. Variations in F-region ionospheric zenith angle dependence EUV heat source are major factors controlling tide. combined interaction solar-cycle dependent background temperature profile (which controls altitude diffusion dominance) variations seasonal plasma sunspot leads to variation morphology For instance, summer-winter differences winds at given height more pronounced during SSMAX as opposed SSMIN. At level activity, westerly winds, vertical temperatures a...