In-situ plasma density measurements from the CHAMP satellite between about 350-420 km altitude are used to delineate intra-annual variations in the longitudinal structure of the F-region ionosphere. It is shown that the longitude structures during mid-day local times are dominated by the space-based longitudinal wavenumbers k(s) = 2, 4 and 3 in January, July and December, respectively. These conform to the same dominating k(s)-values characterizing solar thermal tide zonal winds in the dynamo region, namely the westward-propagating semidiurnal tide with planetary-fixed zonal wavenumber s = 4 (SW4), and the eastward-propagating diurnal tides with s =-3 (DE3) and s =-2 (DE2), respectively. DE3 is the dominating tide during the other months. The results presented indicate that nonmigrating tides other than DE3 may significantly impact the longitudinal structure of the low-latitude ionosphere during certain months.
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Natl Ctr Atmospher Res, High Altitude Observ, Pob 3000, Boulder, CO 80307 USA
Univ Corp Atmospher Res, COSMIC Program Off, Boulder, CO 80305 USANatl Ctr Atmospher Res, High Altitude Observ, Pob 3000, Boulder, CO 80307 USA
Pedatella, N. M.
Lu, G.
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机构:
Natl Ctr Atmospher Res, High Altitude Observ, Pob 3000, Boulder, CO 80307 USANatl Ctr Atmospher Res, High Altitude Observ, Pob 3000, Boulder, CO 80307 USA
Lu, G.
Richmond, A. D.
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Natl Ctr Atmospher Res, High Altitude Observ, Pob 3000, Boulder, CO 80307 USANatl Ctr Atmospher Res, High Altitude Observ, Pob 3000, Boulder, CO 80307 USA