Control of equatorial ionospheric morphology by atmospheric tides

被引:558
作者
Immel, T. J. [1 ]
Sagawa, E.
England, S. L.
Henderson, S. B.
Hagan, M. E.
Mende, S. B.
Frey, H. U.
Swenson, C. M.
Paxton, L. J.
机构
[1] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
[2] Natl Inst Informat & Commun Technol, Tokyo 1849795, Japan
[3] Utah State Univ, Dept Elect & Comp Engn, Logan, UT 84322 USA
[4] Natl Ctr Atmospher Res, High Altitude Observ, Boulder, CO 80307 USA
[5] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA
关键词
D O I
10.1029/2006GL026161
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
A newly discovered 1000-km scale longitudinal variation in ionospheric densities is an unexpected and heretofore unexplained phenomenon. Here we show that ionospheric densities vary with the strength of nonmigrating, diurnal atmospheric tides that are, in turn, driven mainly by weather in the tropics. A strong connection between tropospheric and ionospheric conditions is unexpected, as these upward propagating tides are damped far below the peak in ionospheric density. The observations can be explained by consideration of the dynamo interaction of the tides with the lower ionosphere (E-layer) in daytime. The influence of persistent tropical rainstorms is therefore an important new consideration for space weather.
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页数:4
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