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• W2009384295 abstract "Lunar semidiurnal tides are introduced at the lower boundary of the National Center for Atmospheric Research Thermosphere‐Ionosphere‐Electrodynamics General Circulation Model (TIEGCM). The tides are derived from the model of Vial and Forbes [1994] and interesting properties of these tides are found when they are subjected to Hough decomposition; there is considerable hemispherical antisymmetry in the September tides, and the March and September modal compositions are significantly different. A differencing method is used to isolate the lunar tidal effects in the TIEGCM, and these are compared with lunar tidal analyses of ionospheric data. The model reproduces the broad features of the lunar tide in f 0 F 2 (maximum frequency of the F region) with phase changes around 7° magnetic dip latitude during daytime. The model and data analysis both give variations of the amplitude and phase of the lunar tide with local time. Near the equator the variation of phase with local time changes with latitude as the equatorial anomaly develops during the day. Comparison between the model predictions and analyses of data at observatories at midlatitudes produces mixed results. Here the effects of the lunar components of both electrodynamic drifts and of neutral winds need to be taken into account. Several cases of day to night changes in the phase of the lunar tide in f 0 F 2 are noted. Large nighttime amplitudes of the lunar tide in h m F 2 (height of the maximum density), more than 4 km, seem to be due to inphase action of the electrodynamic and neutral wind effects while during daytime they are out of phase. The lunar tide in the ratio of oxygen to nitrogen density [O]/[N 2 ]is estimated and found to be of relatively minor importance. Amplitudes of the lunar tide in f 0 F 2 may be measured at more than 0.4 MHz at some local times, but the model values are less than this. Comparison is also made with ion drift measurements made by the San Marco D satellite. The several uncertainties which underlie this work are discussed in detail." @default.
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• W2009384295 date "1999-01-01" @default.
• W2009384295 modified "2023-09-26" @default.
• W2009384295 title "Lunar tides in the Thermosphere-Ionosphere-Electrodynamics General Circulation Model" @default.
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• W2009384295 doi "https://doi.org/10.1029/98ja02663" @default.
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