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Zonal neutral winds at equatorial and low latitudes

โœ Scribed by C. Martinis; J. Meriwether; R. Niciejewski; M. Biondi; C. Fesen; M. Mendillo


Publisher
Elsevier Science
Year
2001
Tongue
English
Weight
316 KB
Volume
63
Category
Article
ISSN
1364-6826

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โœฆ Synopsis


Fabry-Perot interferometric (FPI) measurements of thermospheric zonal neutral winds at Arequipa, Peru (16:7 โ€ข S; 71:5 โ€ข W; -2:7 โ€ข dip), and Carmen Alto, Chile (23:1 โ€ข S; 69:4 โ€ข W; -10:2 โ€ข dip), were collected during the solar minimum periods of September-October 1996 and 1997. The data set included 39 nights from Arequipa and 14 nights for Carmen Alto, with 8 nights of simultaneous observations. Analysis of averaged results found the peak evening zonal neutral wind speed of โˆผ127 ยฑ 15 m=s eastward for the Arequipa observatory, which is located near the magnetic equator, to occur between 21:30 and 22:30 LT. In contrast, the peak evening zonal winds of โˆผ100 ยฑ 10 m=s eastward observed from Carmen Alto, which is located near the crest of the equatorial ionization anomaly (EIA), occurred โˆผ 0:5-1 h later. These measurements represent the รฟrst case of groundbased FPI observations of the so called equatorial temperature and wind anomaly (ETWA) over such a small latitude range in the same longitude sector. This reduction in speed of โˆผ 20-25% at Carmen Alto relative to Arequipa is attributed to increased ion drag at Carmen Alto caused by the higher electron density within the EIA region at altitudes of 220 -300 km. Model studies were conducted using electron density and neutral atmosphere parameters form the parameterized ionospheric model (PIM) and the mass spectrometer incoherent scatter (MSIS) models, respectively, to calculate the ratio of ion-neutral collision frequencies at the two sites. We found that the increase in electron density within the EIA was su cient to account for the observed reduction in the zonal wind. Thus, this analysis conรฟrms the dominant role of ion drag in modulating thermospheric dynamics at equatorial latitudes. A comparison of the FPI results with the predictions by two current neutral wind models, the Horizontal Wind Model-90 and the NCAR Thermospheric Ionosphere Electrodynamics General Circulation Model (TIEGCM), reveals that neither is able to reproduce accurately the latitude dependence reported here. Model reรฟnements for electrodynamics and improved resolution are suggested.


๐Ÿ“œ SIMILAR VOLUMES


A comparison between observed and geostr
โœ Charles L. Jordan ๐Ÿ“‚ Article ๐Ÿ“… 1953 ๐Ÿ› John Wiley and Sons ๐ŸŒ English โš– 232 KB

## Abstract Lowโ€latitude wind and pressure data are used to determine the mean departure of the actual wind speed from the geostrophic speed. The computed departure becomes progressively greater equatorward of 30ยฐN and attains a magnitude of about 10 m/sec at 10ยฐN.