STORM-TIME PENETRATION TO LOW LATITUDES OF MAGNETOSPHERIC-IONOSPHERICCONVECTION AND CONVECTION-DRIVEN THERMOSPHERIC WINDS

Authors
Citation
Ca. Reddy et Hg. Mayr, STORM-TIME PENETRATION TO LOW LATITUDES OF MAGNETOSPHERIC-IONOSPHERICCONVECTION AND CONVECTION-DRIVEN THERMOSPHERIC WINDS, Geophysical research letters, 25(16), 1998, pp. 3075-3078
Citations number
30
Categorie Soggetti
Geosciences, Interdisciplinary
ISSN journal
00948276
Volume
25
Issue
16
Year of publication
1998
Pages
3075 - 3078
Database
ISI
SICI code
0094-8276(1998)25:16<3075:SPTLLO>2.0.ZU;2-J
Abstract
From DE-2 satellite measurements during two magnetic storms, we show t hat (i) the magnetospheric convection-driven east-west ion flows of hi gh velocities (1400 m/s) penetrate to magnetic latitudes as low as 30 degrees, with larger velocities (2000-3000 m/s) appearing at 45 degree s 50 degrees latitudes, and (ii) high velocities (300-640 m/s) thermos pheric winds appear in association with the : above ion flows. The sim ilarity of the latitude structures and time evolutions of the ion and neutral motions indicates that the zonal winds are driven by ma,magnet ospheric-ionospheric convection through ion drag. These velocities of the convection-driven ion flows and winds at such low latitudes are mu ch larger than those reported from observations or predicted by curren t models.