Journal
ANNALES GEOPHYSICAE
Volume 22, Issue 9, Pages 3137-3143Publisher
COPERNICUS GESELLSCHAFT MBH
DOI: 10.5194/angeo-22-3137-2004
Keywords
ionosphere; equatorial ionosphere; ionospheric irregularities; atmospheric composition and structure; air-glow and aurora
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Temporal and spatial evolution of two high-altitude plasma bubbles (evening and midnight) was observed on 4 April 2002, at geomagnetic conjugate points at Sata, Japan (magnetic latitude 24degrees N), and Darwin, Australia (magnetic latitude 22degrees S), using two 630-nm airglow imagers. The apex height of the bubbles reached similar to1500km. The upward velocity of the evolution was faster in the evening (similar to170m/s at 20:00-21:00 LT) than around midnight (similar to28 m/s at 23:00-00:00 LT). Bifurcating features of the bubbles into a smaller scale size of similar to50 km were clearly seen for both the evening and midnight bubbles, showing fairly good conjugacy between the Northern and Southern Hemispheres.
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