2010
DOI: 10.1016/j.jastp.2010.01.015
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Optical observations of plasma bubble westward drifts over Brazilian tropical region

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Cited by 19 publications
(19 citation statements)
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References 36 publications
(42 reference statements)
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“…2, and as suggested earlier, observations could have been made under disturbed dynamo conditions (Blanc and Richmond 1980;Fejer et al 2017). Westward motion of the ionospheric irregularities are known to occur during disturbed dynamo (Abdu et al 2003;Paulino et al 2010), and therefore, our observations confirm the occurrence of low-latitude disturbances.…”
Section: Event 3: August 3-4 2016supporting
confidence: 89%
“…2, and as suggested earlier, observations could have been made under disturbed dynamo conditions (Blanc and Richmond 1980;Fejer et al 2017). Westward motion of the ionospheric irregularities are known to occur during disturbed dynamo (Abdu et al 2003;Paulino et al 2010), and therefore, our observations confirm the occurrence of low-latitude disturbances.…”
Section: Event 3: August 3-4 2016supporting
confidence: 89%
“…This is the first report of such a distinct pattern of spread F for the Brazilian equatorial region, though it was observed earlier at the low-latitude station CP (Brazil) for the solar minimum 2008-2009 by Candido et al (2011). By distinct we mean that it occurs in postmidnight hours propagating westward, which is not usually observed during solar minimum unless there is a previous eastward EPB structure propagation, as mentioned by Paulino et al (2010). A careful analysis of equatorial ionograms and other plots from digisonde soundings suggests modifications in the ionospheric plasma density structuring, such as those associated with plasma density depletions, which are responsible for a variety of spread-F-layer patterns.…”
Section: Discussionmentioning
confidence: 54%
“…The depletions also propagated over CZ (350 km south of FZ) with mean westward velocities ∼ 60 m s −1 , which are similar to the propagation velocities of the irregularities observed with the digisonde at FZ. Some authors have demonstrated that EPBs can also present westward propagation after midnight during quiet times (Paulino et al, 2010;Sobral et al, 2011). However, those studies reported that the depletions associated with EPBs should first present movement to the east earlier in the evening and reversal westward at later hours.…”
Section: Depletions In the Airglow Oi 6300 Nm Imagesmentioning
confidence: 98%
“…It has been designed to keep track of the spatial and temporal variations of OH, OI5577, 6300 nm airglow emissions (e.g. Paulino et al, 2010).…”
Section: The All Sky Imagermentioning
confidence: 99%