Abstract. We present a case study of unusual spread-F structures observed by
ionosondes at two equatorial and low-latitude Brazilian stations – São Luís
(SL: 44.2∘ W, 2.33∘ S; dip angle: −6.9∘)
and Fortaleza (FZ: 38.45∘ W, 3.9∘ S; dip angle:
−16∘). The irregularity structures observed from midnight to
postmidnight hours of moderate solar activity (F10.7 < 97 sfu,
where 1 sfu = 10−22 W m−2 s−1) have characteristics different
from typical post-sunset equatorial spread F. The spread-F traces first
appeared at or above the F-layer peak and gradually became well-formed mixed
spread F. They also appeared as plasma depletions in the 630.0 nm airglow
emissions made by a wide-angle imager located at the nearby low-latitude station
Cajazeiras (CZ: 38.56∘ W, 6.87∘ S; dip angle:
−21.4∘). The irregularities appeared first over FZ and later over
SL, giving evidence of an unusual westward propagation or a horizontal
plasma advection. The drift-mode operation available in one of the
ionosondes (a digital portable sounder, DPS-4) has enabled us to analyze the
horizontal drift velocities and directions of the irregularity movement. We
also analyzed the neutral wind velocity measured by a Fabry–Pérot
interferometer (FPI) installed at CZ and discuss its possible role in the
development of the irregularities.