We show evidence for the occurrence of the equatorial temperature anomaly (
ETA) during solar minimum by analyzing the temperature and total ion densit
y data from the Neutral Atmosphere Temperature Experiment (NATE) and the Cy
lindrical Electrostatic Probe (CEP), respectively, on board the Atmospheric
Explorer-E satellite. The chosen data refer to a height of similar to 254
km in the African and Asian longitude sector (340, I degreesE-200 degreesE)
during a summer season in the Southern Hemisphere. As during the solar max
imum period, the spatial characteristics of the ETA are similar to those of
the equatorial ionization anomaly (EIA). A minimum in the gas temperature
is collocated with the minimum in the ion density at the dip equator, and a
temperature maximum on the south side of the equator is collocated with th
e density maximum of the EIA. The daytime behavior of ETA formation is abou
t the same as that of EIA as both of them are clearly present at around 130
0 and 1400 local solar time (LST) only. At 1400 LST the difference between
the temperatures at the crest and the trough (ETA strength) reaches a maxim
um value of about 100 degreesK which is similar to 14% of the temperature a
t the trough. Like the EIA, the ETA also suddenly disappears after 1400 LST
, Thus the EIA appears to be a prerequisite for the ETA formation. During t
he premidnight time (2200 LST), however, while the EIA is nonexistent, the
temperature distribution forms a pattern opposite to that at 1400 LST in th
e daytime. It shows a maximum around the dip equator and a broad minimum at
the daytime crest region where the postsunset cooling also is faster and o
ccurs earlier than at the dip equator. This nighttime maximum appears to be
related to the signature of the midnight temperature maximum (MTM). Mass S
pectrometer Incoherent Scatter (MSIS) model temperatures, in general, are h
igher than the observed average temperatures for the summer season and in p
articular for the region around the dip equator around noon hours.