Combining the long series of the simultaneous data of the horizontal c
omponent of the geomagnetic field (H) at the equatorial station, Triva
ndrum and at the low-latitude station, it has been shown for the first
time that the disturbance daily variation of the equatorial electroje
t current has a very clear anti-so shape with a minimum around noon, D
isturbance atmospheric dynamo seems to be a plausible explanation, but
some systematic magnetospheric processes related to local solar time
may also be effective sources for the phenomenon.