Daily Sq variation in the earth's magnetic field is known to be due to ionospheric electronic currents. Direct measurements of these electronic currents have been made by using rocket‐borne magnetometers since the pioneering work was carried out by Singer et al. [1951]. Most of these measurements have been carried out at or near the geomagnetic equator where the intense equatorial electrojet flows eastward with a relatively narrow band. The magnetic field changes measured by rocket‐borne magnetometers have been large in the equatorial latitudes, so that it has been possible to determine the vertical profiles of the current density from the slope of the field changes [Maynardand Cahill, 1965; Davis et al., 1967; Maynard, 1967; Sastry, 1968; Shuman, 1970]. Their results show that the maximum current density is typically found between 95‐ and 110‐km altitude and that there exists another current layer, the center of which is situated between 120 and 140 km.