Equatorial electrojet studies from rocket and ground measurements

Combining the data of in-situ measurements of ionospheric current, J(m) by rocket-borne instruments and the ground based geomagnetic H field close to the magnetic equator a linear relation has been found between the peak curr ent density Jm and the daily range of H, (R-H). This relationship has been used to convert long series of R-H data into J(m). Combining J(m) and the E -region peak electron density N-m, the electron velocity in the ionosphere, V-E has been calculated. It is shown that after all corrections are made o f the solar zenith angle variations, the ionospheric current as well as ele ctron drift in American and Indian sectors show strong equinoctial maxima, the mean values of both the parameters are larger at American than in India n sector. The solar cycle variation of the electrojet current is primarily due to the variations of NmE, and not due to the variations of electric fie ld. The diurnal variation of the electric field with peak at 09-10 LT inter acting with noon peak of NmE making Delta H to peak at an hour earlier than noon. It is stressed to realise the importance of electric field in diurna l, seasonal and longitudinal variations of the equatorial electrojet curren t.