Abstract
Fine structure of the lunar semimonthly tides in H at different U.T. hours is studied at a station under the influence of equatorial electrojet as well as at a station just outside the influence of the electrojet in the Indian region. It is noticed that the amplitude of the tide varies with solar time at the electrojet station and is complex at the non-electrojet station. Known differential vertical upward drift motion of charged particles in and outside the equatorial electrojet belt appear to be responsible for this phenomena. The maximum deviation in the instantaneous range in H occurs about one day later at Trivandrum than at Alibag.
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