Lunar Tides in the Equatorial Electrojet and in the Ionosphere over the Magnetic Equator

Physics

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Scientific paper

AN abnormally large value of the solar daily range of the horizontal magnetic intensity, H, found at stations within a few degrees from the magnetic equator has been ascribed due to eastward electric currents flowing in the lower ionosphere during the daylight hours and known as equatorial electrojet1. A longitudinal effect in the strength of the electro jet with a maximum in the American zone has been shown by Rastogi2.

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