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The equatorial electrojet (EEJ) is a narrow ribbon of current flowing eastward in the day time equatorial region of the Ionosphere. The abnormally large amplitude of variations in the horizontal components in equatorial geomagnetic observatories, as a result of EEJ, was noticed as early as 1920 from Huancayo geomagnetic observatory. Observations by radar, rockets, satellites and geomagnetic observatories are used to study EEJ.

Causes

The world-wide solar driven wind results in so-called Sq (solar-quite) current system in the E region of the Earth's ionosphere (100-130 Km altitude). Resulting from this current is an electrostatic field directed E-W (dawn-dusk) in the equatorial day side of ionosphere. At the magnetic dip equator, where the geomagnetic field is horizontal, this electric field results in an enhanced eastward current flows within ±3 degrees of the magnetic equator known as the equatorial electrojet.

Studies of EEJ from satellite & ground magnetic data

The EEJ phenomenon was first identified using geomagnetic data. The amplitude of the daily variation of the horizontal magnetic intensity (H) measured at a geomagnetic observatory near the dip-equator is 3-5 fold higher than that of data from other regions of Earth. A typical diurnal equatorial observatory data show a peak of strength ~80 nT at 12.00 LT, with respect to the night-time level. Egedal (1947) showed that the enhancement of quiet day solar daily variations in H (Sq(H)) lay within the 50 latitude centered on the dip equator . The mechanism that produced the abnormal current was proposed as a band of current about 300 km in width flowing over the dip equator.

EEJ studies from satellite data were initiated with the arrival of data from the POGO (Polar orbiting Geophysical Observatories) series of satellite (1967-1970). The characteristic signature of the EEJ ΔH field is a sharp negative V shaped curve attaining its minimum within 0.50 of the magnetic dip equator. The magnetic data from the satellite missions like Ørsted (1999 - present) and CHAMP (2000 - present) vastly improved our knowledge on EEJ.

References

Egedal , J. 1947. The magnetic diurnal variation of the horizontal force near the magnetic equator. Terr. Magn. Atmos. Electr. 52, 449 – 451
Equatorial Electrojet from Cooperative Institute for Research in Environmental Sciences, Colorado University
The Equatorial Electrojet By C. Agodi Onwumechili, Published 1997 CRC Press, ISBN 9056990691, http://books.google.com/books?id=kwCFPH4C3tEC

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-[[Image:eej_cm4.png|thumb|400px|A snap shot of the Earth’s magnetic field at 400 Km altitude  due to the day-time ionsopheric current systems at 6.00 Universal Time (UT).  The equatorial intensification of the magnetic field is due to EEJ. The map was generated by a geomagnetic field model.
+[[Image:eej_cm4.png|thumb|400px|A snap shot of the Earth’s magnetic field at 400 Km altitude  due to the day-time ionsopheric current systems. The equatorial intensification of the magnetic field is due to EEJ. EEJ peaks over India at this UT instance. The map was generated by a geomagnetic field model.
 .]]
 The '''equatorial electrojet''' ('''EEJ''') is a narrow ribbon of current flowing eastward in the day time equatorial region of the [[Ionosphere]]. The abnormally large amplitude of variations in the horizontal components in equatorial [[geomagnetic]] observatories, as a result of EEJ, was noticed as early as 1920 from [[Huancayo]] geomagnetic observatory. Observations by radar, rockets, satellites and geomagnetic observatories are used to study EEJ.