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Analysis of Magnetic Field Variations Produced by Equatorial Electro-Jets

Published online by Cambridge University Press:  24 July 2018

Ericson López
Affiliation:
Observatorio Astronómico de Quito, Escuela Politécnica Nacional, Quito, Ecuador email: ericsson.lopez@epn.edu.ec
Franklin Aldás
Affiliation:
Observatorio Astronómico de Quito, Escuela Politécnica Nacional, Quito, Ecuador email: franklin.aldas@epn.edu.ec
Akimasa Yoshikawa
Affiliation:
International Center for Space Weather Science and Education, Kyushu University, Japan email: yoshi@geo.kyushu-u.ac.jp
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Abstract

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The Equatorial Electrojet (EEJ) is a narrow band of electrons flowing from east to west at daytime at low latitudes. The electron current produces a magnetic field variation that can be measured at different latitudes. In this work, we have used the data analysis in order to quantify the solar and lunar contributions to those variations and study the morphology of the EEJ current.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2018 

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