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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 ,
Franklin Aldás Open the ORCID record for Franklin Aldás [Opens in a new window]  and
Akimasa Yoshikawa
Ericson López
Affiliation:
Observatorio Astronómico de Quito, Escuela Politécnica Nacional, Quito, Ecuador email: [email protected]
Franklin Aldás
Affiliation:
Observatorio Astronómico de Quito, Escuela Politécnica Nacional, Quito, Ecuador email: [email protected]
Akimasa Yoshikawa
Affiliation:
International Center for Space Weather Science and Education, Kyushu University, Japan email: [email protected]
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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.

Keywords

Equatorial Electrojetmagnetic fielddata analysis
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S335: Space Weather of the Heliosphere: Processes and Forecasts , July 2017 , pp. 125 - 127
Copyright
Copyright © International Astronomical Union 2018 

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