No CrossRef data available.
Article contents
Analysis of Magnetic Field Variations Produced by Equatorial Electro-Jets
Published online by Cambridge University Press: 24 July 2018
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
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
- 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
References
Rigoti, A., Chamalaun, N. B. & Padilha, A. L., 1999, Earth Planets Space, 51, 115–128CrossRefGoogle Scholar
You have
Access