Abstract

Abstract. It has been known for many decades that the lunar tidal influence in the equatorial electrojet (EEJ) is noticeably enhanced during Northern Hemisphere winters. Recent literature has discussed the role of stratospheric sudden warming (SSW) events behind the enhancement of lunar tides and the findings suggest a positive correlation between the lunar tidal amplitude and lower stratospheric parameters (zonal mean air temperature and zonal mean zonal wind) during SSW events. The positive correlation raises the question whether an inverse approach could also be developed which makes it possible to deduce the occurrence of SSW events before their direct observations (before 1952) from the amplitude of the lunar tides. This study presents an analysis technique based on the phase of the semi-monthly lunar tide to determine the lunar tidal modulation of the EEJ. A statistical approach using the superposed epoch analysis is also carried out to formulate a relation between the EEJ tidal amplitude and lower stratospheric parameters. Using these results, we have estimated a threshold value for the tidal wave power that could be used to identify years with SSW events from magnetic field observations.

Highlights

  • The equatorial electrojet (EEJ) is a narrow band of intense electric current flowing in the eastward direction above the magnetic dip equator in the daytime E region of the ionosphere

  • We provide a statistical assessment of the relation between stratospheric sudden warming (SSW) parameters and lunar tidal amplitude and make predictions of SSW events derived from lunar tides in magnetic data

  • We have used the magnetic field data of the Huancayo observatory to determine the modulation of the equatorial electrojet (EEJ) by the lunar tide

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Summary

Introduction

The equatorial electrojet (EEJ) is a narrow band of intense electric current flowing in the eastward direction above the magnetic dip equator in the daytime E region of the ionosphere. Bartels and Johnston (1940) carried out the initial study of the lunar influence on the EEJ and they reported the existence of “big L” days between the months November to March at Huancayo in Peru. During these days they observed that the lunar daily variations in the horizontal component of the magnetic field get considerably enhanced compared to normal days. Lühr et al (2012) presented a comprehensive overview of lunar tides in the EEJ using the data from the CHAMP satellite All of these studies confirmed the enhanced tidal amplitudes around the December solstice

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