Abstract

Yamazaki et al. (2009) reported two strong negative crochets during midday (solar flares on 8 June 2000, 3 July 2002), along the Circum-pan pacific magnetometers network (CPMN). The association of these with equatorial counter electrojet was doubted and suggestion was made to investigate the cause of these unique events. Present investigations were motivated by their paper. In this paper, detailed examination of geomagnetic data for the two events is made at all stations within 75°E (Indian) and 160°E (western Pacific) longitude sectors. Latitudinal variations of ΔH on 18 June 2000 showed negative gradient towards the dip equator suggesting a partial counter electrojet both in the Indian and CPMN sectors. A partial counter electrojet also existed from morning to 1300 LT in the western Pacific sector on 3 July 2002. There are two current sheets over the equatorial electrojet region, one at higher level flowing eastward associated with global Sq current system and another intense current layer at 107 km, flowing eastward during normal and westward during partial/full counter electrojet periods. Solar flares are likely to affect the electrojet current more strongly as a result of the absorption, in the lower E-region, of the shorter wavelength solar X-rays flare spectrum.

Highlights

  • IntroductionThe first ground survey of the geomagnetic horizontal field from a chain of fourteen stations in Peru by Giesecke (quoted by Chapman 1951) revealed that the daily range of H slowly increased from 7◦S geographic latitude to a peak at 13◦S (close to magnetic dip equator) by a factor of 2

  • 1.1 Equatorial Electrojet Current (EEJ)The first ground survey of the geomagnetic horizontal field from a chain of fourteen stations in Peru by Giesecke revealed that the daily range of H slowly increased from 7◦S geographic latitude to a peak at 13◦S by a factor of 2

  • The present analysis shows that on 18 June 2000 a partial counter electrojet was observed in both the Indian and Circum-pan pacific magnetometers network (CPMN) longitude sectors

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Summary

Introduction

The first ground survey of the geomagnetic horizontal field from a chain of fourteen stations in Peru by Giesecke (quoted by Chapman 1951) revealed that the daily range of H slowly increased from 7◦S geographic latitude to a peak at 13◦S (close to magnetic dip equator) by a factor of 2. This was explained by him as due to a narrow band of thin current sheet flowing eastward during the day time hours in the ionosphere (100 km) and named it Equatorial Electrojet (EEJ). The equatorial enhancement of Range H was observed later in Nigeria (Onwumechili, 1959), Peru (Forbush and Casaverde, 1961), India (Yacob and Khanna, 1963) and Tschad (Godivier and Copyright c The Society of Geomagnetism and Earth, Planetary and Space Sciences (SGEPSS); The Seismological Society of Japan; The Volcanological Society of Japan; The Geodetic Society of Japan; The Japanese Society for Planetary Sciences; TERRAPUB

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