A Comparison of Equatorial Electrojet in Peru and East Brazil

R.G. Rastogi1, H. Chandra*, 1, Rahul Shah1, N.B. Trivedi2, S.L. Fontes3
1 Physical Research Laboratory, Ahmedabad 380009, India
2 National Institute of Space Research, Sao Jose dos Campos, Brazil
3 Observatario Nacional – ON/MCT, Rio de Janeiro, Brazil

Article Metrics

CrossRef Citations:
Total Statistics:

Full-Text HTML Views: 247
Abstract HTML Views: 672
PDF Downloads: 312
Total Views/Downloads: 1231
Unique Statistics:

Full-Text HTML Views: 155
Abstract HTML Views: 469
PDF Downloads: 228
Total Views/Downloads: 852

© 2013 Rastogiet al. ;

open-access license: This is an open access article distributed under the terms of the Creative Commons Attribution 4.0 International Public License (CC-BY 4.0), a copy of which is available at: This license permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.

* Address correspondence to this author at the Physical Research Laboratory, Navrangpura, Ahmedabad 380 009, India; Tel: +91-79-2631-4556; Fax:+91-79-2631-4900; E-mails:,


The paper describes the characteristics of the equatorial electrojet at Huancayo (HUA, 12.1oS, 75.3oW, inclination 1.5oN, declination 1.0oE) in western side of South America, where the geomagnetic field is aligned almost along the geographic meridian, and at Itinga (ITI, 4.3oS, 47.oW, inclination 1.4oN, declination 19.3oW) in eastern part of South America, where the geomagnetic field is aligned about 19o west of the geographic meridian; although the mean intensity of the magnetic field in the two regions are almost of the same order. Further comparisons are made of the current at Itinga and at Tatuoca (TTB, 1.2oS, 48.5oW, inclination 7.8o N, declination 18.7oW), a low latitude station in the same longitude sector. The daily range of horizontal component of the geomagnetic field, H, is shown to be almost 16% higher at HUA compared to that at ITI. The daily variation of the eastward field, Y, showed a strong minimum of -40 nT around 13-14 hr LT at ITI whereas very low values were observed at HUA with a positive peak of about 4 nT around 11- 12 hr LT. The vertical field, Z, showed abnormally large negative values of -70 nT at TTB around 13 hr LT. The day-today fluctuations of midday and midnight values of X field were positively correlated between HUA and ITI with a high correlation coefficient of 0.78 and 0.88 respectively. Values of Y field were also significantly positively correlated between HUA and ITI for midnight hours (0.72), while no correlation was observed for the midday hours. The midnight values of X field at HUA, ITI and TTB showed significant (0.90 or greater) correlation with Dst index. Correlation values of about 0.7 were observed between Dst and midday values of X at ITI and TTB and to a lesser degree (0.4) at HUA.

Keywords: Equatorial electrojet, equatorial E-region, geomagnetism.