2014
DOI: 10.1186/bf03351632
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Daily variations of geomagnetic HD and Z-field at equatorial latitudes

Abstract: With the establishment of the new geomagnetic field observations in the Ocean Hemisphere Network Project (OHP) in Japan, minutes values of geomagnetic components, H D and Z have been recorded. The hourly mean values were used to study the variations in these three components at these new equatorial electrojet regions. The results of the analysis carried out revealed that the amplitude of d H has diurnal variation which peaks during the day at about local noon in all the three equatorial electrojet regions. Thi… Show more

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Cited by 23 publications
(15 citation statements)
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“…It is widely known that EEJ strength shows semiannual variation with a minimum during solstice periods (Tarpley, 1973;Okeke and Hamano, 2000;Chandra et al, 2000). This semiannual variation of EEJ strength is apparent irrespective of solar activity, with weaker EEJ strength during low solar activity periods.…”
Section: Eej/ceej Dependence Of E Sbmentioning
confidence: 99%
“…It is widely known that EEJ strength shows semiannual variation with a minimum during solstice periods (Tarpley, 1973;Okeke and Hamano, 2000;Chandra et al, 2000). This semiannual variation of EEJ strength is apparent irrespective of solar activity, with weaker EEJ strength during low solar activity periods.…”
Section: Eej/ceej Dependence Of E Sbmentioning
confidence: 99%
“…Even though the ratio Z / H is approximately 0.63 as Rastogi quoted from Doumouya et al (1998) and approximately 0.75 in Okeke and Hamano (2000), the fact remains that the pronounced variation was observed.…”
mentioning
confidence: 91%
“…It is not correct to rule out the possibility that the pronounced variation of Z observed in Kiritimati could be due to sea induction. See page 242 of Okeke and Hamano (2000) for detailed explanation.…”
mentioning
confidence: 99%
“…2 are shown the power spectra of simple differences and cleaned differences between DGL and PDN stations. The analysis of the simple differences power spectra clearly shows prominent peaks centered around diurnal components at the period of 8, 12 and 24 h. Although these variations are the most regular of the all geomagnetic changes, they tend not to repeat exactly itself but relevant differences could be noted from day to day (Okeke and Hamano, 2000). The dayto-day variability is thought to arise from the variations of the solar and geomagnetic activity.…”
Section: Figmentioning
confidence: 99%