Climatology of the inter-hemispheric field-aligned currents system over the Nigeria ionosphere
書誌事項
- 公開日
- 2012-11
- 資源種別
- journal article
- 権利情報
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- https://www.elsevier.com/tdm/userlicense/1.0/
- DOI
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- 10.1016/j.jastp.2012.07.008
- 公開者
- Elsevier BV
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説明
Abstract Records of the declination ( D ) magnetic field data for the year 2009 from the Magnetic Data Acquisition System (MAGDAS) facilities at University of Ilorin were employed for this work. From the minutes value of the D-component, the deduced hourly values of the D-component ( S q ( QD )) were used to estimate its diurnal ( S q ( D )) values with the most five quietest days identified. The monthly mean ( MS q ( D )) of the most five quietest days and their seasonal ( SS q ( D )) variabilities were investigated. The inter-hemispheric field aligned currents (IHFACs) exhibit downward and upward inter-hemispheric field-aligned sheet current that appears as a pair at all local times of the S q ( D ), MS q ( D ), and SS q ( D ) variations. From these variabilities, the IHFACs were observed to flow from the winter to summer hemisphere during noon and dusk sector and flowing in opposite direction during the dawn sector. The S q ( D ) variability patterns that were observed in May, June, August September are gentle compared to the disturbed variabilities in January, February, March and November. The highest positive (∼1.7 arc-min) and negative (∼−2.7 arc min) MS q ( D ) maxima values were observed in August during the dawn and noon sectors respectively. These values indicated that the IHFACs flow in August is strongly southbound (positive) and northbound (negative) in the dawn and noon sectors respectively. Dusk-side IHFACs as can be observed by MAGDAS are weakly northbound in all the seasons. The direction of IHFACs does not flip at the equinoxes but in June and November and does not become largest at solstices but in August. The IHFACs was observed to exhibit longitudinal variability, which indicated that larger amplitude of winter-to-summer IHFACs is observed to be greater in June solstice (northbound/negative IHFACs) than in the December solstice (southbound/positive IHFACs) during the noon sector.
収録刊行物
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- Journal of Atmospheric and Solar-Terrestrial Physics
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Journal of Atmospheric and Solar-Terrestrial Physics 89 144-153, 2012-11
Elsevier BV
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詳細情報 詳細情報について
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- CRID
- 1360004232245208704
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- ISSN
- 13646826
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- 資料種別
- journal article
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- データソース種別
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- Crossref
- KAKEN
- OpenAIRE
