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Variability of Quiet-Time Magnetic Field Intensity Reconstructed from Spherical Harmonic Coefficients Over Asian-Sub Region
Subject area: Science,Engineering and Technology · Area of research: Space and Atmospheric Physics
Abstract
The study used the quiet-time geomagnetic field records for the three orthogonal components (H, D and Z) during period of low solar activity year 2017. The quiet field records are uniquely separated into external and internal contributions using the spherical harmonic analysis (SHA) technique. The result shows that the intensity of the external (MSqHext), internal (MSqHint), and sum of the quiet field (MSqHTot), equator-ward of the Sq focus are bounded by daytime eastward current which decreases away from the equator and those pole-ward of the Sq focus are bounded by westward current which seems to increases with increasing latitudes. At low latitudes, there was a significant intrusion of the opposite hemisphere summertime external Sq current system into the wintertime hemisphere at pre-noon hours. The (MSqDext), amplitude consistently appeared stronger (weaker) in summer (winter) months reflecting marked effect of ionospheric conductivity caused by solar ionizing flux. The exceptionally large MSqZext, amplitude at KNY is associated with the reduced and slight phase shift of MSqHext, amplitude at KNY latitude. The result further revealed that the internal Sq focal latitude is consistently more pole-ward that their corresponding external Sq focus which may possibly reflect electromagnetic induction effect.
Keywords
Ionosphere, Sq current, magnetic field
References
[1] Abbas M, Abidin ZZ, Jusoh MH, Bolaji OS, Yoshikawa A. Features of horizontal magnetic field intensity over northern island of Malaysia. Indian Journal of Physics. 2019 , Oct; 93 (10):1247-57.
[2] Pedatella NM, Forbes JM, Richmond AD. Seasonal and longitudinal variations of the solar quiet (Sq) current system during solar minimum determined by CHAMP satellite magnetic field observations. Journal of Geophysical Research: Space Physics. 2011 Apr;116(A4).
[3] Schuster, A. (1907). The diurnal variation of terrestrial magnetism. Proc. R. Soc. Lond. A, 80(535), 80-82.
[4] Xu, W.Y. and Li, W. D. Longitudinal effects and UT variations of the geomagnetic Sq Field. Chinese Journal of Geophysics, 37, 440-447. https:// doi.Org /10.1029/2002JA009287.
[5] Vichare, G., Rawat, R., Jadhav, M., & Sinha, A. K. (2017). Seasonal variation of the Sq focus position during 2006–2010. Advances in Space Research, 59(2), 542-556.
[6] Yamazaki Y, Maute A. Sq and EEJ—a review on the daily variation of the geomagnetic field caused by ionospheric dynamo currents. Space Science Reviews. 2017 Mar;206(1):299-405.
[7] Campbell WH. Introduction to geomagnetic fields. Cambridge University Press; 2003 Apr 10.
[8] Liu, Xiaocan, Peng Han, Katsumi Hattori, Huaran Chen, Junjie Chen, Liguo Jiao, Jiyao Tu, Yu Lei, and Junhao Zhao. "Seasonal variations of Sq current system in different longitudinal sectors and solar activities." Journal of Geophysical Research: Space Physics 129, no. 1 (2024): e2023JA031956.
[9] Liu, Xiaocan, Peng Han, Katsumi Hattori, Huaran Chen, Chie Yoshino, Xudong Zhao, Liguo Jiao, Xinxin Ma, and Yu Lei. "Seasonal variation characteristics of geomagnetic Sq external and internal equivalent current systems in East Asia and Oceania regions." Journal of Geophysical Research: Space Physics 126, no. 3 (2021): e2021JA029113.
[10] Campbell, W. H., & Schiffmacher, E. R. (1987). Quiet ionospheric currents and earth conductivity profile computed from quiet-time geomagnetic field changes in the region of Australia. Australian journal of physics
[11] Campbell, W. H. (2003). Introduction to geomagnetic fields: Cambridge University Press.
[12] Matsushita, S., & Maeda, H. (1965). On the geomagnetic solar quiet daily variation field during the IGY. Journal of Geophysical Research, 70(11), 2535-2558.
[13] Campbell WH, Schiffmacher ER. Upper mantle electr
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How to cite this paper
@article{1708442,
author = {Mustapha Abbas, Mohammed Bello Kaoje, Mukhtar Mohammed, Mukhtar Ibrahim Furfuri, Aminu Yusuf Koko; Aminu Muhammad},
title = {Variability of Quiet-Time Magnetic Field Intensity Reconstructed from Spherical Harmonic Coefficients Over Asian-Sub Region},
journal = {Iconic Research And Engineering Journals},
year = {2025},
volume = {8},
number = {11},
pages = {1819-1827},
issn = {2456-8880},
url = {https://www.irejournals.com/formatedpaper/1708442.pdf},
abstract = {The study used the quiet-time geomagnetic field records for the three orthogonal components (H, D and Z) during period of low solar activity year 2017. The quiet field records are uniquely separated into external and internal contributions using the spherical harmonic analysis (SHA) technique. The result shows that the intensity of the external (MSqHext), internal (MSqHint), and sum of the quiet field (MSqHTot), equator-ward of the Sq focus are bounded by daytime eastward current which decreases away from the equator and those pole-ward of the Sq focus are bounded by westward current which seems to increases with increasing latitudes. At low latitudes, there was a significant intrusion of the opposite hemisphere summertime external Sq current system into the wintertime hemisphere at pre-noon hours. The (MSqDext), amplitude consistently appeared stronger (weaker) in summer (winter) months reflecting marked effect of ionospheric conductivity caused by solar ionizing flux. The exceptionally large MSqZext, amplitude at KNY is associated with the reduced and slight phase shift of MSqHext, amplitude at KNY latitude. The result further revealed that the internal Sq focal latitude is consistently more pole-ward that their corresponding external Sq focus which may possibly reflect electromagnetic induction effect.},
keywords = {Ionosphere, Sq current, magnetic field},
month = {May},
}