Abstract
Ionospheric dynamo current system representing geomagnetic lunar variation on disturbed days is calculated. A characteristic current system L p is formed at high latitudes owing to conductivity enhancement in the auroral belt, which also influences the L currents at mid and low latitudes: the foci of mid-low latitude current vortices shift 4° toward high latitude. IMF B z and B y effects on mid-low latitude Sq are studied. Rapid variation of magnetospheric convection electric field caused by B z variation will penetrate into the inner magnetosphere and then map onto the ionosphere along geomagnetic field lines, producing a characteristic electric field and current system, which will move the Sq foci and produce a magnetic disturbance of a few nT on ground surface. IMF sector effect on mid-low latitude magnetic filed is examined by using data from Beijing and Gangzhou in China. 3–5 nT effect is recognized.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
Chapman, S., and Bartels, J., Geomagnetism (Clarendon Press, Oxford 1940).
Evans, J. V. (1978), A Note on Lunar Tides in the Ionosphere, J. Geophys. Res. 83, 1647–1652.
Forbes, J. M. (1982), Atmospheric Tides, 2. The Solar and Lunar Semidiurnal Components, J. Geophys. Res. 87, 5241–5252.
Friis-Christensen, E., Polar cap current system, In Magnetospheric Currents (ed. Potemra, T. A.) (AGU, Washington, DC 1984) pp. 86–95.
Jaggi, R. K., and Wolf, R. A. (1973), Self-consistent Calculation of the Motion of a Sheet of Ions in the Magnetosphere, J. Geophys. Res. 78, 2852–2866.
Kendall, M. G., and Stuart, A., The Advanced Theory of Statistics, v. 3 (Charles Griffin, High Wycomb 1976).
Matsushita, S. (1966), Lunar Geomagnetic Variations, J. Geomag. Geoelectr. 18, 163–191.
Matsushita, S. (1969), Dynamo Currents, Winds and Electric Fields, Radio Sci. 4, 771–780.
Matsushita, S., and Xu, Wen-Yao (1981), IMF Behavior Estimated from Geomagnetic Data at South Pole, J. Geophys. Res. 86, 3628–3634.
Matsushita, S., and Xu, Wen-Yao (1982), Sq and L Currents in the Ionosphere, Ann. Geophys. 38, 295–305.
Matsushita, S., Tarpley, J. D., and Campbell, W. H. (1973), IMF Sector Structure Effect on the Quiet Geomagnetic Field, Radio Sci. 8, 1075–1090.
Tarpley, J. D. (1970), The Ionospheric Wind Dynamo—1. Lunar Tide, Planet. Space Sci. 18, 1075–1090.
Wu, L., Gendrin, R., Higel, B., and Berchem, J. (1981), Relationship Between the Solar Wind Electric Field and the Magnetospheric Convection Electric Field, Geophys. Res. Lett. 88, 1099–1102.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1989 Birkhäuser Verlag, Basel
About this chapter
Cite this chapter
Xu, WY. (1989). On Sq and L Current Systems in the Ionosphere. In: Campbell, W.H. (eds) Quiet Daily Geomagnetic Fields. Pageoph Topical Volumes. Birkhäuser Basel. https://doi.org/10.1007/978-3-0348-9280-3_13
Download citation
DOI: https://doi.org/10.1007/978-3-0348-9280-3_13
Publisher Name: Birkhäuser Basel
Print ISBN: 978-3-7643-2338-7
Online ISBN: 978-3-0348-9280-3
eBook Packages: Springer Book Archive