- Article
- Published:
North-south asymmetry of the substorm intensity depending on the IMF B Y -component
Earth, Planets and Space volume 54, pages 955–961 (2002)
Abstract
The dependence of maximum variations of H-component negative bays at magnetic conjugate stations on a sign of the IMF B Y -component during the substorms of small and moderate intensity with |ΔH|max < 750 nT developed at B Z < 0 and |B Z / B Y | < 1 has been studied. By data from Kotzebue (Φ = 64.5°; Λ = 249.7°) and Macquarie Isl. (Φ = −64.5°; Λ = 247.8°) observatories in the eastern hemisphere and Leirvogur (Φ = 65.3°; Λ = 68.2°) and Syowa (Φ = −66.1°; Λ = 71.0°) stations in the western hemisphere it is shown that at B Y < 0 the absolute values of negative bays |ΔH|max are greater in the southern hemisphere and at B Y > 0, on the contrary, in the northern hemisphere.
References
Forbes, M. and M. Harel, Magnetosphere-ionosphere coupling: an experiment in interactive modeling, J. Geophys. Res., 94, 2631, 1989.
Harel, M. R., R. A. Wolf, P. H. Reif, R. W. Spiro, W. J. Burke, F. J. Rich, and M. Smiddy, Quantitative simulation of magnetospheric substorm, 1, Model logic and overview, J. Geophys. Res., 86, 2217, 1981.
Heppner, J. P., Polar cap electric field distributions related to the interplanetary magnetic field direction, J. Geophys. Res., 77, 4877, 1972.
Heppner, J. P. and N. C. Maynard, Empirical high-latitude electric field models, J. Geophys. Res., 92, 4467, 1987.
Iijima, T., R. Fujii, T. A. Potemra, and N. A. Saflekos, Field-aligned currents in the south polar cusp and their relationship to the interplanetary magnetic field, J. Geophys. Res., 83, 5595, 1978.
Knipp, D. J., A. D. Richmond, G. Crowley, O. de la Beaujardiere, D. S. Evans, and H. W. Kroehl, Ionospheric convection response to changing IMF direction, Geophys. Res. Lett., 18, 721, 1991.
Leontyev, S. V. and W. B. Lyatsky, Electric field and currents connected with Y-component of interplanetary magnetic field, Planet. Space Sci., 22, 811, 1974.
Lu, G., et al., Interhemispheric asymmetry of the high-latitude ionospheric convection pattern, J. Geophys. Res., 99, 6491, 1994.
Murayama, T. and K. Hakamada, Effects of solar wind parameters on the development of magnetospheric substorms, Planet. Space Sci., 23, 75, 1975.
Ohtani, S., et al., Four large-scale field-aligned current systems in the daiside high-latitude region, J. Geophys. Res., 100, 137, 1995.
Osaki, H., K. Yumoto, K. Fukao, K. Shiokowa, F. W. Menk, B. J. Fraser, and the 210° MM Magnetic observation group, Characteristics of low-latitude Pi2 pulsations along the 210° Magnetic meridian, J. Geomag. Geoelectr., 48, 1421, 1996.
Rich, F. J. and Y. Kamide, Electric fields and ionospheric currents derived from model field-aligned currents at high latitudes, J. Geophys. Res., 88, 271, 1983.
Velichko, V. A., R. N. Boroyev, and M. G. Gelberg, Azimuth asymmetry of regions of field-aligned currents inflowing and outflowing from the ionosphere in the substorm current wedge, in Physics of Auroral Phenomena, Proc. XXIV Annual Seminar, PGI-01-01-110, 37–40, Apatity, 2001.
Yumoto, K., and the 210° MM Magnetic Observation Group, The STEP 210° magnetic meridian network project, J. Geomag. Geoelectr., 48, 1297, 1996.
Zakharov, V. E. and M. I. Pudovkin, Electrodynamic coupling between ionospheric convection patterns in the northern and southern hemispheres, Ann. Geophysicae, 14, 419, 1996.
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Velichko, V.A., Boroyev, R.N., Gelberg, M.G. et al. North-south asymmetry of the substorm intensity depending on the IMF B Y -component. Earth Planet Sp 54, 955–961 (2002). https://doi.org/10.1186/BF03352443
Received:
Revised:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.1186/BF03352443