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A wave equation describing the generation of field-aligned current in the magnetosphere

Abstract

A wave equation describing the generation of field-aligned current (FAC) in the magnetosphere is derived. The equation has four source terms. The first and second terms represent the effects of inhomogeneous Alfvén speed (VA) and curvilinear magnetic field line, respectively. The perpendicular perturbation inertial current produces the perturbation FAC via these effects. Around the magnetic equator in the region of dipolar magnetic field where VA is inversely proportional to the power of the radial distance from the Earth’s center, the first and second terms have magnitudes of the same order and their signs are identical. The first term dominates over the second one around the region where the gradient of VA is sharp and vice versa around the position where the stretched field line intersects the magnetic equator. The third and fourth terms are related to the diamagnetic current. When the unperturbed magnetic pressure has an inhomogeneous distribution, the perpendicular diamagnetic current due to the perturbation of the plasma pressure yields the perturbation FAC (third term). When the perpendicular diamagnetic current flows in the unperturbed state, the perturbations of the magnetic and plasma pressures also bring about the perturbation FAC (fourth term). In the case of β 1, the third and fourth terms have magnitudes of the same order. If the disturbance bears a diamagnetic property, this would be especially the case. However, if the disturbance propagates perpendicularly to the ambient magnetic field, the perturbation FAC would be little generated by the fourth term.

References

  • Dungey, J. W., Hydromagnetic waves, in Physics of Geomagnetic Phenomena, edited by S. Matsushita and W. H. Campbell, pp. 913–934, Academic Press, New York, 1968.

    Google Scholar 

  • Hasegawa, A. and T. Sato, Generation of field aligned current during sub-storm, in Dynamics of the Magnetosphere, edited by S.-I. Akasofu, pp. 529–542, D. Reidel, Hingham, Mass., 1979.

    Chapter  Google Scholar 

  • Itonaga, M. and A. Yoshikawa, The excitation of shear Alfvén wave and the associated modulation of compressional wave in the inner magnetosphere, J. Geomag. Geoelectr., 48, 1451–1459, 1996.

    Article  Google Scholar 

  • Itonaga, M. and K. Yumoto, ULF waves and the ground magnetic field, J. Geophys. Res., 103, 9285–9291, 1998.

    Article  Google Scholar 

  • Lester, M., W. J. Hughes, and H. Jinger, Polarization pattern of Pi 2 magnetic pulsations and the substorm current wedge, J. Geophys. Res., 88, 7958–7966, 1983.

    Article  Google Scholar 

  • Ohtani, S., A. Miura, and T. Tamao, Coupling between Alfvén and slow magnetosonic waves in an inhomogeneous finite-β plasma—I. Coupled equations and physical mechanism, Planet. Space Sci., 37, 567–577, 1989.

    Article  Google Scholar 

  • Sato, T., Auroral physics, in Magnetospheric Plasma Physics, edited by A. Nishida, pp. 197–243, D. Reidel, Hingham, Mass., 1982.

    Chapter  Google Scholar 

  • Sato, T. and T. Iijima, Primary sources of large-scale Birkeland currents, Space Sci. Rev., 24, 347–366, 1979.

    Article  Google Scholar 

  • Southwood, D. J. and M. G. Kivelson, An approximate description of field-aligned currents in a planetary magnetic field, J. Geophys. Res., 96, 67–75, 1991.

    Article  Google Scholar 

  • Southwood, D. J. and M. A. Saunders, Curvature coupling of slow and Alfvén MHD waves in a magnetotail field configuration, Planet. Space Sci, 33, 127–134, 1985.

    Article  Google Scholar 

  • Stern, D., Geomagnetic Euler potentials, J. Geophys. Res., 72, 3995–4005, 1967.

    Article  Google Scholar 

  • Tanaka, T., Generation mechanisms for magnetosphere-ionosphere current systems deduced from a three-dimensional MHD simulation of the solar wind-magnetosphere-ionosphere coupling processes, J. Geophys. Res., 100, 12,057–12,074, 1995.

    Article  Google Scholar 

  • Vasyliunas, V. M., Fundamentals of current description, in Magnetospheric Currents, edited by T. A. Potemra, pp. 63–66, AGU, Washington, D.C., 1984.

    Chapter  Google Scholar 

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Correspondence to Masahiro Itonaga.

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Itonaga, M., Yoshikawa, A. & Fujita, S. A wave equation describing the generation of field-aligned current in the magnetosphere. Earth Planet Sp 52, 503–507 (2000). https://doi.org/10.1186/BF03351654

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