Contributions to the ring current energy during geomagnetic storms

The purpose of this research was to study the complexity of the energization of the ring current during a geomagnetic storm, produced during southern Bz(IMF) by the injection of plasma sheet ions, accelerated by enhanced convective electric fields. This model assumes that the plasma sheet is continu...

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Autor principal: Van Zele, M.A
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: Kluwer Academic/Plenum Publishers 2002
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100 1 |a Van Zele, M.A. 
245 1 0 |a Contributions to the ring current energy during geomagnetic storms 
260 |b Kluwer Academic/Plenum Publishers  |c 2002 
270 1 0 |m Van Zele, M.A.; Instituto de geofisica Daniel Valenc, Depto. de Cs. Geologicas, FCEN UBA, Ciudad Universitaria Pab II, Buenos Aires C1428EHA, Argentina; email: avanzele@gl.fcen.uba.ar 
506 |2 openaire  |e Política editorial 
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504 |a Chen, M.W., Schulz, M., Lyons, L.R., Modeling of ring current formation and decay: A review (1997) Geophysical Monograph, 98, pp. 173-186. , AGU, USA 
504 |a Daglis, I., Thorne, R.M., Baumjohann, W., Orsini, S., The terrestrial ring current: Origin, formation, and decay (1999) Rev. Geophys, 37, pp. 407-438 
504 |a Dessler, A.J., Parker, E.N., Hydromagnetic theory of geomagnetic storms (1959) J. Geophys. Res, 64, pp. 2239-2252 
504 |a González, W.D., Tsurutani, B.T., González, A.L.C., Smith, E.J., Tang, F., Akasofu, S.-I., Solar wind magnetospheric coupling during intense magnetic storm (1978-1979) (1989) J. Geophys. Res, 94, pp. 8835-8851 
504 |a Kamide, Y., Baumjohann, W., Daglis, I.A., González, W.D., Grande, M., Joselyn, J.A., Mc Pherron R.L. Phillips, J.L., Tsurutani B.T. Vasyliunas, V.M., Current understanding of magnetic storms: Storm-Substorm relationship (1998) J. Geophys. Res, 103, pp. 17705-17728 
504 |a Kamide, Y., McPherron, R.L., González, W.D., Hamilton, D.C., Hudson, H.S., Joselyn, J.A., Kahler S.W. Lyons, L.R., Szuszczewicz, E., Magnetic storms: Current understanding and outstanding questions (1997) Geophysical Monograph, 98, pp. 1-19. , AGU, USA 
504 |a Mayaud, P.N., Deviation, meaning, and use of geomagnetic indices (1980) Geophysical Monograph, 22, pp. 115-129. , AGU, USA 
504 |a Parks, G.K., (1991) Physics of Space Plasma, an Introduction, , Addison-Wesley Publishing Company, Redwood City, U.S.A 
504 |a Sckopke, N., A general relation between the energy of trapped particles and the disturbance field near the Earth (1966) J. Geophys. Res, 71, pp. 3125-3130 
504 |a Spiro, R.W., Wolf, R.A., Electrodynamics of convection in the inner magnetosphere. Magnetospheric currents (1984) Geophysical Monograph, 28, pp. 247-259. , AGU, USA 
504 |a Smith, J.P., Thomsen, M.F., Borovsky, J.E., Collier, M., Solar wind density as a driver for the ring current in mild storms (1999) Geophys. Res. Lett, 26, pp. 1797-1800 
504 |a Terasawa, T., Fujimoto, M., Mukai, T., Shinohara, I., Saito, Y., Yamamoto, T., Machida, S., Lepping, R.P., Solar wind control of density and temperature in the near-Earth plasma sheet: WIND/geotail collaboration (1997) Geophys. Res. Lett, 24, pp. 935-938 
504 |a Thomsen, M.F., Borovsky, D.J., McComas, D.J., Collier, M.R., Variability of the ring current source population (1998) Geophys. Res. Lett, 25, pp. 3481-3484 
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504 |a Van Zele, M.A., Schneider, O., The equatorial ring current as a part of a coupled system (1999) Stud. Geophys. Geod, 43, pp. 284-288 
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504 |a Wygant, J., Rowland, D., Singer, H.J., Temerin, M., Mozer, F., Hudson, M.K., Experimental evidence on the role of the large spatial scale field in creating the ring current (1998) J. Geophys. Res, 103, pp. 29527-29544 
520 3 |a The purpose of this research was to study the complexity of the energization of the ring current during a geomagnetic storm, produced during southern Bz(IMF) by the injection of plasma sheet ions, accelerated by enhanced convective electric fields. This model assumes that the plasma sheet is continuously populated by H+ from the sun and the ionosphere, and sporadically by ionospheric O+, making the ring current a coupled system whose energy can hardly be expressed analytically. When Bz(IMF) turns north, the ring current becomes uncoupled, and the energy decays exponentially if the storm is weak, or can be expressed as a combination of exponentials during strong storms representing the quick decay of O+ and the slower decay of H+, as has been shown.  |l eng 
536 |a Detalles de la financiación: Universidad de Buenos Aires 
536 |a Detalles de la financiación: Facultad de Ciencias Físicas y Matemáticas 
536 |a Detalles de la financiación: Consejo Nacional de Investigaciones Científicas y Técnicas 
536 |a Detalles de la financiación: Acknowledgments: The author wishes to thank Consejo Nacional de Investigaciones Científicas y Técnicas (Argentina) and to Departamento de Ciencias Geológicas (Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires) for supporting the research. 
593 |a Instituto de geofisica Daniel Valenc, Depto. de Cs. Geologicas, FCEN UBA, Ciudad Universitaria Pab II, Buenos Aires C1428EHA, Argentina 
690 1 0 |a RING CURRENT 
690 1 0 |a SOLAR WIND-MAGNETOSPHERE COUPLING 
690 1 0 |a GEOMAGNETIC STORM 
690 1 0 |a MAGNETOSPHERE 
690 1 0 |a SOLAR WIND 
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