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Investigating dynamic coupling in geospace through the combined use of modeling, simulations and data analysis

Wybrane pełne teksty z tego czasopisma
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Warianty tytułu
Języki publikacji
EN
Abstrakty
EN
Comprehensive understanding of the dynamics of the coupled solar wind-magnetosphere-ionosphere system is of utmost interest, both from the perspective of solar system astrophysics and geophysics research and from the perspective of space applications. The physical processes involved in the dynamical evolution of this complex coupled system are pertinent not only for the Sun-Earth connection, but also for major phenomena in other astrophysical systems. Furthermore, the conditions in geospace collectively termed space weather affect the ever increasing technological assets of mankind in space and therefore need to be understood, quantified and efficiently forecasted. The present collaborative paper communicates recent advances in geospace dynamic coupling research through modeling, simulations and data analysis and discusses future directions.
Czasopismo
Rocznik
Strony
141--157
Opis fizyczny
Bibliogr. 41 poz.
Twórcy
autor
autor
autor
autor
autor
  • National Observatory of Athens, Institute for Space Applications and Remote Sensing, Athens, Greece, daglis@space.noa.gr
Bibliografia
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  • Balasis, G., I.A. Daglis, P. Kapiris, M. Mandea, D. Vassiliadis, and K. Eftaxias (2006), From prestorm activity to magnetic storms: a transition described in terms of fractal dynamics, Ann. Geophys. 24, 3557-3567.
  • Belehaki, A., and I. Tsagouri (2002), On the occurrence of storm-induced nighttime ionization enhancements at ionospheric middle latitudes, J. Geophys. Res. 107, A8, 1209,
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  • Consolini, G., and P. De Michelis (2002), Fractal time statistics of AE-index burst waiting times: evidence of metastability, Nonlinear Proc. Geoph. 9, 419-423.
  • Daglis, I.A., and W.I. Axford (1996), Fast ionospheric response to enhanced activity in geospace: Ion feeding of the inner magnetotail, J. Geophys. Res. 101, A3, 5047-5065,
  • Daglis, I.A., J.U. Kozyra, Y. Kamide, D. Vassiliadis, A.S. Sharma, M.W. Liemohn, W.D. Gonzalez, B.T. Tsurutani, and G. Lu (2003), Intense space storms: Critical issues and open disputes, J. Geophys. Res. 108, A5, 1208,
  • Daglis, I.A., D. Delcourt, F.-A. Metallinou, and Y. Kamide (2004), Particle acceleration in the frame of the storm-substorm relation, IEEE Trans. Plasma Science 32, 4, 1449-1454,
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  • Ganushkina, N.Y., T.I. Pulkkinen, and T. Fritz (2005), Role of substorm-associated impulsive electric fields in the ring current development during storms, Ann. Geophys. 23, 579-591.
  • Ganushkina, N.Y., T.I. Pulkkinen, A. Milillo, and M. Liemohn (2006), Evolution of the proton ring current energy distribution during 21-25 April 2001 storm, J. Geophys. Res. 111, A11SO8,
  • Janhunen, P. (1996), GUMICS-3: a global ionosphere-magnetosphere coupling simulation with high ionospheric resolution, Proceedings of Environmental Modeling for Space-Based Applications, ESA SP-392.
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  • Kutiev, I., and P. Muhtarov (2001), Modeling of midlatitude F region response to geomagnetic activity, J. Geophys. Res. 106, A8, 15501-15509,
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  • Mandea, M., and G. Balasis (2006), The SGR 1806-20 magnetar signature on the Earth's magnetic field, Geophys. J. Int. 167, 586-591, (see report http://www.sciencemag.org/content/vol314/issue5798/twil.dtl).
  • Maynard, N.C., W.J. Burke, E.M. Basinska, G.M. Erickson, W.J. Hughes, H.J. Singer, A.G. Yahnin, D.A. Hardy, and F.S. Mozer (1996), Dynamics of the inner magnetosphere near times of substorm onsets, J. Geophys. Res. 101, A4, 7705-7736,
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  • Milillo, A., S. Orsini, and I.A. Daglis (2001), Empirical model of proton fluxes in the equatorial inner magnetosphere: Development, J. Geophys. Res. 106,A11, 25,713-25,729,
  • Muhtarov, P., I. Kutiev, and L. Cander (2002), Geomagnetically correlated autoregression model for short-term prediction of ionospheric parameters, Inverse Problems 18, 1, 49-65.
  • Palmroth, M., T.I. Pulkkinen, P. Janhunen, and C.-C. Wu (2003), Storm time energy transfer in global MHD simulation, J. Geophys. Res. 108, A1, 1048
  • Palmroth, M., P. Janhunen, T.I. Pulkkinen, and H.E.J. Koskinen (2004), Ionospheric energy input as a function of solar wind parameters: Global MHD simulation results, Ann. Geophys. 22, 549-566.
  • Palmroth, M., P. Janhunen, T.I. Pulkkinen, A. Aksnes, G. Lu, N. Ostgaard, J. Watermann, G.D. Reeves, and G.A. Germany (2005), Assessment of ionospheric Joule heating by GUMICS-4 MHD simulation, AMIE, and satellitebased statistics: Towards a synthesis, Ann. Geophys. 23, 2051-2068.
  • Palmroth, M., P. Janhunen, G.A. Germany, D. Lummerzheim, K. Liou, D.N. Baker, C. Barth, A.T. Weatherwax, and J. Watermann (2006a), Precipitation and total power consumption in the ionosphere: Global MHD simulation results compared with Polar and SNOE observations, Ann. Geophys. 24, 861-872.
  • Palmroth, M., T.V. Laitinen, and T.I. Pulkkinen (2006b), Magnetopause energy and mass transfer: Results from a global MHD simulation, Ann. Geophys. 24, 3467-3480.
  • Palmroth, M., P. Janhunen, and T.I. Pulkkinen (2006c), Hysteresis in solar wind power input to the magnetosphere, Geophys. Res. Lett. 33, L03107,
  • Proelss, G.W. (1995), Ionospheric F-region storms, Handbook of Atmospheric Electrodynamics, vol. II, 195-248, CRC Press.
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  • Sitnov, M.I., A.S. Sharma, K. Papadopoulos, and D. Vassiliadis (2001), Modeling substorm dynamics of the magnetosphere: From self-organization and selforganized criticality to nonequilibrium phase transitions, Phys. Rev. E 65, 016116
  • Stern, D.P. (1975), The motion of a proton in the equatorial magnetosphere, J. Geophys. Res. 80, 595-599,
  • Tsagouri, I., and A. Belehaki (2006), A new empirical model of middle latitude ionospheric response for space weather applications, Adv. Space Res. 37, 420-425,
  • Tsagouri, I., and A. Belehaki (2008), An upgrade of the solar wind driven empirical model for the middle latitude ionospheric storm-time response, J. Atmos. Sol.-Terr. Phys. submitted.
  • Tsagouri, I., A. Belehaki, G. Moraitis, and H. Mavromihalaki (2000), Positive and negative ionospheric disturbances at middle latitudes during geomagnetic storms, Geophys. Res. Lett. 27, 21, 3579-3582,
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  • Volland, H. (1973), A semi-empirical model of large-scale magnetospheric electric field, J. Geophys. Res. 78, 171-180,
Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-article-BSL8-0025-0031
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