Storm-substorm coupling during 16 Hours of Dst steadily at -150 nT

The Inner Magnetosphere: Physics and Modeling

Volumn , Issue , 2013, Pages 155-161

  Pulkkinen, Tuija I ^b   Ganushkina, N Yu ^b   Donovan, E ^a   Li, X ^c   Reeves, G D ^d   Russell, C T ^e   Singer, H J ^f   Slavin, J A ^g  

^a UNIVERSITY OF CALGARY   (Canada)

^b FINNISH METEOROLOGICAL INSTITUTE   (Finland)

^c UNIVERSITY OF COLORADO   (United States)

^d LOS ALAMOS NATIONAL LABORATORY   (United States)

^e UNIVERSITY OF CALIFORNIA   (United States)

^f NOAA EARTH SYSTEM RESEARCH LABORATORY   (United States)

^g NASA GODDARD SPACE FLIGHT CENTER   (United States)

Author keywords

Magnetospheric physics Simulation methods

Indexed keywords

BUDGET CONTROL; IONOSPHERE; SOLAR WIND; STORMS; STRUCTURAL DYNAMICS; WIND EFFECTS;

ENERGY BUDGETS; INNER MAGNETOSPHERE; MAGNETOSPHERE-IONOSPHERE COUPLING; MAGNETOSPHERIC PHYSICS; MAGNETOTAIL DYNAMICS; SOLAR WIND PRESSURE; TAIL CONFIGURATION; TAIL CURRENTS;

MAGNETOSPHERE;

EID: 33947502535     PISSN: None     EISSN: None     Source Type: Book    
DOI: 10.1029/155GM18     Document Type: Chapter

References (22)

1. Ahn, B.-H., S.-I. Akasofu, and Y. Kamide, The Joule heat production rate and the particle energy injection rate as a function of the geomagnetic indices AE and AL., J. Geophys. Res., 88, 6275, 1983.
2. Akasofu, S.-I., Energy coupling between the solar wind and the magnetosphere, Space Sci. Rev., 28, 121, 1981.
3. Baker, D.N., How to cope with space weather, Science, 297, 30 Aug 2002.
4. Boudouridis, A., E. Zesta, L.R. Lyons, P.C. Anderson, and D. Lummerzheim, Effect of solar wind pressure pulses on the size and strength of the auroral oval, J. Geophys. Res., 108, A4, 8012, doi:10.1029/2002JA009373, 2003.
5. Burton, R.K., R.L. McPherron, and C.T. Russell, An empirical relationship between interplanetary conditions and Dst, J. Geophys. Res., 80, 4204, 1975.
6. Chapman, S., and VC.A. Ferraro, A new theory of magnetic storms, Terr. Mag. Atmosph. Electr., 36, 77, 1931.
7. Ganushkina, N. Yu., Drivers of the inner magnetosphere, this volume.
8. Häkkinen, L.VT, T.I. Pulkkinen, R.J. Pirjola, H. Nevanlinna, E.I. Tanskanen, and N.E. Turner, Seasonal and diurnal variation of geomagnetic activity: revised Dst vs. external drivers, J. Geophys. Res., 108, A2, 1060, doi: 10.1029/2002JA009428, 2003.
9. Le, G., C.T. Russell, and K. Takahashi, Morphology of the ring current derived from magnetic field observations, Ann. Geophys, in press, 2004.
10. Lu, G., et al. Global energy deposition during the January 1997 magnetic cloud event, J. Geophys. Res., 103, 11685, 1998.
11. O'Brien, T.P., and R.L. McPherron, An empirical phase space analysis of ring current dynamics: Solar wind control of injection and decay, J. Geophys. Res., 105, 7707, 2000.
12. Østgaard, N.R., R. Vondrak, J.W. Gjerloev, and G.A. Germany, A relation between the energy deposition by electron precipitation and geomagnetic indices during substorms, J. Geophys. Res., 107(A9), SMP 16, DOI 10.1029/2001JA002003, 2002.
13. Pulkkinen, T.I., N.Yu. Ganushkina, VF. Bashkirov, D.N. Baker, J.F. Fennell, J. Roeder, T.A. Fritz, M. Grande, B. Kellett, and G. Kettmann, Ring current enhancement due to substormassociated inductive electric fields, in: Proceedings of the Fifth International Conference on Substorms, ESA SP-443, p. 451-454, 2000.
14. Pulkkinen, T.I., H.E.J. Koskinen, K.E.J. Huttunen, K. Kauristie, E.I. Tanskanen, M. Palmroth, G.D. Reeves, Effects of magnetic storms on substorm evolution, Sixth International Conference on Substorms, edited by R.M. Winglee, University of Washington, Seattle, 2002, pp. 464-471.
15. Reeves, G.D., M.G. Henderson, R.M. Skoug, M.F. Thomsen, J.E. Borovsky, H.O. Funsten, P. C:son Brandt, D.J. Mitchell, J.-M. Jahn, C.J. Pollock, D.J. McComas, and S.B. Mende, IMAGE, POLAR, and geosynchronous observations of substorm and ring current ion injection, AGU Monograph on the Storm-Substorm Relationship, in press, 2002.
16. Sergeev, VA., T.I. Pulkkinen, and R.J. Pellinen, Steady magnetospheric convection: A review of recent results, Space Sci. Rev., 75, 551, 1996.
17. Shue, J.-H., P. Song, C.T. Russell, J.T. Steinberg, J.K. Chao, G. Zastenker, O.L. Vaisberg, S. Kokubun, H.J. Singer, T.R. Detman, and H. Kawano, Magnetopause location under extreme J. Geophys. Res., 103, 17691, 1998.
18. Tanskanen, E.I., T.I. Pulkkinen, H.E.J. Koskinen, Substorm energy budget near solar minimum and maximum: 1997 and 1999 compared, J. Geophys. Res., 107, A6, 10.1029/2001JA900153, 2002.
19. Temerin, M. and Li, X., A new model for the prediction of Dst on the basis of the solar wind, J. Geophys. Res., 107, A12, 1472, doi:10.1029/2001JA007532, 2002.
20. Tsurutani, B.T., and W.D. Gonzalez, The cause of high-intensity long-duration continuous AE activity (HILDCAAs): interplanetary Alfven wave trains, Planet. Space Sci., 35, 405, 1987.
21. Tsyganenko, N.A., Modeling the Earth's magnetospheric magnetic field confined within a realistic magnetopause, J. Geophys. Res., 100, 5599, 1995.
22. Turner, N.E., D.N. Baker, T.I. Pulkkinen, and R.L. McPherron, Evaluation of the tail current contribution to Dst, J. Geophys. Res., 105, 5431-5440, 2000.