New interpretation of magnetospheric energy circulation

Geophysical Research Letters

Volumn 33, Issue 7, 2006, Pages

  Pulkkinen, Tuija I ^a,b   Palmroth, M ^b   Tanskanen, E I ^b   Janhunen, P ^b,c   Koskinen, H E J ^b,c   Laitinen, T V ^b,c  

^a LOS ALAMOS NATIONAL LABORATORY   (United States)

^b FINNISH METEOROLOGICAL INSTITUTE   (Finland)

^c UNIVERSITY OF HELSINKI   (Finland)

Author keywords

[No Author keywords available]

Indexed keywords

ENERGY DISSIPATION; ENERGY TRANSFER; GEOPHYSICAL PROSPECTING; MAGNETIC PROPERTIES; SOLAR ENERGY;

MAGNETOSPHERIC ENERGY CIRCULATION; MAGNETOTAIL STABILITY; SOLAR WIND; SUBSTORM ENERGETICS; SUBSTORM GROWTH PHASE;

MAGNETOSPHERE;

ATMOSPHERIC CIRCULATION; ENERGY DISSIPATION; MAGNETOSPHERE; SOLAR WIND;

EID: 33646824564     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/2005GL025457     Document Type: Article

References (16)

1. Ahn, B.-H., S.-I. Akasofu, and Y. Kamide (1983), 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.
2. Akasofu, S.-I. (1964), The development of the auroral substorm, Planet. Space Sci., 12, 273.
3. Akasofu, S.-I. (1981), Energy coupling between the solar wind and the magnetosphere, Space Sci. Rev., 28, 121.
4. Axford, W. I, and C. O. Hines (1961), A unifying theory of high-latitude geophysical phenomena and geomagnetic storms, Can. J. Phys., 39, 1433.
5. Baker, D. N., T. I. Pulkkinen, V. Angelopoulos, W. Baumjohann, and R. L. McPherron (1996), The neutral line model of substorms: Past results and present view, J. Geophys. Res., 101, 12,975.
6. Bargatze, L. F., D. N. Baker, R. L. McPherron, and E. W. Hones Jr. (1985), Magnetospheric impulse response for many levels of geomagnetic activity, J. Geophys. Res., 90, 6387.
7. Dmitreva, N. P., V. A. Sergeev, and M. A. Shukhtina (2004), Average characteristics of the midtail plasma sheet in different dynamic regimes of the magnetosphere, Ann. Geophys., 22, 2107.
8. Dungey, J. R. (1961), Interplanetary magnetic field and the auroral zones, Phys. Rev. Lett., 6, 47.
9. Janhunen, P. (1996), GUMICS-3: A global ionosphere-magnetosphere coupling simulation with high ionospheric resolution, in Proceedings of Environmental Modelling for Space-Based Applications, Eur. Space Agency Spec. Publ., ESA-SP 392, 205.
10. Laitinen, T. V., T. I. Pulkkinen, M. Palmroth, P. Janhunen, and H. E. J. Koskinen (2005), The magnetotail reconnection region in a global MHD simulation, Ann. Geophys., 23, 3753.
11. Lopez, R. E., S. Hernandez, J. G. Lyon, and M. Wiltberger (2004), Solar wind density control of energy transfer to the magnetosphere, Geophys. Res. Lett., 31, L08804, doi:10.1029/2003GL018780.
12. Olsson, A., P. Janhunen, T. Karlsson, L. G. Blomberg, and N. Ivchenko (2004), Statistics of Joule heating in the auroral zone and polar cap using Astrid-2 satellite Poynting flux, Ann. Geophys., 22, 4133.
13. 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, doi:10.1029/2002JA009446.
14. 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.
15. Palmroth, M., P. Janhunen, and T. I. Pulkkinen (2006), Hysteresis in the solar wind power input into the magnetosphere, Geophys. Res. Lett., 33, L03107, doi:10.1029/2005GL025188.
16. Tanskanen, E. I., T. I. Pulkkinen, and H. E. J. Koskinen (2002), Substorm energy budget near solar minimum and maximum: 1997 and 1999 compared, J. Geophys. Res., 107(A6), 1086, doi:10.1029/2001JA900153, 2002.