Relation between the ring current and the tail current during magnetic storms

V. V. Kalegaev (1) , N. Y. Ganushkina (2) , T. I. Pulkkinen (2) , M. V. Kubyshkina (3) , H. J. Singer (4) , C. T. Russell (5)

1 SINP - D.V. Skobeltsyn Institute of Nuclear Physics
2 Geophysical Research Division [Helsinki]
3 Institute of Physics
4 NOAA Space Environment Center
5 IGPP - Institute of Geophysics and Planetary Physics [Los Angeles]

We study the dynamics of the magnetospheric large-scale current systems during storms by using three different magnetospheric magnetic field models: the paraboloid, event-oriented, and Tsyganenko T01 models. We have modelled two storm events, one moderate storm on 25-26 June 1998, when D_st reached -120nT and one intense storm on 21-23 October 1999, when D_st dropped to -250nT. We compare the observed magnetic field from GOES 8, GOES 9, and GOES 10, Polar and Geotail satellites with the magnetic field given by the three models to estimate their reliability. All models demonstrated quite good agreement with observations. Since it is difficult to measure exactly the relative contributions from different current systems to the D_st index, we compute the contributions from ring, tail and magnetopause currents given by the three magnetic field models. We discuss the dependence of the obtained contributions to the D_st index in relation to the methods used in constructing the models. All models show a significant tail current contribution to the D_st index, comparable to the ring current contribution during moderate storms. The ring current becomes the major D_st source during intense storms.

Domaines: Océan, Atmosphère; Sciences de la Terre

V. V. Kalegaev, N. Y. Ganushkina, T. I. Pulkkinen, M. V. Kubyshkina, H. J. Singer, et al.. Relation between the ring current and the tail current during magnetic storms. Annales Geophysicae, 2005, 23 (2), pp.523-533. ⟨hal-00317557⟩