Articles | Volume 23, issue 2
https://doi.org/10.5194/angeo-23-523-2005
© Author(s) 2005. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
https://doi.org/10.5194/angeo-23-523-2005
© Author(s) 2005. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
28 Feb 2005
Relation between the ring current and the tail current during magnetic storms
V. V. Kalegaev
Skobeltsyn Institute of Nuclear Physics, Moscow State University, Moscow 119992, Russia
N. Y. Ganushkina
Geophysical Research, Finnish Meteorological Institute, POBox 503, Helsinki, FIN-00101, Finland
T. I. Pulkkinen
Geophysical Research, Finnish Meteorological Institute, POBox 503, Helsinki, FIN-00101, Finland
M. V. Kubyshkina
Institute of Physics, University of St-Petersburg, St-Petersburg, 198904, Russia
H. J. Singer
H. J. Singer, NOAA Space Environment Center, Boulder, CO 80305–3328, USA
C. T. Russell
Institute of Geophysics and Planetary Physics, University of California, Los Angeles, CA 90095–1567, USA
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- Offsets in the geomagnetic indices of the magnetospheric ring current G. Makarov https://doi.org/10.12737/stp-73202103
- Evolvement of the Ring Current During a Magnetic Storm: TC‐2 Neutral Atom Imager Observations https://doi.org/10.1002/cjg2.1541
- Magnetic field at geosynchronous orbit during high‐speed stream‐driven storms: Connections to the solar wind, the plasma sheet, and the outer electron radiation belt J. Borovsky & M. Denton https://doi.org/10.1029/2009JA015116
- Impact of the solar wind dynamic pressure on the Region 2 field‐aligned currents S. Nakano et al. https://doi.org/10.1029/2008JA013674
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Latest update: 24 Jun 2026
