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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37 citations as recorded by crossref.
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- Causes responsible for intense and severe storms during the declining phase of Solar Cycle 24 K. Patel et al. 10.1007/s12036-018-9569-7
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- Ionospheric F-region response to geomagnetic disturbances A. Danilov 10.1016/j.asr.2013.04.019
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Latest update: 24 Apr 2025
