Articles | Volume 28, issue 9
https://doi.org/10.5194/angeo-28-1703-2010
© Author(s) 2010. 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-28-1703-2010
© Author(s) 2010. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
22 Sep 2010
Empirically modelled Pc3 activity based on solar wind parameters
B. Heilig
Tihany Geophysical Observatory, Eötvös Loránd Geophysical Institute, Hungary
S. Lotz
Hermanus Geomagnetic Observatory, Hermanus, South Africa
Dept. of Physics and Electronics, Rhodes University, Grahamstown, South Africa
J. Verő
Geodetic and Geophysical Research Institute, Hungarian Academy of Sciences, Sopron, Hungary
P. Sutcliffe
Hermanus Geomagnetic Observatory, Hermanus, South Africa
J. Reda
Belsk Geophysical Observatory, Polish Academy of Sciences, Poland
K. Pajunpää
Nurmijärvi Geophysical Observatory, Finnish Meteorological Institute, Finland
T. Raita
Sodankylä Geophysical Observatory, University of Oulu, Finland
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Cited
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- An initial ULF wave index derived from 2 years of Swarm observations C. Papadimitriou et al. https://doi.org/10.5194/angeo-36-287-2018
- From Foreshock 30-Second Waves to Magnetospheric Pc3 Waves L. Turc et al. https://doi.org/10.1007/s11214-025-01152-y
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