Articles | Volume 33, issue 10
https://doi.org/10.5194/angeo-33-1271-2015
© Author(s) 2015. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
Special issue:
https://doi.org/10.5194/angeo-33-1271-2015
© Author(s) 2015. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
The relationship between plasmapause, solar wind and geomagnetic activity between 2007 and 2011
G. Verbanac
CORRESPONDING AUTHOR
Department of Geophysics, University of Zagreb, Zagreb, Croatia
V. Pierrard
Belgian Institute for Space Aeronomy (Space Physics and STCE), 3 Av. Circulaire, 1180 Brussels, Belgium
Université Catholique de Louvain, TECLIM, Earth and Life Institute, Place Louis Pasteur 3 bte L4.03.08, 1348 Louvain-La-Neuve, Belgium
M. Bandić
Preziosastr. 15a, 81927 München, Germany
F. Darrouzet
Belgian Institute for Space Aeronomy (Space Physics and STCE), 3 Av. Circulaire, 1180 Brussels, Belgium
J.-L. Rauch
Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), Orléans, France
P. Décréau
Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), Orléans, France
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Cited
30 citations as recorded by crossref.
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Latest update: 23 Nov 2024
Short summary
Using Cluster data, we develop plasmapause Lpp models parameterized by solar wind coupling functions and geomagnetic activity indices. We show that the Lpp response to the changes in the interplanetary conditions depends on the magnetic local time. The faster plasmapause response is observed in the post-midnight sector. At low activity, Lpp exhibits the largest values on the dayside. For enhanced activity, displacements towards larger values on the evening side are identified.
Using Cluster data, we develop plasmapause Lpp models parameterized by solar wind coupling...
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