Articles | Volume 35, issue 1
https://doi.org/10.5194/angeo-35-147-2017
© Author(s) 2017. 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-35-147-2017
© Author(s) 2017. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
Understanding the variability of magnetic storms caused by ICMEs
Remi Benacquista
CORRESPONDING AUTHOR
Departement environnement spatial, ONERA , Toulouse, France
Sandrine Rochel
Departement environnement spatial, ONERA , Toulouse, France
Guy Rolland
CNES, The French Space Agency, Toulouse, France
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P. M. E. Décréau, S. Aoutou, A. Denazelle, I. Galkina, J.-L. Rauch, X. Vallières, P. Canu, S. Rochel Grimald, F. El-Lemdani Mazouz, and F. Darrouzet
Ann. Geophys., 33, 1285–1300, https://doi.org/10.5194/angeo-33-1285-2015, https://doi.org/10.5194/angeo-33-1285-2015, 2015
Short summary
Short summary
We present here cases of wide banded Non Thermal Continuum (NTC) observed from the multi-point Cluster observatory. We point out that a large portion of the plasmasphere boundary layer, covering magnetic latitudes from 0 to above 30°, is radiating these radio waves. The radiation is confined inside multiple beams of small cone angles. We show how the spectral signature evolves, from integer harmonics of the electron gyrofrequency, when the observatory moves away from their sources.
H. Breuillard, O. Agapitov, A. Artemyev, E. A. Kronberg, S. E. Haaland, P. W. Daly, V. V. Krasnoselskikh, D. Boscher, S. Bourdarie, Y. Zaliznyak, and G. Rolland
Ann. Geophys., 33, 583–597, https://doi.org/10.5194/angeo-33-583-2015, https://doi.org/10.5194/angeo-33-583-2015, 2015
H. Breuillard, O. Agapitov, A. Artemyev, V. Krasnoselskikh, O. Le Contel, C. M. Cully, V. Angelopoulos, Y. Zaliznyak, and G. Rolland
Ann. Geophys., 32, 1477–1485, https://doi.org/10.5194/angeo-32-1477-2014, https://doi.org/10.5194/angeo-32-1477-2014, 2014
P. M. E. Décréau, S. Kougblénou, G. Lointier, J.-L. Rauch, J.-G. Trotignon, X. Vallières, P. Canu, S. Rochel Grimald, F. El-Lemdani Mazouz, and F. Darrouzet
Ann. Geophys., 31, 2097–2121, https://doi.org/10.5194/angeo-31-2097-2013, https://doi.org/10.5194/angeo-31-2097-2013, 2013
H. Breuillard, Y. Zaliznyak, O. Agapitov, A. Artemyev, V. Krasnoselskikh, and G. Rolland
Ann. Geophys., 31, 1429–1435, https://doi.org/10.5194/angeo-31-1429-2013, https://doi.org/10.5194/angeo-31-1429-2013, 2013
Short summary
The Earth's magnetic field creates a magnetic bulk all around it called the magnetosphere. This bulk a priori protects us from the particles coming from the sun but sometimes undergoes violent events such as interplanetary coronal mass ejections. These cause the entry of particles into the magnetosphere, which can be harmful for satellites. In this paper, we performed a statistical study to characterize the interplanetary coronal mass ejections and their ability to disturb the magnetosphere.
The Earth's magnetic field creates a magnetic bulk all around it called the magnetosphere. This...