Abstract
SPACE WEATHER,
VOL. 7,
S06003,
19 PP., 2009
doi:10.1029/2008SW000453
Three frontside full halo coronal mass ejections with a nontypical geomagnetic response
Solar-Terrestrial Center of Excellence, SIDC, Royal Observatory of Belgium, Brussels, Belgium
Solar-Terrestrial Center of Excellence, SIDC, Royal Observatory of Belgium, Brussels, Belgium
Skobeltsyn Institute of Nuclear Physics, Moscow State University, Moscow, Russia
Department of Physics, University of Alcala, Alcala de Henares, Spain
Department of Physics, University of Alcala, Alcala de Henares, Spain
Department of Physics, University of Alcala, Alcala de Henares, Spain
Facultad Regional Mendoza, Universidad Tecnológica Nacional, Mendoza, Argentina
Instituto de Astronomía y Física del Espacio, CONICET, Universidad de Buenos Aires, Buenos Aires, Argentina
Departamento de Física, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Buenos Aires, Argentina
Centre d'Etude des Environnements Terrestre et Planétaires, Vélizy-Villacoublay, France
Department of Astronomy and Meteorology, University of Barcelona, Barcelona, Spain
Instituto de Astronomía y Física del Espacio, CONICET, Universidad de Buenos Aires, Buenos Aires, Argentina
Centre for Plasma Astrophysics, Catholic University Leuven, Leuven, Belgium
Observatoire de Paris, Meudon, France
Forecasting potential geoeffectiveness of solar disturbances (in particular, of frontside full halo coronal mass ejections) is important for various practical purposes, e.g., for satellite operations, radio communications, global positioning system applications, power grid, and pipeline maintenance. We analyze three frontside full halo coronal mass ejections (CMEs) that occurred in the year 2000 (close to the activity maximum of solar cycle 23), together with associated solar and heliospheric phenomena as well as their impact on the Earth's magnetosphere. Even though all three were fast full halos (with plane of the sky speeds higher than 1100 km/s), the geomagnetic response was very different for each case. After analyzing the source regions of these halo CMEs, it was found that the halo associated with the strongest geomagnetic disturbance was the one that initiated farther away from disk center (source region at W66); while the other two CMEs originated closer to the central meridian but had weaker geomagnetic responses. Therefore, these three events do not fit into the general statistical trends that relate the location of the solar source and the corresponding geoeffectivity. We investigate possible causes of such a behavior. Nonradial direction of eruption, passage of the Earth through a leg of an interplanetary flux rope, and strong compression at the eastern flank of a propagating interplanetary CME during its interaction with the ambient solar wind are found to be important factors that have a direct influence on the resulting north-south interplanetary magnetic field (IMF) component and thus on the CME geoeffectiveness. We also find indications that interaction of two CMEs could help in producing a long-lasting southward IMF component. Finally, we are able to explain successfully the geomagnetic response using plasma and magnetic field in situ measurements at the L1 point. We discuss the implications of our results for operational space weather forecasting and stress the difficulties of making accurate predictions with the current knowledge and tools at hand.
Received 24 October 2008; accepted 17 March 2009; published 11 June 2009.
Citation: (2009), Three frontside full halo coronal mass ejections with a nontypical geomagnetic response, Space Weather, 7, S06003, doi:10.1029/2008SW000453.
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