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Rodriguez, L.; Zhukov A.N.; Cid C.; Cerrato Y.; Saiz E.; Cremades H.; Dasso S.; Menvielle M.; Aran A.; Mandrini C.; Poedts S.; Schmieder B. "Three frontside full halo coronal mass ejections with a nontypical geomagnetic response" (2009) Space Weather. 7(6)
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Abstract:

[1] 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. Copyright 2009 by the American Geophysical Union.

Registro:

Documento: Artículo
Título:Three frontside full halo coronal mass ejections with a nontypical geomagnetic response
Autor:Rodriguez, L.; Zhukov A.N.; Cid C.; Cerrato Y.; Saiz E.; Cremades H.; Dasso S.; Menvielle M.; Aran A.; Mandrini C.; Poedts S.; Schmieder B.
Filiación:Solar-Terrestrial Center of Excellence, SIDC, Royal Observatory of Belgium, Avenue Circulaire 3, B-1180 Brussels, Belgium
Skobeltsyn Institute of Nuclear Physics, Moscow State University, Moscow, Russian Federation
Department of Physics, University of Alcala, Ctra. Nacional II, Km. 33,600, E-28871 Alcala de Henares, Spain
Facultad Regional Mendoza, Universidad Tecnológica Nacional, Rodriguez 273, 5502 Mendoza, Argentina
Instituto de Astronomiá y Fiśica del Espacio, CONICET, Universidad de Buenos Aires, 1428 Buenos Aires, Argentina
Departamento de Fiśica, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Buenos Aires, Argentina
Centre d'Etude des Environnements Terrestre et Planétaires, 10-12 Avenue de l'Europe, F-78140 Veĺizy-Villacoublay, France
Department of Astronomy and Meteorology, University of Barcelona, Marti i Franques 1, E-08028 Barcelona, Spain
Centre for Plasma Astrophysics, Catholic University Leuven, Celestijnenlaan 200 B, B-3001 Leuven, Belgium
Observatoire de Paris, 5 Place Jules Janssen, F-92195 Meudon, France
Año:2009
Volumen:7
Número:6
DOI: http://dx.doi.org/10.1029/2008SW000453
Título revista:Space Weather
Título revista abreviado:Space Weather
ISSN:15427390
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_15427390_v7_n6_p_Rodriguez

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Citas:

---------- APA ----------
Rodriguez, L., Zhukov A.N., Cid C., Cerrato Y., Saiz E., Cremades H., Dasso S.,..., Schmieder B. (2009) . Three frontside full halo coronal mass ejections with a nontypical geomagnetic response. Space Weather, 7(6).
http://dx.doi.org/10.1029/2008SW000453
---------- CHICAGO ----------
Rodriguez, L., Zhukov A.N., Cid C., Cerrato Y., Saiz E., Cremades H., et al. "Three frontside full halo coronal mass ejections with a nontypical geomagnetic response" . Space Weather 7, no. 6 (2009).
http://dx.doi.org/10.1029/2008SW000453
---------- MLA ----------
Rodriguez, L., Zhukov A.N., Cid C., Cerrato Y., Saiz E., Cremades H., et al. "Three frontside full halo coronal mass ejections with a nontypical geomagnetic response" . Space Weather, vol. 7, no. 6, 2009.
http://dx.doi.org/10.1029/2008SW000453
---------- VANCOUVER ----------
Rodriguez, L., Zhukov A.N., Cid C., Cerrato Y., Saiz E., Cremades H., et al. Three frontside full halo coronal mass ejections with a nontypical geomagnetic response. Space Weather. 2009;7(6).
http://dx.doi.org/10.1029/2008SW000453