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Rodriguez, L.; Masías-Meza, J.J.; Dasso, S.; Démoulin, P.; Zhukov, A.N.; Gulisano, A.M.; Mierla, M.; Kilpua, E.; West, M.; Lacatus, D.; Paraschiv, A.; Janvier, M. "Typical Profiles and Distributions of Plasma and Magnetic Field Parameters in Magnetic Clouds at 1 AU" (2016) Solar Physics. 291(7):2145-2163
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Abstract:

Magnetic clouds (MCs) are a subset of interplanetary coronal mass ejections (ICMEs). They are important because of their simple internal magnetic field configuration, which resembles a magnetic flux rope, and because they represent one of the most geoeffective types of solar transients. In this study, we analyze their internal structure using a superposed epoch method on 63 events observed at L1 by the Advance Composition Explorer (ACE), between 1998 and 2006. In this way, we obtain an average profile for each plasma and magnetic field parameter at each point of the cloud. Furthermore, we take a fixed time-window upstream and downstream from the MC to also sample the regions preceding the cloud and the wake trailing it. We then perform a detailed analysis of the internal characteristics of the clouds and their surrounding solar wind environments. We find that the parameters studied are compatible with log-normal distribution functions. The plasma β and the level of fluctuations in the magnetic field vector are the best parameters to define the boundaries of MCs. We find that one third of the events shows a peak in plasma density close to the trailing edge of the flux ropes. We provide several possible explanations for this result and investigate if the density peak is of a solar origin (e.g. erupting prominence material) or formed during the magnetic cloud travel from the Sun to 1 AU. The most plausible explanation is the compression due to a fast overtaking flow, coming from a coronal hole located to the east of the solar source region of the magnetic cloud. © 2016, Springer Science+Business Media Dordrecht.

Registro:

Documento: Artículo
Título:Typical Profiles and Distributions of Plasma and Magnetic Field Parameters in Magnetic Clouds at 1 AU
Autor:Rodriguez, L.; Masías-Meza, J.J.; Dasso, S.; Démoulin, P.; Zhukov, A.N.; Gulisano, A.M.; Mierla, M.; Kilpua, E.; West, M.; Lacatus, D.; Paraschiv, A.; Janvier, M.
Filiación:Solar–Terrestrial Center of Excellence, SIDC, Royal Observatory of Belgium, Av. Circulaire 3, Brussels, 1180, Belgium
Departamento de Física - IFIBA, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Buenos Aires, 1428, Argentina
Instituto de Astronomía y Física del Espacio (UBA-CONICET), Universidad de Buenos Aires, CC. 67, Suc. 28, Buenos Aires, 1428, Argentina
Departamento de Ciencias de la Atmósfera y los Océanos and Departamento de Física (FCEN-UBA), Universidad de Buenos Aires, Buenos Aires, 1428, Argentina
Observatoire de Paris, LESIA, UMR 8109 (CNRS), Meudon Principal Cedex, 92195, France
Skobeltsyn Institute of Nuclear Physics, Moscow State University, Moscow, 119992, Russian Federation
Instituto Antártico Argentino, Cerrito 1248, Buenos Aires, 1010, Argentina
Institute of Geodynamics of the Romanian Academy, Jean-Louis Calderon 19-21, Bucharest-37, 020032, Romania
Department of Physics, Division of Geophysics and Astronomy, University of Helsinki, Kumpula campus Gustaf Hällströmin katu 2a, Helsinki, 00560, Finland
School of Mathematical Sciences, Monash University, Clayton, VIC 3800, Australia
Institut d’Astrophysique Spatiale, UMR8617, Univ. Paris-Sud-CNRS, Université Paris-Saclay, Batiment 121, Orsay Cedex, 91405, France
Palabras clave:Coronal mass ejections, low coronal signatures, initiation and propagation; Interplanetary coronal mass ejections; Magnetic clouds; Space weather
Año:2016
Volumen:291
Número:7
Página de inicio:2145
Página de fin:2163
DOI: http://dx.doi.org/10.1007/s11207-016-0955-5
Título revista:Solar Physics
Título revista abreviado:Sol. Phys.
ISSN:00380938
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00380938_v291_n7_p2145_Rodriguez

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Citas:

---------- APA ----------
Rodriguez, L., Masías-Meza, J.J., Dasso, S., Démoulin, P., Zhukov, A.N., Gulisano, A.M., Mierla, M.,..., Janvier, M. (2016) . Typical Profiles and Distributions of Plasma and Magnetic Field Parameters in Magnetic Clouds at 1 AU. Solar Physics, 291(7), 2145-2163.
http://dx.doi.org/10.1007/s11207-016-0955-5
---------- CHICAGO ----------
Rodriguez, L., Masías-Meza, J.J., Dasso, S., Démoulin, P., Zhukov, A.N., Gulisano, A.M., et al. "Typical Profiles and Distributions of Plasma and Magnetic Field Parameters in Magnetic Clouds at 1 AU" . Solar Physics 291, no. 7 (2016) : 2145-2163.
http://dx.doi.org/10.1007/s11207-016-0955-5
---------- MLA ----------
Rodriguez, L., Masías-Meza, J.J., Dasso, S., Démoulin, P., Zhukov, A.N., Gulisano, A.M., et al. "Typical Profiles and Distributions of Plasma and Magnetic Field Parameters in Magnetic Clouds at 1 AU" . Solar Physics, vol. 291, no. 7, 2016, pp. 2145-2163.
http://dx.doi.org/10.1007/s11207-016-0955-5
---------- VANCOUVER ----------
Rodriguez, L., Masías-Meza, J.J., Dasso, S., Démoulin, P., Zhukov, A.N., Gulisano, A.M., et al. Typical Profiles and Distributions of Plasma and Magnetic Field Parameters in Magnetic Clouds at 1 AU. Sol. Phys. 2016;291(7):2145-2163.
http://dx.doi.org/10.1007/s11207-016-0955-5