Abstract:
The conservation of magnetic flux in systems of very low dissipation, as the interplanetary medium, is used to analyze magnetic clouds in significant expansion. In particular, we analyze the fast and huge event observed at one astronomical unit in the solar wind on Nov. 9-10, 2004. We compare magnetic and velocity observations to two self-similar and free expansion models that allow us to correct the mixing spatial-variation/time-evolution observed in situ by the spacecrafts. As magnetic clouds are astrophysical objects that transport a very important amount of magnetic flux and helicity from the Sun to the interplanetary medium, we compare the values of these global quantities obtained using the present models with those values coming from the commonly used static Lundquist's model.
Registro:
Documento: |
Artículo
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Título: | Dynamical evolution of magnetic flux ropes in the solar wind |
Autor: | Nakwacki, M.S.; Dasso, S.; Démoulin, P.; Mandrini, C.H. |
Filiación: | Instituto de Astronomía y Física del Espacio, Consejo Nacional de Investigaciones Científicas y Técnicas, Universidad de Buenos Aires, Buenos Aires, Argentina Departamento de Física, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Buenos Aires, Argentina Observatoire de Paris, Laboratorie d'Etudes Spatiales et d'Instrumentation en Astrophysique, F-92195 Meudon Principal Cedex, France
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Palabras clave: | Coronal mass ejections; Disturbances; Interplanetary; Magnetic fields; Magnetic reconnection; Observational signatures; Solar wind; astronomy; coronal mass ejection; geomagnetic field; numerical model; observational method; solar wind; spatial variation; temporal evolution |
Año: | 2008
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Volumen: | 47
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Número: | 3
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Página de inicio: | 295
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Página de fin: | 299
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Título revista: | Geofisica Internacional
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Título revista abreviado: | Geofis. Int.
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ISSN: | 00167169
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Registro: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00167169_v47_n3_p295_Nakwacki |
Referencias:
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Citas:
---------- APA ----------
Nakwacki, M.S., Dasso, S., Démoulin, P. & Mandrini, C.H.
(2008)
. Dynamical evolution of magnetic flux ropes in the solar wind. Geofisica Internacional, 47(3), 295-299.
Recuperado de https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00167169_v47_n3_p295_Nakwacki [ ]
---------- CHICAGO ----------
Nakwacki, M.S., Dasso, S., Démoulin, P., Mandrini, C.H.
"Dynamical evolution of magnetic flux ropes in the solar wind"
. Geofisica Internacional 47, no. 3
(2008) : 295-299.
Recuperado de https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00167169_v47_n3_p295_Nakwacki [ ]
---------- MLA ----------
Nakwacki, M.S., Dasso, S., Démoulin, P., Mandrini, C.H.
"Dynamical evolution of magnetic flux ropes in the solar wind"
. Geofisica Internacional, vol. 47, no. 3, 2008, pp. 295-299.
Recuperado de https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00167169_v47_n3_p295_Nakwacki [ ]
---------- VANCOUVER ----------
Nakwacki, M.S., Dasso, S., Démoulin, P., Mandrini, C.H. Dynamical evolution of magnetic flux ropes in the solar wind. Geofis. Int. 2008;47(3):295-299.
Available from: https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00167169_v47_n3_p295_Nakwacki [ ]