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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
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
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
Volumen:47
Número:3
Página de inicio:295
Página de fin:299
Título revista:Geofisica Internacional
Título revista abreviado:Geofis. Int.
ISSN:00167169
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 [ ]