Abstract:
We provide evidence for the link between coronal ejective events and their interplanetary manifestations. We combine multi-wavelength remote sensing and in situ observations with the computation of the coronal and interplanetary magnetic fields using a standard linear force-free approach. The analysis and computations are applied to one of the smallest (on 11 May, 1998) and to a large ejecta (on 14 October, 1995), as well as to their related magnetic clouds. The connection between the coronal and interplanetary events is shown by comparing the magnetic helicity variation (pre- to post-eruption) in the corona to the helicity content in the associated magnetic clouds, and through the compatibility of other observational characteristics and computed quantities (e.g. magnetic flux) in both environments. Our results show that, within the uncertainties, the computed helicities are in good agreement. For the event on 11 May, 1998, the ejected magnetic flux and the flux in the associated interplanetary cloud also agree. Such quantitative analyses help to unambiguously identify the solar source region of magnetic clouds, and allow us to constrain theoretical models in both environments.
Registro:
Documento: |
Conferencia
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Título: | Quantitative link between solar ejecta and interplanetary magnetic clouds: Magnetic helicity |
Autor: | Mandrini, C.H.; Dasso, S.; Luoni, M.L.; Pohjolainen, S.; Démoulin, P.; Van Driel-Gesztelyi, L. |
Ciudad: | Katlenburg - Lindau |
Filiación: | Instituto de Astronomía y Física Del Espacio, IAFE, CONICET-UBA, CC. 67, Suc. 28, 1428, Buenos Aires, Argentina Departamento de Física, Facultad de Ciencias Exactas y Naturales, PBI, 1428 Buenos Aires, Argentina Tuorla Observatory/VISPA, University of Turku, FIN-21500 Piikkiö, Finland Oservatoire de Paris, LESIA, UMR 8109 (CNRS), F-92195, Meudon, France Mullard Space Science Laboratory, Univ. College London, Dorking, Surrey, RH5 6NT, United Kingdom Konkoly Observatory, H-1525 Budapest, P.O. Box 67, Hungary
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Palabras clave: | Magnetic fields; Magnetic flux; Mathematical models; Remote sensing; Magnetic clouds; Solar ejecta; Solar radiation |
Año: | 2005
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Número: | 596
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Página de inicio: | 391
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Página de fin: | 396
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Título revista: | International Scientific Conference on Chromospheric and Coronal Magnetic Fields
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Título revista abreviado: | Eur Space Agency Spec Publ ESA SP
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ISSN: | 03796566
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CODEN: | ESPUD
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Registro: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03796566_v_n596_p391_Mandrini |
Referencias:
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Citas:
---------- APA ----------
Mandrini, C.H., Dasso, S., Luoni, M.L., Pohjolainen, S., Démoulin, P. & Van Driel-Gesztelyi, L.
(2005)
. Quantitative link between solar ejecta and interplanetary magnetic clouds: Magnetic helicity. International Scientific Conference on Chromospheric and Coronal Magnetic Fields(596), 391-396.
Recuperado de https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03796566_v_n596_p391_Mandrini [ ]
---------- CHICAGO ----------
Mandrini, C.H., Dasso, S., Luoni, M.L., Pohjolainen, S., Démoulin, P., Van Driel-Gesztelyi, L.
"Quantitative link between solar ejecta and interplanetary magnetic clouds: Magnetic helicity"
. International Scientific Conference on Chromospheric and Coronal Magnetic Fields, no. 596
(2005) : 391-396.
Recuperado de https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03796566_v_n596_p391_Mandrini [ ]
---------- MLA ----------
Mandrini, C.H., Dasso, S., Luoni, M.L., Pohjolainen, S., Démoulin, P., Van Driel-Gesztelyi, L.
"Quantitative link between solar ejecta and interplanetary magnetic clouds: Magnetic helicity"
. International Scientific Conference on Chromospheric and Coronal Magnetic Fields, no. 596, 2005, pp. 391-396.
Recuperado de https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03796566_v_n596_p391_Mandrini [ ]
---------- VANCOUVER ----------
Mandrini, C.H., Dasso, S., Luoni, M.L., Pohjolainen, S., Démoulin, P., Van Driel-Gesztelyi, L. Quantitative link between solar ejecta and interplanetary magnetic clouds: Magnetic helicity. Eur Space Agency Spec Publ ESA SP. 2005(596):391-396.
Available from: https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03796566_v_n596_p391_Mandrini [ ]