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Mandrini, C.H.; Nuevo, F.A.; Vásquez, A.M.; Démoulin, P.; van Driel-Gesztelyi, L.; Baker, D.; Culhane, J.L.; Cristiani, G.D.; Pick, M. "How Can Active Region Plasma Escape into the Solar Wind from Below a Closed Helmet Streamer?" (2014) Solar Physics. 289(11):4151-4171
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Abstract:

Recent studies show that active-region (AR) upflowing plasma, observed by the EUV-Imaging Spectrometer (EIS) onboard Hinode, can gain access to open-field lines and be released into the solar wind (SW) via magnetic-interchange reconnection at magnetic null-points in pseudo-streamer configurations. When only one bipolar AR is present on the Sun and is fully covered by the separatrix of a streamer, such as AR 10978 in December 2007, it seems unlikely that the upflowing AR plasma can find its way into the slow SW. However, signatures of plasma with AR composition have been found at 1 AU by Culhane et al. (Solar Phys. 289, 3799, 2014) that apparently originated west of AR 10978. We present a detailed topology analysis of AR 10978 and the surrounding large-scale corona based on a potential-field source-surface (PFSS) model. Our study shows that it is possible for the AR plasma to move around the streamer separatrix and be released into the SW via magnetic reconnection, which occurs in at least two main steps. We analyse data from the Nançay Radioheliograph (NRH) in a search for evidence of the chain of magnetic reconnections that we propose. We find a noise storm above the AR and several varying sources at 150.9 MHz. Their locations suggest that they might be associated with particles accelerated during the first-step reconnection process at a null point well outside of the AR. We find no evidence of the second reconnection step in the radio data, however. Our results demonstrate that even when it appears highly improbable for the AR plasma to reach the SW, indirect channels involving a sequence of reconnections can make it possible. © 2014 Springer Science+Business Media Dordrecht.

Registro:

Documento: Artículo
Título:How Can Active Region Plasma Escape into the Solar Wind from Below a Closed Helmet Streamer?
Autor:Mandrini, C.H.; Nuevo, F.A.; Vásquez, A.M.; Démoulin, P.; van Driel-Gesztelyi, L.; Baker, D.; Culhane, J.L.; Cristiani, G.D.; Pick, M.
Filiación:Instituto de Astronomía y Física del Espacio (IAFE), CONICET-UBA, Buenos Aires, Argentina
Facultad de Ciencias Exactas y Naturales (FCEN), UBA, Buenos Aires, Argentina
Observatoire de Paris, LESIA, UMR 8109 (CNRS), 92195 Meudon Principal Cedex, France
UCL-Mullard Space Science Laboratory, Holmbury St. Mary, Dorking, Surrey, RH5 6NT, United Kingdom
Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, Hungarian Academy of Sciences, Budapest, Hungary
Palabras clave:Active regions; Corona active; Magnetic extrapolations; Magnetic fields; Quiet; Radio Bursts; Radio emission; Solar wind; Type I
Año:2014
Volumen:289
Número:11
Página de inicio:4151
Página de fin:4171
DOI: http://dx.doi.org/10.1007/s11207-014-0582-y
Título revista:Solar Physics
Título revista abreviado:Sol. Phys.
ISSN:00380938
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00380938_v289_n11_p4151_Mandrini

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Citas:

---------- APA ----------
Mandrini, C.H., Nuevo, F.A., Vásquez, A.M., Démoulin, P., van Driel-Gesztelyi, L., Baker, D., Culhane, J.L.,..., Pick, M. (2014) . How Can Active Region Plasma Escape into the Solar Wind from Below a Closed Helmet Streamer?. Solar Physics, 289(11), 4151-4171.
http://dx.doi.org/10.1007/s11207-014-0582-y
---------- CHICAGO ----------
Mandrini, C.H., Nuevo, F.A., Vásquez, A.M., Démoulin, P., van Driel-Gesztelyi, L., Baker, D., et al. "How Can Active Region Plasma Escape into the Solar Wind from Below a Closed Helmet Streamer?" . Solar Physics 289, no. 11 (2014) : 4151-4171.
http://dx.doi.org/10.1007/s11207-014-0582-y
---------- MLA ----------
Mandrini, C.H., Nuevo, F.A., Vásquez, A.M., Démoulin, P., van Driel-Gesztelyi, L., Baker, D., et al. "How Can Active Region Plasma Escape into the Solar Wind from Below a Closed Helmet Streamer?" . Solar Physics, vol. 289, no. 11, 2014, pp. 4151-4171.
http://dx.doi.org/10.1007/s11207-014-0582-y
---------- VANCOUVER ----------
Mandrini, C.H., Nuevo, F.A., Vásquez, A.M., Démoulin, P., van Driel-Gesztelyi, L., Baker, D., et al. How Can Active Region Plasma Escape into the Solar Wind from Below a Closed Helmet Streamer?. Sol. Phys. 2014;289(11):4151-4171.
http://dx.doi.org/10.1007/s11207-014-0582-y