Artículo

Schmeider, B.; Démoulin, P.; Aulanier, G.; Malherbe, J.M.; Van Driel-Gesztelyi, L.; Mandrini, C.H.; Roudier, T.; Nitta, N.; Harra-Murnion, L.K. "3-D reconnection related to new emerging flux" (1997) Advances in Space Research. 19(12):1871-1874
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Abstract:

We present evidences that emergence of new flux in the lower atmosphere leads to magnetic reconnection of field lines. In a first phase the phenomenon is observed in the chromosphere by the formation of dark filaments (arch filament system) which are overlaid by bright loops visible in soft X-rays. Different types of event appear according to the magnetic field configuration and the amount of energy involved. 3-D modelling of the photospheric magnetic field provides a new tool for understanding reconnection in real configurations. The observed chromospheric and coronal loops are good diagnostics for the modelling. We document our statement by examples obtained during coordinated campaigns with the Hα Multichannel Subtractive Double Pass spectrographs-MSDP (Pic du Midi and Tenerife) and the Yohkoh instruments. © 1997 COSPAR. Published by Elsevier Science Ltd.

Registro:

Documento: Artículo
Título:3-D reconnection related to new emerging flux
Autor:Schmeider, B.; Démoulin, P.; Aulanier, G.; Malherbe, J.M.; Van Driel-Gesztelyi, L.; Mandrini, C.H.; Roudier, T.; Nitta, N.; Harra-Murnion, L.K.
Filiación:Observatoire de Paris, D.A.S.O.P., F-92195 Meudon, France
Konkoly Observatory, Budapest, Pf. 67, H-1525, Hungary
Inst. Astronomia y Fis. del Espacio, IAFE, CC.67, Suc.28, 1428 Buenos Aires, Argentina
OPMT, BP 136, 67201 Bagnères de Bigorre, France
Lockheed, 3251 Hanover Street, Palo Alto, CA 94304, United States
Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Surrey RH5 6HT, United Kingdom
Año:1997
Volumen:19
Número:12
Página de inicio:1871
Página de fin:1874
DOI: http://dx.doi.org/10.1016/S0273-1177(97)00090-2
Título revista:Advances in Space Research
Título revista abreviado:Adv Space Res
ISSN:02731177
CODEN:ASRSD
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_02731177_v19_n12_p1871_Schmeider

Referencias:

  • Démoulin, P., Hénoux, J.C., Priest, E.R., Mandrini, C.H., Quasi-separatrix layers in solar flares I method (1996) Astron. and Astrophys., 308, p. 643
  • Mandrini, C.H., Démoulin, P., Van Driel-Gesztelyi, L., Schmieder, B., Cauzzi, G., Hofmann, A., 3-D magnetic reconnection at an X-ray bright point (1996) Solar Phys., , in press
  • Priest, E., Démoulin, P., Three-dimensional magnetic reconnection without null points, I (1995) J.G.R., 100, p. 23443
  • Van Driel-Gesztelyi, L., Schmieder, B., Cauzzi, G., Mein, N., Hofmann, A., Nitta, N., Kurokawa, H., Staiger, J., X-ray bright point flares due to magnetic reconnection (1996) Solar Phys., 163, p. 145

Citas:

---------- APA ----------
Schmeider, B., Démoulin, P., Aulanier, G., Malherbe, J.M., Van Driel-Gesztelyi, L., Mandrini, C.H., Roudier, T.,..., Harra-Murnion, L.K. (1997) . 3-D reconnection related to new emerging flux. Advances in Space Research, 19(12), 1871-1874.
http://dx.doi.org/10.1016/S0273-1177(97)00090-2
---------- CHICAGO ----------
Schmeider, B., Démoulin, P., Aulanier, G., Malherbe, J.M., Van Driel-Gesztelyi, L., Mandrini, C.H., et al. "3-D reconnection related to new emerging flux" . Advances in Space Research 19, no. 12 (1997) : 1871-1874.
http://dx.doi.org/10.1016/S0273-1177(97)00090-2
---------- MLA ----------
Schmeider, B., Démoulin, P., Aulanier, G., Malherbe, J.M., Van Driel-Gesztelyi, L., Mandrini, C.H., et al. "3-D reconnection related to new emerging flux" . Advances in Space Research, vol. 19, no. 12, 1997, pp. 1871-1874.
http://dx.doi.org/10.1016/S0273-1177(97)00090-2
---------- VANCOUVER ----------
Schmeider, B., Démoulin, P., Aulanier, G., Malherbe, J.M., Van Driel-Gesztelyi, L., Mandrini, C.H., et al. 3-D reconnection related to new emerging flux. Adv Space Res. 1997;19(12):1871-1874.
http://dx.doi.org/10.1016/S0273-1177(97)00090-2