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.
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 |