Solar transient activity: Magnetic energy release and topology
We will discuss how the computation and analysis of the coronal magnetic field topology can be used to identify the energy release locations and their physical characteristics.
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| Otros Autores: | , , |
| Formato: | Acta de conferencia Capítulo de libro |
| Lenguaje: | Inglés |
| Publicado: |
Universidad Nacional Autonoma de Mexico
2014
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| Acceso en línea: | Registro en Scopus Handle Registro en la Biblioteca Digital |
| Aporte de: | Registro referencial: Solicitar el recurso aquí |
| LEADER | 03198caa a22004337a 4500 | ||
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| 001 | PAPER-14573 | ||
| 003 | AR-BaUEN | ||
| 005 | 20240513192007.0 | ||
| 008 | 190411s2014 xx ||||fo|||| 10| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-84914153107 | |
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 100 | 1 | |a Mandrini, C.H. | |
| 245 | 1 | 0 | |a Solar transient activity: Magnetic energy release and topology |
| 260 | |b Universidad Nacional Autonoma de Mexico |c 2014 | ||
| 270 | 1 | 0 | |m Mandrini, C.H.; Instituto de Astronomía y Física del Espacio, IAFE, UBA-CONICET, CC. 67, Suc. 28, Argentina |
| 506 | |2 openaire |e Política editorial | ||
| 504 | |a Aulanier, G., Pariat, E., Démoulin, P., (2005) A&A, 444, p. 961 | ||
| 504 | |a Aulanier, G., Pariat, E., Démoulin, P., DeVore, C.R., (2006) Solar Phys., 238, p. 347 | ||
| 504 | |a Démoulin, P., Hénoux, J.C., Priest, E.R., Mandrini, C.H., (1996) A&A, 308, p. 643 | ||
| 504 | |a Démoulin, P., Bagalá, L.G., Mandrini, C.H., Hénoux, J.C., Rovira, M.G., (1997) A&A, 325, p. 305 | ||
| 504 | |a Longcope, D.W., (2006) Living Rev. Solar Phys., 2. , http://www.livingreviews.org/lrsp-2005-7 | ||
| 504 | |a Mandrini, C.H., Démoulin, P., Bagalá, L.G., Van Driel-Gesztelyi, L., Hénoux, J.C., Schmieder, B., Rovira, M.G., (1997) Solar. Phys., 174, p. 229 | ||
| 504 | |a Mandrini, C.H., Schmieder, B., Guo, Y., Démoulin, P., Cristiani, G.D., (2014) Sol. Phys., 289, p. 2041 | ||
| 504 | |a Pariat, E., Aulanier, G., Schmieder, B., Georgoulis, M.K., Rust, D.M., Bernasconi, P.N., (2004) A&A, 614, p. 1099 | ||
| 504 | |a Titov, V.S., Priest, E.R., Démoulin, P., (1993) A&A, 276, p. 564 | ||
| 504 | |a Titov, V.S., Hornig, G., Démoulin, P., (2002) JGR, 107 (3), pp. 1-13. , SSHA4 - | ||
| 520 | 3 | |a We will discuss how the computation and analysis of the coronal magnetic field topology can be used to identify the energy release locations and their physical characteristics. |l eng | |
| 593 | |a Instituto de Astronomía y Física del Espacio, IAFE, UBA-CONICET, CC. 67, Suc. 28, C.A.B.A., 1428, Argentina | ||
| 593 | |a Facultad de Ciencias Exactas y Naturales, FCEN, UBA, Buenos Aires, Argentina | ||
| 700 | 1 | |a Gregorio-Hetem, J. | |
| 700 | 1 | |a Mateus, A. | |
| 700 | 1 | |a Cid Fernandes, R. | |
| 711 | 2 | |d 24 November 2013 through 30 November 2013 |g Código de la conferencia: 109340 | |
| 773 | 0 | |d Universidad Nacional Autonoma de Mexico, 2014 |g v. 44 |h pp. 47 |p Rev.Mex. Astron. Astrofis. Ser. Conf. |n Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias |x 14052059 |w (AR-BaUEN)CENRE-1052 |t 14th Latin American Regional IAU Meeting, LARIM 2013 | |
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| 856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_14052059_v44_n_p47_Mandrini |x handle |y Handle |
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