Magnetic sources of flares and CMEs from multi-wavelength flare studies
We will present the data analysis of an observing campaign on October 2003 with the objective of. understanding the onset of Coronal Mass Ejections (CME) and solar flares. The magnetic field was observed with THEMIS and MDI, the chromosphere with the MSDP operating on THEMIS, the EUV images with SOH...
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| Otros Autores: | , , , |
| Formato: | Acta de conferencia Capítulo de libro |
| Lenguaje: | Inglés |
| Publicado: |
2006
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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 | 03995caa a22005897a 4500 | ||
|---|---|---|---|
| 001 | PAPER-21800 | ||
| 003 | AR-BaUEN | ||
| 005 | 20250306082639.0 | ||
| 008 | 190411s2006 xx ||||fo|||| 10| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-33749175599 | |
| 030 | |a ESPUD | ||
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 100 | 1 | |a Schmieder, B. | |
| 245 | 1 | 0 | |a Magnetic sources of flares and CMEs from multi-wavelength flare studies |
| 260 | |c 2006 | ||
| 270 | 1 | 0 | |m Schmieder, B.; Observatoire de Paris, LESIA, Meudon, France |
| 504 | |a Antiochos, S.K., DeVore, C.R., Klimchuk, J.A., (1999) Astrophys. J., 510, p. 485 | ||
| 504 | |a Berlicki, A., Mein, P., Schmieder, B., (2006) A&A, 445, p. 1127 | ||
| 504 | |a Démoulin, P., Bagala, L.G., Mandrini, C.H., (1997) A&A, 325, p. 305 | ||
| 504 | |a Li, H., Berlicki, A., Schmieder, B., (2005) A&A, 438, p. 325 | ||
| 504 | |a Mandrini, C.H., Démoulin, P., Schmieder, B., Deluca, E.E., Pariat, E., Uddin, W., (2006) Solar Phys., , in press | ||
| 504 | |a Schmieder, B., Mandrini, C.H., Démoulin, P., Pariat, E., Berlicki, A., Deluca, E.E., (2006) Adv. Sp. Res., , in pressA4 - European Space Agency | ||
| 506 | |2 openaire |e Política editorial | ||
| 520 | 3 | |a We will present the data analysis of an observing campaign on October 2003 with the objective of. understanding the onset of Coronal Mass Ejections (CME) and solar flares. The magnetic field was observed with THEMIS and MDI, the chromosphere with the MSDP operating on THEMIS, the EUV images with SOHO/EIT and TRACE, the X-rays with RHESSI. We will show how important is the magnetic configuration of the active region to produce CMEs. Two examples of flares will be presented: the 28 Oct 2003 X17 flare and the 20 October 2003 M 1.9 flare. The magnetic field analysis of the active regions is done using a linear-force-free field code. The X17 flare gave a halo CME while the M1.9 flare has no corresponding CME. Before the X17 flare there was a pre-flare event which allowed to change the connectivities in a first phase and to relax the stressed field in a second phase producing the X17 flare. A compact twisted emerging flux was responsible of the M1.9 flare, which remains a compact flare due to very tied overlaying loops. RHESSI showed that even during the M1.9 flare both components thermal and non thermal component are present. |l eng | |
| 593 | |a Observatoire de Paris, LESIA, Meudon, France | ||
| 593 | |a IAFE, Buenos Aires, Argentina | ||
| 593 | |a Astronomical Institute, Wroclaw University, Poland | ||
| 593 | |a Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, China | ||
| 690 | 1 | 0 | |a CORONAL MASS EJECTIONS |
| 690 | 1 | 0 | |a FLARES |
| 690 | 1 | 0 | |a SUN |
| 690 | 1 | 0 | |a IMAGE ANALYSIS |
| 690 | 1 | 0 | |a MAGNETIC FIELDS |
| 690 | 1 | 0 | |a SOLAR ENERGY |
| 690 | 1 | 0 | |a SUN |
| 690 | 1 | 0 | |a X RAYS |
| 690 | 1 | 0 | |a CORONAL MASS EJECTIONS (CME) |
| 690 | 1 | 0 | |a EUV IMAGES |
| 690 | 1 | 0 | |a FLARES |
| 690 | 1 | 0 | |a LINEAR-FORCE-FREE FIELD CODE |
| 690 | 1 | 0 | |a SPACE RESEARCH |
| 700 | 1 | |a Mandrini, C. | |
| 700 | 1 | |a Berlicki, A. | |
| 700 | 1 | |a Démoulin, Pascal | |
| 700 | 1 | |a Li, H. | |
| 711 | 2 | |c Sicily |d 7 May 2006 through 12 May 2006 |g Código de la conferencia: 68134 | |
| 773 | 0 | |d 2006 |k n. 617 |p Eur Space Agency Spec Publ ESA SP |n European Space Agency, (Special Publication) ESA SP |x 03796566 |z 9290929286 |z 9789290929284 |t SOHO-17: 10 Years of SOHO and Beyond | |
| 856 | 4 | 1 | |u https://www.scopus.com/inward/record.uri?eid=2-s2.0-33749175599&partnerID=40&md5=f74d95b37da77417532cffebfff45c47 |x registro |y Registro en Scopus |
| 856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_03796566_v_n617_p_Schmieder |x handle |y Handle |
| 856 | 4 | 0 | |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03796566_v_n617_p_Schmieder |x registro |y Registro en la Biblioteca Digital |
| 961 | |a paper_03796566_v_n617_p_Schmieder |b paper |c PE | ||
| 962 | |a info:eu-repo/semantics/conferenceObject |a info:ar-repo/semantics/documento de conferencia |b info:eu-repo/semantics/publishedVersion | ||