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Schmieder, B.; Démoulin, P.; Pariat, E.; Török, T.; Molodij, G.; Mandrini, C.H.; Dasso, S.; Chandra, R.; Uddin, W.; Kumar, P.; Manoharan, P.K.; Venkatakrishnan, P.; Srivastava, N. "Actors of the main activity in large complex centres during the 23 solar cycle maximum" (2011) Advances in Space Research. 47(12):2081-2091
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Abstract:

During the maximum of Solar Cycle 23, large active regions had a long life, spanning several solar rotations, and produced large numbers of X-class flares and CMEs, some of them associated to magnetic clouds (MCs). This is the case for the Halloween active regions in 2003. The most geoeffective MC of the cycle (Dst = -457) had its source during the disk passage of one of these active regions (NOAA 10501) on 18 November 2003. Such an activity was presumably due to continuous emerging magnetic flux that was observed during this passage. Moreover, the region exhibited a complex topology with multiple domains of different magnetic helicities. The complexity was observed to reach such unprecedented levels that a detailed multi-wavelength analysis is necessary to precisely identify the solar sources of CMEs and MCs. Magnetic clouds are identified using in situ measurements and interplanetary scintillation (IPS) data. Results from these two different sets of data are also compared. © 2010 Published by Elsevier Ltd. on behalf of COSPAR.

Registro:

Documento: Artículo
Título:Actors of the main activity in large complex centres during the 23 solar cycle maximum
Autor:Schmieder, B.; Démoulin, P.; Pariat, E.; Török, T.; Molodij, G.; Mandrini, C.H.; Dasso, S.; Chandra, R.; Uddin, W.; Kumar, P.; Manoharan, P.K.; Venkatakrishnan, P.; Srivastava, N.
Filiación:Observatoire de Paris, LESIA, 92195 Meudon, France
Instituto de Astronomía y Física Del Espacio (UBA-CONICET), Facultad de Ciencias Exactas y Naturales (UBA), Buenos Aires, Argentina
Department of Physics, DSB Campus, Kumaun University, Nainital 263 002, Uttarakhand, India
ARIES, Manora Peak, Nainital 263 129, India
Radio Astronomy Centre, Tata Institute of Fundamental Research, Udhagamandalam (Ooty) 643 001, India
Udaipur Solar Observatory, 198, Dewali, Udaipur 313 001, India
Predictive Science, Inc., 9990 Mesa Rim Road, San Diego, CA 92121, United States
Palabras clave:Active region; Coronal mass ejection; Magnetic clouds; Magnetic helicity; Active regions; Complex topology; Coronal mass ejection; Helicities; In-situ measurement; Interplanetary scintillation; Long life; Magnetic clouds; Magnetic helicity; Multiple domains; Multiwavelength; Solar cycle; Solar rotation; Solar source; X-class flares; Clouds; Extraterrestrial atmospheres; Magnetic flux; Solar energy; Solar system; Magnetic domains
Año:2011
Volumen:47
Número:12
Página de inicio:2081
Página de fin:2091
DOI: http://dx.doi.org/10.1016/j.asr.2011.02.001
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_v47_n12_p2081_Schmieder

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Citas:

---------- APA ----------
Schmieder, B., Démoulin, P., Pariat, E., Török, T., Molodij, G., Mandrini, C.H., Dasso, S.,..., Srivastava, N. (2011) . Actors of the main activity in large complex centres during the 23 solar cycle maximum. Advances in Space Research, 47(12), 2081-2091.
http://dx.doi.org/10.1016/j.asr.2011.02.001
---------- CHICAGO ----------
Schmieder, B., Démoulin, P., Pariat, E., Török, T., Molodij, G., Mandrini, C.H., et al. "Actors of the main activity in large complex centres during the 23 solar cycle maximum" . Advances in Space Research 47, no. 12 (2011) : 2081-2091.
http://dx.doi.org/10.1016/j.asr.2011.02.001
---------- MLA ----------
Schmieder, B., Démoulin, P., Pariat, E., Török, T., Molodij, G., Mandrini, C.H., et al. "Actors of the main activity in large complex centres during the 23 solar cycle maximum" . Advances in Space Research, vol. 47, no. 12, 2011, pp. 2081-2091.
http://dx.doi.org/10.1016/j.asr.2011.02.001
---------- VANCOUVER ----------
Schmieder, B., Démoulin, P., Pariat, E., Török, T., Molodij, G., Mandrini, C.H., et al. Actors of the main activity in large complex centres during the 23 solar cycle maximum. Adv. Space Res. 2011;47(12):2081-2091.
http://dx.doi.org/10.1016/j.asr.2011.02.001