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Multi-wavelength observations of flares and eruptive filaments

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Abstract

In this paper we report some results obtained from multi-wavelength observations carried out to study the mechanisms operating in flares and filament eruptions. Most of these studies have given indication of the presence of phenomena that might be considered signatures of magnetic reconnection, while others have pointed out the important role played by magnetic helicity transport in corona before the eruptive phase.

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References

  • Contarino, L., P. Romano, V.B. Yurchyshyn, and F. Zuccarello (2003), THEMIS, BBSO, MDI and TRACE observations of a filament eruption, Solar Phys. 216, 173–188, DOI: 10.1023/A:1026107727149.

    Article  Google Scholar 

  • Contarino, L., P. Romano, and F. Zuccarello (2006a), RHESSI and TRACE observations of an M 2.5 flare: a direct application of the Kopp and Pneuman model (Research Note), Astron. Astrophys. 458, 297–300, DOI: 10.1051/0004-6361:20054638.

    Article  Google Scholar 

  • Contarino, L., P. Romano, and F. Zuccarello (2006b), Cancelling magnetic feature and filament activation, Astron. Nachr. 327, 674–679, DOI: 10.1002/asna.200610619.

    Article  Google Scholar 

  • Demoulin, P., and M.A. Berger (2003), Magnetic energy and helicity fluxes at the photospheric level, Solar Phys. 215, 203–215, DOI: 10.1023/A:1025679813955.

    Article  Google Scholar 

  • Heyvaerts, J., E.R. Priest, and D.M. Rust (1977), An emerging flux model for the solar flare phenomenon, Astrophys. J. 216, 123–137, DOI: 10.1086/155453.

    Article  Google Scholar 

  • Kopp, R.A., and G.W. Pneuman (1976), Magnetic reconnection in the corona and the loop prominence phenomenon, Solar Phys. 50, 85–98, DOI: 10.1007/BF00206193.

    Article  Google Scholar 

  • Litvinenko, Y.E. (1999), Photospheric Magnetic Reconnection and Canceling Magnetic Features on the Sun, Astrophys. J. 515, 435–440, DOI: 10.1086/307001.

    Article  Google Scholar 

  • Litvinenko, Y.E., and B.V. Somov (1994), Magnetic reconnection in the temperature minimum region and prominence formation, Solar Phys. 151, 265–270, DOI: 10.1007/BF00679075.

    Article  Google Scholar 

  • Miklenic, C.H., A.M. Veronig, B. Vršnak and A. Hanslmeier (2007), Reconnection and energy release rates in a two-ribbon flare, Astron. Astrophys. 461, 697–706, DOI: 10.1051/0004-6361:20065751.

    Article  Google Scholar 

  • Moon, Y.J., J. Chae, G.S. Choe, H. Wang, Y.D. Park, H.S. Yun, V. Yurchyshyn, and P.R. Goode (2002), Flare activity and magnetic helicity injection by photospheric horizontal motions, Astrophys. J. 574, 1066–1073, DOI: 10.1086/340975.

    Article  Google Scholar 

  • Priest, E.R., and T.G. Forbes (2000), Magnetic Reconnection: MHD Theory and Applications, Cambridge University Press, Cambridge.

    Google Scholar 

  • Priest, E.R., and T.G. Forbes (2002), The magnetic nature of solar flares, Astron. Astrophys. Rev. 10, 313–377, DOI: 10.1007/s001590100013.

    Article  Google Scholar 

  • Romano, P., L. Contarino, and F. Zuccarello (2003a), Eruption of a helically twisted prominence, Solar Phys. 214, 313–323, DOI: 10.1023/A:1024257603143.

    Article  Google Scholar 

  • Romano, P., L. Contarino, and F. Zuccarello (2003b), Magnetic helicity transport in corona and filament eruptions, Solar Phys. 218, 137–150, DOI: 10.1023/B:SOLA.0000013035.62270.e4.

    Article  Google Scholar 

  • Romano, P., L. Contarino, and F. Zuccarello (2005), Observational evidence of the primary role played by photospheric motions in magnetic helicity transport before a filament eruption, Astron. Astrophys. 433, 683–690, DOI: 10.1051/0004-6361:20041807.

    Article  Google Scholar 

  • Romano, P., F. Zuccarello, and L. Contarino (2007), An M1.5 flare triggered by a multireconnection process, Solar Phys. 240, 49–61, DOI: 10.1007/s11207-006-0287-y.

    Article  Google Scholar 

  • Ternullo, M., L. Contarino, P. Romano, and F. Zuccarello (2006), A statistical analysis of sunspot groups hosting M and X flares, Astron. Nachr. 327, 36–43, DOI: 10.1002/asna.200510485.

    Article  Google Scholar 

  • Zuccarello, F., L. Contarino, P. Romano, and E.R. Priest (2003), Flare activity in solar active region 8421 observed by the TRACE satellite, Astron. Astrophys. 402, 1085–1102, DOI: 10.1051/0004-6361:20030316.

    Article  Google Scholar 

  • Zuccarello, F., V. Battiato, L. Contarino, P. Romano, and D. Spadaro (2007), Plasma motions in a short-lived filament related to a magnetic flux cancellation, Astron. Astrophys. 468, 299–305, DOI: 10.1051/0004-6361:20066556.

    Article  Google Scholar 

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Correspondence to Francesca Zuccarello.

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Zuccarello, F., Contarino, L., Romano, P. et al. Multi-wavelength observations of flares and eruptive filaments. Acta Geophys. 57, 24–30 (2009). https://doi.org/10.2478/s11600-008-0040-z

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  • DOI: https://doi.org/10.2478/s11600-008-0040-z

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