Multi-wavelength observations of flares and eruptive filaments
Author:
Publisher
Springer Science and Business Media LLC
Subject
Geophysics
Link
http://link.springer.com/content/pdf/10.2478/s11600-008-0040-z.pdf
Reference19 articles.
1. 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.
2. 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.
3. Contarino, L., P. Romano, and F. Zuccarello (2006b), Cancelling magnetic feature and filament activation, Astron. Nachr. 327, 674–679, DOI: 10.1002/asna.200610619.
4. 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.
5. 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.
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