Multiwavelengths study of active region 09778

Details Multiwavelengths study of active region 09778 Multiwavelengths study of active region 09778

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1043..272c&link_type=abstract

EXPLORING THE SOLAR SYSTEM AND THE UNIVERSE. AIP Conference Proceedings, Volume 1043, pp. 272-276 (2008).

Astronomy and Astrophysics

Astronomy

Corona, Flares, Magnetohydrodynamics And Plasmas, Chromosphere, Astronomical Observations, Solar System, Planetology

Scientific paper

We have studied the evolution and decay of the active region 09778, as well as the evolution of the filament below it and its possible relation with the active region. Using data from SOHO-LASCO, BBSO, Mauna Loa, we analyzed the evolution of active region in different wavelengths. The AR presented high flare productivity. From MDI magnetograms we extrapolate the magnetic field in order to obtain a 3D configuration and to understand flare occurrence.

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