A&A 465, 603-612 (2007)
DOI: 10.1051/0004-6361:20065845
Stationary parts of an EIT and Moreton wave: a topological model
C. Delannée1, J.-F. Hochedez1, and G. Aulanier21 Royal Observatory of Belgium, Brussels, Belgium
e-mail: ceaulanier@wanadoo.fr
2 LESIA, Meudon observatory, Meudon, France
(Received 16 June 2006 / Accepted 30 August 2006)
Abstract
Context.EIT and Moreton waves came into focus in 1997, when a
propagating disturbance on a large area of the solar disc was
discovered. The process generating the EIT and Moreton waves has been
frequently discussed.
Aims.On May 2, 1998, a halo CME was observed related
to an EIT wave, a Moreton wave,
a X1 flare, radio emission sources, and dimmings. We studied this event
to find the relation between all these structures.
Methods.We use and co-align multi-wavelength observations and the online potential
field source surface (pfss) package.
Results.The observed EIT and Moreton waves present some brightenings that remain at
the same location. We relate the connectivity of the coronal potential
magnetic field to the stationary brightenings. We find that the areas where
the magnetic field lines have drastic jumps of connectivity are cospatial to
the stationary brightenings of the waves.
Conclusions.We conclude that the EIT and Moreton waves may be due to Joule heating
resulting from the generation of electric currents in the neighboring
area of the drastic
jumps of magnetic connectivity, while the magnetic field lines
are opening during a CME.
Key words: Sun: coronal mass ejections (CMEs) -- Sun: magnetic fields -- Sun: activity -- Sun: flares -- Sun: chromosphere -- Sun: corona
© ESO 2007

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