We present here a review of observations and the current theories that attempt to explain
coronal EIT waves. EIT waves were first observed by SOHO-EIT in 1996. Since then, careful …

We present the extension of the magnetic breakout model for CME initiation to a fully three-
dimensional, spherical geometry. Given the increased complexity of the dynamic magnetic …

EIT waves and extreme-ultraviolet (EUV) dimmings attract particular attention as they
frequently accompany Coronal Mass Ejections (CMEs). We present several examples of EIT …

During its 2000 January flight, the Flare Genesis Experiment observed the gradual
emergence of a bipolar active region, by recording a series of high-resolution photospheric …

We present three methods for deriving the velocity field in magnetized regions of the Sun's
photosphere. As a preliminary step, we introduce a Fourier-based local correlation tracking …

We report two sympathetic solar eruptions including a partial and a full flux rope eruption in
a quadrupolar magnetic region where a large and a small filament resided above the middle …

The solar atmosphere being magnetic in nature, the understanding of the structure and
evolution of the magnetic field in different regions of the solar atmosphere has been an …

We compute the magnetic helicity injected by transient photospheric horizontal flows in six
solar active regions associated with halo coronal mass ejections (CMEs) that produced …

We compare the" magnetic breakout" model for coronal mass ejections (CMEs) with
observed general properties of CMEs by analyzing in detail recent high-resolution MHD …

The first evidence of transverse oscillations of a multistranded loop with growing amplitudes
and internal coupling observed by the Atmospheric Imaging Assembly on board the Solar …