Coronal mass ejections (CMEs) were discovered in the early 1970s when space-borne
coronagraphs revealed that eruptions of plasma are ejected from the Sun. Today, it is known …

This article broadly reviews our knowledge of solar flares. There is a particular focus on their
global properties, as opposed to the microphysics such as that needed for magnetic …

In this paper, we study the temperature and density properties of multiple structural
components of coronal mass ejections (CMEs) using differential emission measure (DEM) …

This review on coronal mass ejections (CMEs) treats hydromagnetic issues posed by
observations, in order to relate CMEs to flares and prominence eruptions and to consider the …

Two-dimensional magnetohydrodynamic (MHD) simulation of a solar flare including the
effect of anisotropic heat conduction and chromospheric evaporation based on the magnetic …

The Sun is magnetically active and often produces eruptive events on different energetic
and temporal scales. Until recently, the upper limit of such events was unknown and …

We investigate the properties of two" classical" EUV Imaging Telescope (EIT) coronal waves.
The two source regions of the associated coronal mass ejections (CMEs) possess opposite …

We observed the fast coronal mass ejection (CME) of 1998 April 20 with the radioheliograph
at Nançay, France, between 164 and 432 MHz. Spectroscopic data were obtained between …

This paper will review the input of 65 years of radio observations to our understanding of
solar and solar–terrestrial physics. It is focussed on the radio observations of phenomena …

We have analyzed the coronal dimmings for seven fast (> 600 km/s) coronal mass ejections
(CMEs) occurring between 23 April and 9 May which were associated with flares from NOAA …