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 …

Basic topology of twisted magnetic configurations in solar flares ADS Classic is now deprecated.
It will be completely retired in October 2019. This page will automatically redirect to the new …

Mounting observational evidence of the emergence of twisted magnetic flux tubes through
the photosphere have now been published. Such flux tubes, formed by the solar dynamo …

We analyze the physical mechanisms that form a three-dimensional coronal flux rope and
later cause its eruption. This is achieved by a zero-β magnetohydrodynamic (MHD) …

A sudden depletion or intensity" dimming" of the X-ray corona sometimes accompanies a
solar eruptive flare or coronal mass ejection (CME). We have identified a dimming that …

It is now commonly accepted that prominence plasma is supported in magnetic dips, in
particular in twisted flux-tubes. But present two-dimensional models are unable to explain …

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 …

To determine the relationship between transient coronal (soft X-ray or EUV) sigmoids and
erupting flux ropes, we analyse four events in which a transient sigmoid could be associated …

We study dynamical consequences of the kink instability of a twisted coronal flux rope, using
the force-free coronal loop model by [CITE] as the initial condition in ideal-MHD simulations …

A coronal mass ejection (CME), strictly speaking, is a phenomenon observed via a white‐
light coronal imager. In addition to coronagraphs, a wide variety of other instruments provide …