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 …

This paper deals with the temporal dynamics of solar flares. It gives a systematic description
of solar flare models and tries to link the observations to results of simulations. After a review …

We give an extensive overview of Doppler shift oscillations in hot active region loops
obtained with SUMER. The oscillations have been detected in loops sampled 50-100 arcsec …

On May 13, 1998 the EIT (Extreme ultraviolet Imaging Telescope) on board of SoHO (Solar
and Heliospheric Observatory) and TRACE (Transition Region And Coronal Explorer) …

We report the first observation at high spatial resolution of long-period quasi-periodic
pulsations (QPP) of X-ray radiation during solar flares, made possible with the Reuven …

Solar flare emission at X‐ray and extreme ultraviolet (EUV) energies can cause substantial
enhancements in the electron density in the Earth's lower ionosphere. It has now become …

We review the evolution of our knowledge and understanding of the eruptive (dynamic, two-
ribbon) flare phenomenon. Starting with the first observation of a white-light flare by …

We demonstrate that even in the absence of flares there are very often volumes of hot
plasma in the corona above active regions with temperatures in excess of 10 million …

One has to distinguish between two kinds of the gradual phase of flares:(1) a gradual phase
during which no energy is released so that we see only cooling after the impulsive phase (a …

In this study we perform a statistical study on, 8319 X-Ray solar flares observed with the
Hard X-Ray Burst Spectrometer (HXRBS) on the Solar Maximum Mission satellite (SMM) …