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 …

Abstract The Atacama Large Millimeter/submillimeter Array (ALMA) is a new powerful tool for
observing the Sun at high spatial, temporal, and spectral resolution. These capabilities can …

This review discusses the complementary relationship between radio and hard X-ray
observations of the Sun using primarily results from the era of the Reuven Ramaty High …

The optical and near-ultraviolet (NUV) continuum radiation in M-dwarf flares is thought to be
the impulsive response of the lower stellar atmosphere to magnetic energy release and …

We discuss the implications of the first systematic observations of solar flares at
submillimeter wavelengths, defined here as observing wavelengths shorter than 3 mm …

We investigate the origin of the increasing spectra observed at submillimeter wavelengths
detected in the flare on 2 November 2003 starting at 17: 17 UT. This flare, classified as an …

Mobile communication towers represent a relatively new but growing contributor to the total
radio-leakage associated with planet Earth. We investigate the overall power contribution of …

The 5 July 2012 solar flare SOL2012-07-05T11: 44 (11: 39–11: 49 UT) with an increasing
millimeter spectrum between 93 and 140 GHz is considered. We use space and ground …

In this paper, we present a tutorial review which was presented at the first Advanced School
on Space Environment (ASSE 2004). We first describe the basics of radioastronomy …

Solar flares observed in the 200–400 GHz radio domain may exhibit a slowly varying and
time-extended component which follows a short (few minutes) impulsive phase and can last …