The structure of the upper solar atmosphere, on all observable scales, is intimately governed
by the magnetic field. The same holds for a variety of solar phenomena that constitute solar …

Radio bursts provide important diagnostics of energetic phenomena of the Sun. In particular,
bursts in decimetric and metric wavelengths probe the physical conditions and the energy …

Fiber bursts are a type of fine structure that frequently occurs in solar flares. Although
observations and theory of fiber bursts have been studied for decades, their microphysical …

The reconfiguration of the magnetic field during and after a coronal mass ejection (CME)
may be accompanied by radio emission from non-thermal electrons. In particular, stationary …

We have studied a complex metric radio event that originated in a compact flare, observed
with the ARTEMIS-JLS radiospectrograph on February 12, 2010. The event was associated …

An investigation of the generation mechanism for stripes-pattern radio spectra is important
for an understanding of the dynamics of non-thermal electrons in several astronomical …

We present results of observations of Type IV burst with unusual high polarization equalled
in maximum phase about 100%. This burst was registered both by URAN-2 and NDA radio …

Analysis of solar transients for space weather forecasting Page 1 Analysis of solar transients for
space weather forecasting by Khaled Alielden Darwish Supervisors: Dr. Youra Toryan Prof. Huw …