Incoherent solar radio radiation comes from the free-free, gyroresonance, and
gyrosynchrotron emission mechanisms. Free-free is primarily produced from Coulomb …

The Sun is the nearest stellar and astrophysical laboratory, available for detailed studies in
several fields of physics and astronomy. It is a sphere of hot gas with a complex and highly …

The Kilpisjärvi Atmospheric Imaging Receiver Array (KAIRA) is a dual array of
omnidirectional VHF radio antennas located near Kilpisjärvi, Finland. It is operated by the …

This paper examines long-term (more than four solar cycles) temporal and spatial
fluctuations in the solar rotation by investigating radio-emission escapes from various layers …

ADAHELI (ADvanced Astronomy for HELIophysics) is a small-class (500kg) low-budget (50
MEuro) satellite mission for the study of the solar photosphere and the chromosphere and …

In solar physics, it is a big challenge to measure the magnetic fields directly from
observations in the upper solar atmosphere, including the chromosphere and corona. Radio …

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 solar radio bursts are the results of solar flares take place on the surface of the Sun.
Some of them could reach the surface of the Earth and can be detected by the ground base …

The present work is an effort to investigate possible radial variations in the solar coronal
rotation by analysing the solar radio emission data at 15 different frequencies (275–1755 …

We use a numerical code called PAKALMPI to compute synthetic spectra of the solar
emission in quiet conditions at millimeter, sub-millimeter, and infrared wavelengths …