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 …

This paper presents the latest observations from the newly built solar radio spectrograph at
the Chashan Solar Observatory. On July 18, 2016, the spectrograph records a solar spike …

Spectral observations with high temporal and frequency resolution are of great significance
for studying the fine structures of solar radio bursts. In addition, it is helpful to understand the …

Solar radio bursts can be used to study the properties of solar activities and the underlying
coronal conditions on the basis of the present understanding of their emission mechanisms …

Context. Narrow-band bursts appear on dynamic spectra from microwave to decametric
frequencies as fine structures with very small duration and bandwidth. They are believed to …

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 solar radio signal that can be received by the ground-based telescopes covers a wide
frequency range, allowing us to monitor the complex physical processes occurred from the …

Real-time detection of solar radio bursts is crucial in solar physics research and space
weather forecasting. However, current research on the automatic detection of solar radio …

Solar radio spikes are narrowband, short duration radio bursts. They are excited by the
energetic electrons accelerated during small scale magnetic reconnections. Spikes play an …

Aims. We study the characteristics of intermediate drift bursts (fibers) embedded in a large
type-IV event. Methods. We used high-sensitivity, low-noise dynamic spectra obtained with …