This review covers fairly comprehensively experimental and theoretical research on the fine
structure of types zebra pattern (ZP) and fiber bursts (FB) in solar type II+ IV radio bursts. The …

Our high time resolution observations of individual pulses from the Crab pulsar show that
both the time and frequency signatures of the interpulse are distinctly different from those of …

Rare series of the slowly drifting structures observed during two solar flares (April 11, 2001
and March 18, 2003) in the 0.8-4.5 GHz frequency range are studied. Their time-frequency …

We have observed in the microwave range (with the radio spectrometer of the Huairu station
(Beijing, NAOC) around 3 GHz) the fine structure of solar radio bursts called zebra patterns …

ABSTRACT A zebra pattern (ZP) structure is the most intriguing fine structure on the dynamic
spectrograph of a solar microwave burst. On 2011 February 15, an X2. 2 flare event erupted …

A comparative analysis of two recent solar radio outbursts around 3 GHz with zebra
structures and fiber bursts in their dynamical radio spectra is carried out using all available …

The results of the first observations of a zebra pattern at frequencies around 5.6 GHz are
presented. The fine structures in the emission spectrum were recorded simultaneously by …

A specific combination of spectral fine structures in meter–decimeter dynamic spectra of
solar radio burst emission is reported in observations carried out at the Astrophysical …

We present new diagnostics of the solar flare reconnection, mainly based on the plasma
radio emission. We propose that the high-frequency (600-2000 MHz) slowly drifting …

We analyze a special kind of temporal fine structure in microwave radio emission for the 25
August 1999 solar flare observed by the PMO spectrometer over the range of 4.5–7.5 GHz …