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 ground-based and satellite data (SOHO, TRACE, RHESSI). The latest theoretical models of the zebra pattern are critically discussed. New data on microwave zebra structures and fiber bursts suggests that they are analogous to similar structures observed at meter wavelengths. It was discovered that in the 2,6–3,8 GHz frequency band more than 34 zebra stripes can appear simultaneously, and some isolated fiber bursts can continuously be transformed into zebra stripes. This fact indicates a single origin for both structures. The zebra pattern was observed when the signs ...
A very general dynamic model for the interpretation of Zebra patterns (Mollwo, 1983) traces back the...
We report the first systematic analysis of zebra–like fine spectral structures in the decametric fre...
681 solar radio events observed by the Ondřejov 0.8-2.0 GHz radiospectrograph during 1992-2000 are a...
Abstract This review covers the most recent experimental results and theoretical re-search on zebra ...
We have observed in the microwave range (with the radio spectrometer of the Huairu station (Beijing,...
Context. Radio bursts with fine structures are used in diagnostics of solar flare plasmas, of which ...
Context. During solar flares several types of radio bursts are observed. The fine striped structures...
Context. Radio bursts and their fine structures are an integral part of solar flares. Fine structure...
The results of the first observations of a zebra pattern at frequencies around 5.6 GHz are presented...
Context. The unusual radio burst of May 29, 2003 connected with the M1.5 flare in AR 10368 has been ...
Several complex uncommon zebra patterns in meter/ decimeter and microwave range are shown. It is dif...
We discuss a source model for the origin of solar type IV burst fine structures (FS) using the data ...
Context. Solar radio zebras are used in diagnostics of solar flare plasmas and it is of great import...
Aims. We aim to answer the question how waves with plasma density variations affect the radio contin...
The Ondřejov radiospectrograph operating in the 0.8-2.0 GHz frequency range recorded in recent years...
A very general dynamic model for the interpretation of Zebra patterns (Mollwo, 1983) traces back the...
We report the first systematic analysis of zebra–like fine spectral structures in the decametric fre...
681 solar radio events observed by the Ondřejov 0.8-2.0 GHz radiospectrograph during 1992-2000 are a...
Abstract This review covers the most recent experimental results and theoretical re-search on zebra ...
We have observed in the microwave range (with the radio spectrometer of the Huairu station (Beijing,...
Context. Radio bursts with fine structures are used in diagnostics of solar flare plasmas, of which ...
Context. During solar flares several types of radio bursts are observed. The fine striped structures...
Context. Radio bursts and their fine structures are an integral part of solar flares. Fine structure...
The results of the first observations of a zebra pattern at frequencies around 5.6 GHz are presented...
Context. The unusual radio burst of May 29, 2003 connected with the M1.5 flare in AR 10368 has been ...
Several complex uncommon zebra patterns in meter/ decimeter and microwave range are shown. It is dif...
We discuss a source model for the origin of solar type IV burst fine structures (FS) using the data ...
Context. Solar radio zebras are used in diagnostics of solar flare plasmas and it is of great import...
Aims. We aim to answer the question how waves with plasma density variations affect the radio contin...
The Ondřejov radiospectrograph operating in the 0.8-2.0 GHz frequency range recorded in recent years...
A very general dynamic model for the interpretation of Zebra patterns (Mollwo, 1983) traces back the...
We report the first systematic analysis of zebra–like fine spectral structures in the decametric fre...
681 solar radio events observed by the Ondřejov 0.8-2.0 GHz radiospectrograph during 1992-2000 are a...