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The so-called zebra structures in radio dynamic spectra, specifically their frequencies and frequency drifts of emission stripes, contain information on the plasma parameters in the coronal part of flare loops. This paper presents…

Solar and Stellar Astrophysics · Physics 2011-09-28 A. T. Altyntsev , S. V. Lesovoi , N. S. Meshalkina , R. A. Sych , Y. Yan

We analyze complex zebra patterns and fiber bursts during type-IV solar radio bursts on August 1, 2010. It was shown that all of the main details of sporadic zebra patterns can be explained within the model of zebra patterns and fiber…

Solar and Stellar Astrophysics · Physics 2018-12-12 G. P. Chernov , V. V. Fomichev , R. A. Sych

The publications of the last three years concerning the study of the most intriguing fine structure in type IV solar radio bursts, zebra pattern (ZP), are surveyed. The main attention is paid to new observations, irrespective of whether a…

Solar and Stellar Astrophysics · Physics 2016-03-15 Gennady Chernov

Discussion about the nature of zebra-structure (ZS) in the type IV radio bursts continues, despite the ten proposed models. First of all, this is due to the wide variety of stripes in each new phenomenon, when the explanation of all the…

Solar and Stellar Astrophysics · Physics 2017-04-11 G. P. Chernov , V. V. Fomichev , R. A. Sych

In the literature, discussion continues about the nature of the zebra structure (ZS) in type IV radio bursts, and understanding even the most extended mechanism associated with double plasma resonance has been improved in series of works.…

Solar and Stellar Astrophysics · Physics 2018-07-25 G. P. Chernov

We investigate the formation of zebra-like fine spectral structures (consisting of several parallel bands in the dynamic spectrum) in the Jovian broadband kilometric radiation; such radio bursts were observed by Cassini in 2000/2001. We…

Earth and Planetary Astrophysics · Physics 2015-06-11 A. A. Kuznetsov , V. G. Vlasov

The reason for the occurrence of different elements of the fine structure of solar radio bursts in the decimeter and centimeter wavelength ranges has been determined based on all available data from terrestrial and satellite observations.…

Solar and Stellar Astrophysics · Physics 2017-11-22 G. P. Chernov , V. V. Fomichev , Y. Yan , B. Tan , Ch. Tan , Q. Fu

The analysis of the spectral characteristics of the burst radio emission on June 21, 2011 was carried out on the basis of an improved methodology for determining harmonic numbers for the corresponding stripes of the zebra structure. By…

Solar and Stellar Astrophysics · Physics 2020-02-05 L. V. Yasnov , G. P. Chernov

The microwave zebra pattern (ZP) is the most interesting, intriguing, and complex spectral structure frequently observed in solar flares. A comprehensive statistical study will certainly help us to understand the formation mechanism, which…

Solar and Stellar Astrophysics · Physics 2015-06-18 Baolin Tan , Chengming Tan , Yin Zhang , H. Meszarosova , M. Karlicky

Zebra pattern structure (ZP) is the most intriguing fine structure on the dynamic spectrograph of solar microwave burst. On 15 February 2011, there erupts an X2.2 flare event on the solar disk, it is the first X-class flare since the solar…

Solar and Stellar Astrophysics · Physics 2015-05-30 Baolin Tan , Yihua Yan , Chengming Tan , Robert Sych , Guannan Gao

The unusual radio burst of May 29, 2003 connected with the M1.5 flare in AR 10368 has been analyzed. It was observed by the Solar Broadband Radio Spectrometer (SBRS/Huairou station, Beijing) in the 5.2-7.6 GHz range. It proved to be only…

Solar and Stellar Astrophysics · Physics 2015-06-03 G. P. Chernov , R. A. Sych , N. S. Meshalkina , Y. Yan , C. Tan

A theory of the spectral "zebra" pattern of the Crab pulsar's high-frequency interpulse (HFIP) radio emission is developed. The observed emission bands are interference maxima caused by multiple ray propagation through the pulsar…

High Energy Astrophysical Phenomena · Physics 2026-02-20 Mikhail V. Medvedev

Quasi-periodic wiggles of microwave zebra pattern structures with period range from about 0.5 s to 1.5 s are found in a X-class solar flare on 2006 December 13 at the 2.6-3.8 GHz with the Chinese Solar Broadband Radio Spectrometer…

Solar and Stellar Astrophysics · Physics 2015-06-17 Sijie Yu , V. M. Nakariakov , L. A. Selzer , Baolin Tan , Yihua Yan

Microwave emission with spectral zebra pattern structures (ZPs) is observed frequently in solar flares and the Crab pulsar. The previous observations show that ZP is only a structure overlapped on the underlying broadband continuum with…

Solar and Stellar Astrophysics · Physics 2015-06-22 Baolin Tan , Chengming Tan , Yin Zhang , Jing Huang , Hana Meszarosova , Marian Karlicky , Yihua Yan

It is generally considered that the emission of microwave zebra pattern (ZP) structures requires high density and high temperatures, which is similar to the situation of the flaring region where primary energy releases. Therefore, the…

Solar and Stellar Astrophysics · Physics 2015-06-11 Sijie Yu , Yihua Yan , Baolin Tan

The measurement of positions and sizes of radio sources in the observations of solar radio spectral fine structures in an M6.5 flare on April 11, 2013 were observed simultaneously by several radio instruments at four different…

Solar and Stellar Astrophysics · Physics 2016-02-17 Gennady Chernov , Robert Sych , Baolin Tan , Yihua Yan , Chengming Tan , Qijun Fu , Marian Karlicky , Valery Fomichev

Coherent radio emission mechanism of solar radio bursts is one of the most complicated and controversial topics in solar physics. To clarify the mechanism(s) of different types of solar radio bursts, (radio) wave excitation by energetic…

Solar and Stellar Astrophysics · Physics 2025-02-07 Xiaowei Zhou , Patricio Munoz , Jan Benacek , Lijie Zhang , Dejin Wu , Ling Chen , Zongjun Ning , Joerg Buechner

The polarization characteristics of zebra patterns (ZPs) in type IV solar bursts were studied. We analyzed 21 ZP events observed by the Assembly of Metric-band Aperture Telescope and Real-time Analysis System between 2010 and 2015 and…

Solar and Stellar Astrophysics · Physics 2017-07-04 Kazutaka Kaneda , H. Misawa , K. Iwai , F. Tsuchiya , T. Obara , Y. Katoh , S. Masuda

Radiobursts exibiting fine structure observed over two years during the rising phase of Cycle 24 by the SBRS are analyzed. In five events zebra structure, various fiber bursts and fast pulsations were observed. Events on 15 and 24 February…

Solar and Stellar Astrophysics · Physics 2015-06-22 Gennady Chernov , Valery Fomichev , Baolin Tan , Yihua Yan , Chengming Tan , Qijun Fu

The modulation of the intensity of microwave emission from a plasma slab caused by a standing linear kink fast magnetoacoustic wave is considered. The slab is stretched along a straight magnetic field, and can represent, for example, a…

Solar and Stellar Astrophysics · Physics 2023-02-22 T. I. Kaltman , E. G. Kupriyanova
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