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相关论文: Zebra stripes with high gyro-harmonic numbers

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Fine structures of radio bursts play an important role in diagnostics of the solar flare plasma. Among them the zebras, which are prevalently assumed to be generated by the double plasma resonance instability, belong to the most important.…

太阳与恒星天体物理 · 物理学 2019-04-11 Leonid V. Yasnov , Jan Benáček , Marian Karlický

Context. The zebra patterns observed in solar radio emission are very important for are plasma diagnostics. The most promising model of these patterns is based on double plasma resonance instability, which generates upper-hybrid waves,…

太阳与恒星天体物理 · 物理学 2017-02-08 Jan Benáček , Marian Karlický , Leonid V. Yasnov

The double plasma resonance (DPR) instability plays a basic role in the generation of solar radio zebras. In the plasma, consisting of the loss-cone type distribution of hot electrons and much denser and colder background plasma, this…

等离子体物理 · 物理学 2018-03-28 Jan Benáček , Marian Karlický

Zebras were observed not only in the solar radio emission but also in radio emissions of Jupiter and Crab Nebula pulsar. In their models, growth rates of the electrostatic waves play an important role. Considering the plasma composed from…

等离子体物理 · 物理学 2019-08-16 Jan Benáček , Marian Karlický

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…

太阳与恒星天体物理 · 物理学 2020-02-05 L. V. Yasnov , G. P. Chernov

We estimated the brightness temperature of radio zebras (zebra pattern -- ZP), considering that ZPs are generated in loops having an exponential density profile in their cross-section. We took into account that when in plasma there is a…

太阳与恒星天体物理 · 物理学 2017-10-31 Leonid V. Yasnov , Jan Benáček , Marian Karlický

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…

太阳与恒星天体物理 · 物理学 2015-06-11 Sijie Yu , Yihua Yan , Baolin Tan

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…

太阳与恒星天体物理 · 物理学 2011-09-28 A. T. Altyntsev , S. V. Lesovoi , N. S. Meshalkina , R. A. Sych , Y. Yan

Giant pulses (GPs) are extremely bright individual pulses of radio pulsar. In microbursts of Crab pulsar, which is an active GP emitter, zebra-pattern-like spectral structures are observed, which are reminiscent of the `zebra bands' that…

高能天体物理现象 · 物理学 2018-11-28 Weiyang Wang , Jiguang Lu , Songbo Zhang , Xuelei Chen , Rui Luo , Renxin Xu

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…

高能天体物理现象 · 物理学 2026-02-20 Mikhail V. Medvedev

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…

太阳与恒星天体物理 · 物理学 2017-04-11 G. P. Chernov , V. V. Fomichev , R. A. Sych

Sausage modes that are axisymmetric fast magnetoacoustic oscillations of solar coronal loops are characterized by variation of the plasma density and magnetic field, and hence cause time variations of the electron plasma frequency and…

太阳与恒星天体物理 · 物理学 2016-08-17 Sijie Yu , V. M. Nakariakov , Yihua Yan

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.…

太阳与恒星天体物理 · 物理学 2018-07-25 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…

太阳与恒星天体物理 · 物理学 2015-06-18 Baolin Tan , Chengming Tan , Yin Zhang , H. Meszarosova , M. Karlicky

The microwave radio dynamic spectra of the Crab pulsar interpulse contain fine structures represented via narrowband quasiharmonic stripes. The pattern significantly constrains any potential emission mechanism. Similar to the zebra patterns…

高能天体物理现象 · 物理学 2024-01-31 M. Labaj , J. Benáček , M. Karlický

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…

地球与行星天体物理 · 物理学 2015-06-11 A. A. Kuznetsov , V. G. Vlasov

The laser interaction with an electron-positron-ion mixed plasma is studied, from the perspective of the associated high-order harmonic generation. For an idealized mixed plasma which is assumed with a sharp plasma-vacuum interface and…

等离子体物理 · 物理学 2021-01-20 W. L. Zhang , T. Grismayer , K. M. Schoeffler , R. A. Fonseca , L. O. Silva

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.…

太阳与恒星天体物理 · 物理学 2017-11-22 G. P. Chernov , V. V. Fomichev , Y. Yan , B. Tan , Ch. Tan , Q. Fu

Zebra-like patterns have been observed in the electron cyclotron emission spectra from strongly nonequilibrium plasma confined in a table-top mirror magnetic trap. The analysis of the experimental data suggests that the formation of…

等离子体物理 · 物理学 2020-06-16 M. E. Viktorov , A. G. Shalashov , E. D. Gospodchikov , N. Yu. Semin , S. V. Golubev

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…

太阳与恒星天体物理 · 物理学 2016-03-15 Gennady Chernov
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