Magnetic Field and Density Models in the Zebra Source Region

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Magnetic Field and Density Models in the Zebra Source Region. / Yasnov, L.V. ; Karlický, Marian.

In: Solar Physics, Vol. 297, No. 10, 133, 13.10.2022.

Research output: Contribution to journal › Article › peer-review

BibTeX

@article{42f8a6563f4a44e9bdcfd78da8b7a4a1,

title = "Magnetic Field and Density Models in the Zebra Source Region",

abstract = "Using the double-plasma resonance model of solar radio zebras, we analyze five models of the magnetic field and density in the zebra source region. We present analytical relations of zebra-stripe frequencies depending on the gyro-harmonic number. By fitting of observed zebra-stripe frequencies using model frequencies, we find that the determined gyro-harmonic number and corresponding magnetic field depend on the model used. We show that all previously analyzed zebras, where the absolute value of the difference between neighboring zebra-stripe frequencies increases with respect to increasing frequency, can be well fitted by the model with exponential dependencies of the magnetic field and density or by the model with smaller gradients of both of these variables. Although these models give different results, their more sophisticated versions give more similar results. We also present the models that can fit the zebras, if observed, where the absolute value of the difference between neighboring zebra-stripe frequencies decreases with respect to increasing frequency. We check all these models by a fitting of the zebra-stripe frequencies observed in the 21 June 2011 zebra event. In one model, although it reasonably describes the conditions in the atmosphere above the active region, the fit of the observed zebra-stripe frequencies could not be made.",

keywords = "Dynamic spectrum, Dynamics, Flares, Radio bursts",

author = "L.V. Yasnov and Marian Karlick{\'y}",

note = "Publisher Copyright: {\textcopyright} 2022, The Author(s), under exclusive licence to Springer Nature B.V.",

year = "2022",

month = oct,

day = "13",

doi = "10.1007/s11207-022-02067-5",

language = "English",

volume = "297",

journal = "Solar Physics",

issn = "0038-0938",

publisher = "Springer Nature",

number = "10",

}

RIS

TY - JOUR

T1 - Magnetic Field and Density Models in the Zebra Source Region

AU - Yasnov, L.V.

AU - Karlický, Marian

PY - 2022/10/13

Y1 - 2022/10/13

N2 - Using the double-plasma resonance model of solar radio zebras, we analyze five models of the magnetic field and density in the zebra source region. We present analytical relations of zebra-stripe frequencies depending on the gyro-harmonic number. By fitting of observed zebra-stripe frequencies using model frequencies, we find that the determined gyro-harmonic number and corresponding magnetic field depend on the model used. We show that all previously analyzed zebras, where the absolute value of the difference between neighboring zebra-stripe frequencies increases with respect to increasing frequency, can be well fitted by the model with exponential dependencies of the magnetic field and density or by the model with smaller gradients of both of these variables. Although these models give different results, their more sophisticated versions give more similar results. We also present the models that can fit the zebras, if observed, where the absolute value of the difference between neighboring zebra-stripe frequencies decreases with respect to increasing frequency. We check all these models by a fitting of the zebra-stripe frequencies observed in the 21 June 2011 zebra event. In one model, although it reasonably describes the conditions in the atmosphere above the active region, the fit of the observed zebra-stripe frequencies could not be made.

AB - Using the double-plasma resonance model of solar radio zebras, we analyze five models of the magnetic field and density in the zebra source region. We present analytical relations of zebra-stripe frequencies depending on the gyro-harmonic number. By fitting of observed zebra-stripe frequencies using model frequencies, we find that the determined gyro-harmonic number and corresponding magnetic field depend on the model used. We show that all previously analyzed zebras, where the absolute value of the difference between neighboring zebra-stripe frequencies increases with respect to increasing frequency, can be well fitted by the model with exponential dependencies of the magnetic field and density or by the model with smaller gradients of both of these variables. Although these models give different results, their more sophisticated versions give more similar results. We also present the models that can fit the zebras, if observed, where the absolute value of the difference between neighboring zebra-stripe frequencies decreases with respect to increasing frequency. We check all these models by a fitting of the zebra-stripe frequencies observed in the 21 June 2011 zebra event. In one model, although it reasonably describes the conditions in the atmosphere above the active region, the fit of the observed zebra-stripe frequencies could not be made.

KW - Dynamic spectrum

KW - Dynamics

KW - Flares

KW - Radio bursts

UR - http://www.scopus.com/inward/record.url?scp=85139972355&partnerID=8YFLogxK

UR - https://www.mendeley.com/catalogue/e22c1989-eedd-3467-8ddb-e1c76cdd8585/

U2 - 10.1007/s11207-022-02067-5

DO - 10.1007/s11207-022-02067-5

M3 - Article

VL - 297

JO - Solar Physics

JF - Solar Physics

SN - 0038-0938

IS - 10

M1 - 133

ER -

ID: 99465699