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Modelling graph dynamics of flaring active regions using SDO/HMI data. / Lukyanov, A. D.; Knyazeva, I. S.

In: Journal of Physics: Conference Series, Vol. 798, No. 1, 012181, 07.03.2017.

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Lukyanov, AD & Knyazeva, IS 2017, 'Modelling graph dynamics of flaring active regions using SDO/HMI data', Journal of Physics: Conference Series, vol. 798, no. 1, 012181. https://doi.org/10.1088/1742-6596/798/1/012181

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Author

Lukyanov, A. D. ; Knyazeva, I. S. / Modelling graph dynamics of flaring active regions using SDO/HMI data. In: Journal of Physics: Conference Series. 2017 ; Vol. 798, No. 1.

BibTeX

@article{e27ea475d7d34053b8ec79ddceb07c41,
title = "Modelling graph dynamics of flaring active regions using SDO/HMI data",
abstract = "Large solar flares define parameters of space weather near the Earth and normal operation of spacecrafts substantially depends on the cosmic particles flux of solar wind. Therefore, search for large flares predictors is an important problem. We propose to approximate topology of the magnetic field of active region by graph, whose vertices are minima and maxima of a scalar field and edges form a so-called critical net. Localization and number of critical points change during the process of evolution and, therefore, it is possible to track dynamic regimes of active region by considering dynamics of graphs. Numerical characteristic of the critical net is a spectrum of eigenvalues of its discrete Laplacian. We present examples which show that, apparently, Laplacian spectrum is closely related to flaring activity. It will allow us to use critical net in prognostic systems for prediction of large solar flares.",
author = "Lukyanov, {A. D.} and Knyazeva, {I. S.}",
year = "2017",
month = mar,
day = "7",
doi = "10.1088/1742-6596/798/1/012181",
language = "English",
volume = "798",
journal = "Journal of Physics: Conference Series",
issn = "1742-6588",
publisher = "IOP Publishing Ltd.",
number = "1",

}

RIS

TY - JOUR

T1 - Modelling graph dynamics of flaring active regions using SDO/HMI data

AU - Lukyanov, A. D.

AU - Knyazeva, I. S.

PY - 2017/3/7

Y1 - 2017/3/7

N2 - Large solar flares define parameters of space weather near the Earth and normal operation of spacecrafts substantially depends on the cosmic particles flux of solar wind. Therefore, search for large flares predictors is an important problem. We propose to approximate topology of the magnetic field of active region by graph, whose vertices are minima and maxima of a scalar field and edges form a so-called critical net. Localization and number of critical points change during the process of evolution and, therefore, it is possible to track dynamic regimes of active region by considering dynamics of graphs. Numerical characteristic of the critical net is a spectrum of eigenvalues of its discrete Laplacian. We present examples which show that, apparently, Laplacian spectrum is closely related to flaring activity. It will allow us to use critical net in prognostic systems for prediction of large solar flares.

AB - Large solar flares define parameters of space weather near the Earth and normal operation of spacecrafts substantially depends on the cosmic particles flux of solar wind. Therefore, search for large flares predictors is an important problem. We propose to approximate topology of the magnetic field of active region by graph, whose vertices are minima and maxima of a scalar field and edges form a so-called critical net. Localization and number of critical points change during the process of evolution and, therefore, it is possible to track dynamic regimes of active region by considering dynamics of graphs. Numerical characteristic of the critical net is a spectrum of eigenvalues of its discrete Laplacian. We present examples which show that, apparently, Laplacian spectrum is closely related to flaring activity. It will allow us to use critical net in prognostic systems for prediction of large solar flares.

UR - http://www.scopus.com/inward/record.url?scp=85016242137&partnerID=8YFLogxK

U2 - 10.1088/1742-6596/798/1/012181

DO - 10.1088/1742-6596/798/1/012181

M3 - Article

AN - SCOPUS:85016242137

VL - 798

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

SN - 1742-6588

IS - 1

M1 - 012181

ER -

ID: 9327480