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Methods of Computational Topology for the Analysis of Dynamics of Active Regions of the Sun. / Makarenko, N.; Malkova, D.; Machin, M.; Knyazeva, I.; Makarenko, I.

в: Journal of Mathematical Sciences, Том 203, № 6, 01.01.2014, стр. 806-815.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Makarenko, N, Malkova, D, Machin, M, Knyazeva, I & Makarenko, I 2014, 'Methods of Computational Topology for the Analysis of Dynamics of Active Regions of the Sun', Journal of Mathematical Sciences, Том. 203, № 6, стр. 806-815. https://doi.org/10.1007/s10958-014-2170-y, https://doi.org/10.1007/s10958-014-2170-y

APA

Makarenko, N., Malkova, D., Machin, M., Knyazeva, I., & Makarenko, I. (2014). Methods of Computational Topology for the Analysis of Dynamics of Active Regions of the Sun. Journal of Mathematical Sciences, 203(6), 806-815. https://doi.org/10.1007/s10958-014-2170-y, https://doi.org/10.1007/s10958-014-2170-y

Vancouver

Makarenko N, Malkova D, Machin M, Knyazeva I, Makarenko I. Methods of Computational Topology for the Analysis of Dynamics of Active Regions of the Sun. Journal of Mathematical Sciences. 2014 Янв. 1;203(6):806-815. https://doi.org/10.1007/s10958-014-2170-y, https://doi.org/10.1007/s10958-014-2170-y

Author

Makarenko, N. ; Malkova, D. ; Machin, M. ; Knyazeva, I. ; Makarenko, I. / Methods of Computational Topology for the Analysis of Dynamics of Active Regions of the Sun. в: Journal of Mathematical Sciences. 2014 ; Том 203, № 6. стр. 806-815.

BibTeX

@article{e068472734894e6f9e23ef14a7e3fae4,
title = "Methods of Computational Topology for the Analysis of Dynamics of Active Regions of the Sun",
abstract = "The aim of this work is to diagnose pre-flare dynamics of magnetic fields in the active regions of the Sun on the HMI SDO magnetograms. We use a tool based on the methods of the geometry of random fields and computational topology. The results show that the proposed formalism allows one to find some precursors of major flares for practically significant time slots.",
author = "N. Makarenko and D. Malkova and M. Machin and I. Knyazeva and I. Makarenko",
year = "2014",
month = jan,
day = "1",
doi = "10.1007/s10958-014-2170-y",
language = "English",
volume = "203",
pages = "806--815",
journal = "Journal of Mathematical Sciences",
issn = "1072-3374",
publisher = "Springer Nature",
number = "6",

}

RIS

TY - JOUR

T1 - Methods of Computational Topology for the Analysis of Dynamics of Active Regions of the Sun

AU - Makarenko, N.

AU - Malkova, D.

AU - Machin, M.

AU - Knyazeva, I.

AU - Makarenko, I.

PY - 2014/1/1

Y1 - 2014/1/1

N2 - The aim of this work is to diagnose pre-flare dynamics of magnetic fields in the active regions of the Sun on the HMI SDO magnetograms. We use a tool based on the methods of the geometry of random fields and computational topology. The results show that the proposed formalism allows one to find some precursors of major flares for practically significant time slots.

AB - The aim of this work is to diagnose pre-flare dynamics of magnetic fields in the active regions of the Sun on the HMI SDO magnetograms. We use a tool based on the methods of the geometry of random fields and computational topology. The results show that the proposed formalism allows one to find some precursors of major flares for practically significant time slots.

UR - http://www.scopus.com/inward/record.url?scp=84922078967&partnerID=8YFLogxK

U2 - 10.1007/s10958-014-2170-y

DO - 10.1007/s10958-014-2170-y

M3 - Article

VL - 203

SP - 806

EP - 815

JO - Journal of Mathematical Sciences

JF - Journal of Mathematical Sciences

SN - 1072-3374

IS - 6

ER -

ID: 5811014