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Evolution of the magnetic fields of solar flare active regions from the geometry and topology of HMI/SDO magnetograms. / Knyazeva, I. S.; Makarenko, N. G.

In: Astronomy Reports, Vol. 58, No. 3, 2014, p. 145-155.

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

Harvard

Knyazeva, IS & Makarenko, NG 2014, 'Evolution of the magnetic fields of solar flare active regions from the geometry and topology of HMI/SDO magnetograms', Astronomy Reports, vol. 58, no. 3, pp. 145-155. https://doi.org/10.1134/S1063772914030044

APA

Knyazeva, I. S., & Makarenko, N. G. (2014). Evolution of the magnetic fields of solar flare active regions from the geometry and topology of HMI/SDO magnetograms. Astronomy Reports, 58(3), 145-155. https://doi.org/10.1134/S1063772914030044

Vancouver

Knyazeva IS, Makarenko NG. Evolution of the magnetic fields of solar flare active regions from the geometry and topology of HMI/SDO magnetograms. Astronomy Reports. 2014;58(3):145-155. https://doi.org/10.1134/S1063772914030044

Author

Knyazeva, I. S. ; Makarenko, N. G. / Evolution of the magnetic fields of solar flare active regions from the geometry and topology of HMI/SDO magnetograms. In: Astronomy Reports. 2014 ; Vol. 58, No. 3. pp. 145-155.

BibTeX

@article{af1faa66eabb4c88b719dd7e0081aaa6,
title = "Evolution of the magnetic fields of solar flare active regions from the geometry and topology of HMI/SDO magnetograms",
abstract = "The testing and development of topological approaches to the analysis of solar magnetic fields are considered. A technique based on the geometry of random fields, mathematical morphology and topology, and scale-space analyses are applied to describe and diagnose the pre-flare dynamics of the magnetic fields of solar active regions using HMI/SDO magnetograms. The results show that this formalism can be used to diagnose pre-flare dynamics over time intervals that are of practical interest.",
author = "Knyazeva, {I. S.} and Makarenko, {N. G.}",
year = "2014",
doi = "10.1134/S1063772914030044",
language = "English",
volume = "58",
pages = "145--155",
journal = "Astronomy Reports",
issn = "1063-7729",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "3",

}

RIS

TY - JOUR

T1 - Evolution of the magnetic fields of solar flare active regions from the geometry and topology of HMI/SDO magnetograms

AU - Knyazeva, I. S.

AU - Makarenko, N. G.

PY - 2014

Y1 - 2014

N2 - The testing and development of topological approaches to the analysis of solar magnetic fields are considered. A technique based on the geometry of random fields, mathematical morphology and topology, and scale-space analyses are applied to describe and diagnose the pre-flare dynamics of the magnetic fields of solar active regions using HMI/SDO magnetograms. The results show that this formalism can be used to diagnose pre-flare dynamics over time intervals that are of practical interest.

AB - The testing and development of topological approaches to the analysis of solar magnetic fields are considered. A technique based on the geometry of random fields, mathematical morphology and topology, and scale-space analyses are applied to describe and diagnose the pre-flare dynamics of the magnetic fields of solar active regions using HMI/SDO magnetograms. The results show that this formalism can be used to diagnose pre-flare dynamics over time intervals that are of practical interest.

U2 - 10.1134/S1063772914030044

DO - 10.1134/S1063772914030044

M3 - Article

VL - 58

SP - 145

EP - 155

JO - Astronomy Reports

JF - Astronomy Reports

SN - 1063-7729

IS - 3

ER -

ID: 5811357