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Magnetic Field Topology by MDI Data: Active Region. / Makarenko, N. G.; Knyazeva, I. S.; Karimova, L.M.

в: Astronomy Letters, Том 38, № 8, 2012, стр. 531-542.

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

Harvard

Makarenko, NG, Knyazeva, IS & Karimova, LM 2012, 'Magnetic Field Topology by MDI Data: Active Region', Astronomy Letters, Том. 38, № 8, стр. 531-542. https://doi.org/10.1134/S1063773712070055

APA

Makarenko, N. G., Knyazeva, I. S., & Karimova, L. M. (2012). Magnetic Field Topology by MDI Data: Active Region. Astronomy Letters, 38(8), 531-542. https://doi.org/10.1134/S1063773712070055

Vancouver

Makarenko NG, Knyazeva IS, Karimova LM. Magnetic Field Topology by MDI Data: Active Region. Astronomy Letters. 2012;38(8):531-542. https://doi.org/10.1134/S1063773712070055

Author

Makarenko, N. G. ; Knyazeva, I. S. ; Karimova, L.M. / Magnetic Field Topology by MDI Data: Active Region. в: Astronomy Letters. 2012 ; Том 38, № 8. стр. 531-542.

BibTeX

@article{bb57e5c8f5e24e9799e823a4cac39810,
title = "Magnetic Field Topology by MDI Data: Active Region",
abstract = "Themain purpose of this paper is to describe the evolution of the magnetic field of active regions of the Sun in the context of Minkowski functionals: the Euler characteristic and perimeter calculated on the excursion set for a specified level. Themethods of geometry of random fields was applied to the MDI SOHO magnetogram, containing flaring active regions. The results demonstrated that morphological functional tracked the dynamic scenarios of the magnetic fields preceded by flares or accompanying them.",
author = "Makarenko, {N. G.} and Knyazeva, {I. S.} and L.M. Karimova",
year = "2012",
doi = "10.1134/S1063773712070055",
language = "English",
volume = "38",
pages = "531--542",
journal = "Astronomy Letters",
issn = "1063-7737",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "8",

}

RIS

TY - JOUR

T1 - Magnetic Field Topology by MDI Data: Active Region

AU - Makarenko, N. G.

AU - Knyazeva, I. S.

AU - Karimova, L.M.

PY - 2012

Y1 - 2012

N2 - Themain purpose of this paper is to describe the evolution of the magnetic field of active regions of the Sun in the context of Minkowski functionals: the Euler characteristic and perimeter calculated on the excursion set for a specified level. Themethods of geometry of random fields was applied to the MDI SOHO magnetogram, containing flaring active regions. The results demonstrated that morphological functional tracked the dynamic scenarios of the magnetic fields preceded by flares or accompanying them.

AB - Themain purpose of this paper is to describe the evolution of the magnetic field of active regions of the Sun in the context of Minkowski functionals: the Euler characteristic and perimeter calculated on the excursion set for a specified level. Themethods of geometry of random fields was applied to the MDI SOHO magnetogram, containing flaring active regions. The results demonstrated that morphological functional tracked the dynamic scenarios of the magnetic fields preceded by flares or accompanying them.

U2 - 10.1134/S1063773712070055

DO - 10.1134/S1063773712070055

M3 - Article

VL - 38

SP - 531

EP - 542

JO - Astronomy Letters

JF - Astronomy Letters

SN - 1063-7737

IS - 8

ER -

ID: 5565061