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Topology of Magnetic Fields from MDI Data: Background Field. / Knyazeva, I. S.; Makarenko, N. G.; Karimova, L. M.

In: Astronomy Reports, Vol. 54, No. 8, 2010, p. 747-755.

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

Harvard

Knyazeva, IS, Makarenko, NG & Karimova, LM 2010, 'Topology of Magnetic Fields from MDI Data: Background Field', Astronomy Reports, vol. 54, no. 8, pp. 747-755. https://doi.org/10.1134/S1063772910080081

APA

Knyazeva, I. S., Makarenko, N. G., & Karimova, L. M. (2010). Topology of Magnetic Fields from MDI Data: Background Field. Astronomy Reports, 54(8), 747-755. https://doi.org/10.1134/S1063772910080081

Vancouver

Knyazeva IS, Makarenko NG, Karimova LM. Topology of Magnetic Fields from MDI Data: Background Field. Astronomy Reports. 2010;54(8):747-755. https://doi.org/10.1134/S1063772910080081

Author

Knyazeva, I. S. ; Makarenko, N. G. ; Karimova, L. M. / Topology of Magnetic Fields from MDI Data: Background Field. In: Astronomy Reports. 2010 ; Vol. 54, No. 8. pp. 747-755.

BibTeX

@article{f42f1559312841edb77c9d8ba433c34f,
title = "Topology of Magnetic Fields from MDI Data: Background Field",
abstract = "A quantitative description of the geometry and topology of the magnetic field of the Sun is given in terms ofMinkowski functionals: the Euler characteristic and the perimeter of excursion sets for specified levels. Methods of mathematical morphology are applied to background fragments of magnetograms for the entire solar disk. The results obtained show that the topological characteristics of the background field are stable in time and correspond to log-normal, intermittent random fields.",
author = "Knyazeva, {I. S.} and Makarenko, {N. G.} and Karimova, {L. M.}",
year = "2010",
doi = "10.1134/S1063772910080081",
language = "English",
volume = "54",
pages = "747--755",
journal = "Astronomy Reports",
issn = "1063-7729",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "8",

}

RIS

TY - JOUR

T1 - Topology of Magnetic Fields from MDI Data: Background Field

AU - Knyazeva, I. S.

AU - Makarenko, N. G.

AU - Karimova, L. M.

PY - 2010

Y1 - 2010

N2 - A quantitative description of the geometry and topology of the magnetic field of the Sun is given in terms ofMinkowski functionals: the Euler characteristic and the perimeter of excursion sets for specified levels. Methods of mathematical morphology are applied to background fragments of magnetograms for the entire solar disk. The results obtained show that the topological characteristics of the background field are stable in time and correspond to log-normal, intermittent random fields.

AB - A quantitative description of the geometry and topology of the magnetic field of the Sun is given in terms ofMinkowski functionals: the Euler characteristic and the perimeter of excursion sets for specified levels. Methods of mathematical morphology are applied to background fragments of magnetograms for the entire solar disk. The results obtained show that the topological characteristics of the background field are stable in time and correspond to log-normal, intermittent random fields.

U2 - 10.1134/S1063772910080081

DO - 10.1134/S1063772910080081

M3 - Article

VL - 54

SP - 747

EP - 755

JO - Astronomy Reports

JF - Astronomy Reports

SN - 1063-7729

IS - 8

ER -

ID: 5564970