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Model of poleward magnetic field streams from sunspot butterflies. / Zolotova, N.V.; Ponyavin, D.I.

In: Proceedings of the International Astronomical Union, Vol. 8, No. S294, 2013, p. 87-92.

Research output: Contribution to journal › Conference article

Harvard

Zolotova, NV & Ponyavin, DI 2013, 'Model of poleward magnetic field streams from sunspot butterflies', Proceedings of the International Astronomical Union, vol. 8, no. S294, pp. 87-92. https://doi.org/10.1017/S1743921313002317

APA

Zolotova, N. V., & Ponyavin, D. I. (2013). Model of poleward magnetic field streams from sunspot butterflies. Proceedings of the International Astronomical Union, 8(S294), 87-92. https://doi.org/10.1017/S1743921313002317

Vancouver

Zolotova NV, Ponyavin DI. Model of poleward magnetic field streams from sunspot butterflies. Proceedings of the International Astronomical Union. 2013;8(S294):87-92. https://doi.org/10.1017/S1743921313002317

Author

Zolotova, N.V. ; Ponyavin, D.I. / Model of poleward magnetic field streams from sunspot butterflies. In: Proceedings of the International Astronomical Union. 2013 ; Vol. 8, No. S294. pp. 87-92.

BibTeX

@article{08333ab201e644f4becf4e0cce99d028,
title = "Model of poleward magnetic field streams from sunspot butterflies",
abstract = "The poleward magnetic field streams on time-latitude diagram of the photospheric magnetic field of the Sun during 1975–2011 (Kitt Peak NSO, SOLIS NSO, SOHO MDI data) are modeled. We performed simulations in terms of probability density function and bipole orientation according to Joy's law and Hale's cycle. The difference between distributions of leading and trailing fluxes of bipolar sunspots defines the so-called surplus. Finally, magnetic field streams and polar field reversals are a result of meridional drift of a surplus to the poles.",
keywords = "Sun: activity, Sun: magnetic fields, (Sun:) sunspots",
author = "N.V. Zolotova and D.I. Ponyavin",
year = "2013",
doi = "10.1017/S1743921313002317",
language = "English",
volume = "8",
pages = "87--92",
journal = "Proceedings of the International Astronomical Union",
issn = "1743-9213",
publisher = "Cambridge University Press",
number = "S294",

}

RIS

TY - JOUR

T1 - Model of poleward magnetic field streams from sunspot butterflies

AU - Zolotova, N.V.

AU - Ponyavin, D.I.

PY - 2013

Y1 - 2013

N2 - The poleward magnetic field streams on time-latitude diagram of the photospheric magnetic field of the Sun during 1975–2011 (Kitt Peak NSO, SOLIS NSO, SOHO MDI data) are modeled. We performed simulations in terms of probability density function and bipole orientation according to Joy's law and Hale's cycle. The difference between distributions of leading and trailing fluxes of bipolar sunspots defines the so-called surplus. Finally, magnetic field streams and polar field reversals are a result of meridional drift of a surplus to the poles.

AB - The poleward magnetic field streams on time-latitude diagram of the photospheric magnetic field of the Sun during 1975–2011 (Kitt Peak NSO, SOLIS NSO, SOHO MDI data) are modeled. We performed simulations in terms of probability density function and bipole orientation according to Joy's law and Hale's cycle. The difference between distributions of leading and trailing fluxes of bipolar sunspots defines the so-called surplus. Finally, magnetic field streams and polar field reversals are a result of meridional drift of a surplus to the poles.

KW - Sun: activity

KW - Sun: magnetic fields

KW - (Sun:) sunspots

U2 - 10.1017/S1743921313002317

DO - 10.1017/S1743921313002317

M3 - Conference article

VL - 8

SP - 87

EP - 92

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

SN - 1743-9213

IS - S294

ER -

ID: 73930588