Topology and dynamics of the Sun’s magnetic field

Gavryuseva, E.; Kroussanova, N. L.

doi:10.1063/1.1618587

AIP Conference Proceedings

2003

DOI: 10.1063/1.1618587

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Topology and dynamics of the Sun’s magnetic field

E. Gavryuseva¹,

N. L. Kroussanova²

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“…Differential rotational rate of the magnetic field and its temporal dependence has been evidenced at different latitudes through activity cycles (Gavryuseva & Godoli (2004), , Gavryuseva (2007)). Rotational rate of the large scale magnetic field at the latitudes above 55 degrees doesn't getting slower.…”

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confidence: 99%

Differential Rotation of the Sun from helioseismology and magnetic field study.

Gavryuseva¹,

Höfner²

2009

Proc. IAU

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Abstract. Differential rotational rate of the large scale magnetic field and its temporal dependence has been evidenced at different latitudes through activity cycles 21-23. Rotational rate of the magnetic field at the latitudes above 55 degrees doesn't getting slower. Torsional waves with 11-year period are clearly seen in the magnetic field rotation. Rotation is slower where and when the magnetic field is getting stronger.The time of the magnetic field emergence to the photosphere was estimated. It was revealed the existence of quasi-stable over 30 years exceptionally regular and symmetric in the both hemispherest longitudinal structure. This structure is originated from the tachocline zone rotating like a rigid body with the rotation rate corresponding to the rotation in the photosphere on the 55-60 degrees of the helio-latitudes.

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mentioning

confidence: 99%

Differential Rotation of the Sun from helioseismology and magnetic field study.

Gavryuseva¹,

Höfner²

2009

Proc. IAU

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The latitudinal distributions of sunspot areas and magnetic fields and their correlation with the background solar magnetic field in the cycle 23

Zharkov

Gavryuseva

Zharkova

2007

Advances in Space Research

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Structure and rotation of the large scale solar magnetic field observed at the Wilcox Solar Observatory

Gavryuseva

Godoli

2006

Physics and Chemistry of the Earth, Parts A/B/C

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Topology and dynamics of the Sun’s magnetic field

Cited by 3 publications

References 0 publications

Differential Rotation of the Sun from helioseismology and magnetic field study.

Differential Rotation of the Sun from helioseismology and magnetic field study.

The latitudinal distributions of sunspot areas and magnetic fields and their correlation with the background solar magnetic field in the cycle 23

Structure and rotation of the large scale solar magnetic field observed at the Wilcox Solar Observatory

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