The perturbed photometric-magnetic dynamical model for the sunspot evolution

G. Livadiotis; X. Moussas

doi:10.1007/978-3-540-75826-6_46

The perturbed photometric-magnetic dynamical model for the sunspot evolution

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract

We present the perturbed version of the Photometric-Magnetic Dynamical (PhMD) model for describing the sunspot evolution. This involves fluctuating the magnetic flux inflow into the sunspot, by a harmonic perturbation with frequency equal to that of the solar rotation. The nonlinear dynamical system is studied either for the conservative or for the dissipative case.

Original language	English (US)
Title of host publication	Astrophysics and Space Science Proceedings
Editors	G. Contopoulos, P.A. Patsis
Publisher	Springer Science and Business Media B.V.
Pages	455-459
Number of pages	5
ISBN (Electronic)	9783540758266
ISBN (Print)	9780387727677, 9780387876207, 9781402055720, 9781402069321, 9781402088674, 9781402091896, 9781441981608, 9781441983688, 9783540758259, 9783540758259, 9783642033230, 9783642103216, 9783642103513, 9783642113406, 9783642172502, 9789048133994, 9789048134984
DOIs	https://doi.org/10.1007/978-3-540-75826-6_46
State	Published - 2009
Externally published	Yes
Event	Conference on Chaos in Astronomy, 2007 - Athens, Greece Duration: Sep 17 2007 → Sep 20 2007

Publication series

Name	Astrophysics and Space Science Proceedings
Volume	0
ISSN (Print)	1570-6591
ISSN (Electronic)	1570-6605

Conference

Conference	Conference on Chaos in Astronomy, 2007
Country/Territory	Greece
City	Athens
Period	9/17/07 → 9/20/07

All Science Journal Classification (ASJC) codes

General Physics and Astronomy
Computer Science Applications
Spectroscopy
Space and Planetary Science
Nuclear and High Energy Physics

Access to Document

10.1007/978-3-540-75826-6_46

Cite this

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title = "The perturbed photometric-magnetic dynamical model for the sunspot evolution",

abstract = "We present the perturbed version of the Photometric-Magnetic Dynamical (PhMD) model for describing the sunspot evolution. This involves fluctuating the magnetic flux inflow into the sunspot, by a harmonic perturbation with frequency equal to that of the solar rotation. The nonlinear dynamical system is studied either for the conservative or for the dissipative case.",

author = "G. Livadiotis and X. Moussas",

note = "Publisher Copyright: {\textcopyright} Springer-Verlag Berlin Heidelberg 2009.; Conference on Chaos in Astronomy, 2007 ; Conference date: 17-09-2007 Through 20-09-2007",

year = "2009",

doi = "10.1007/978-3-540-75826-6_46",

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series = "Astrophysics and Space Science Proceedings",

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Livadiotis, G & Moussas, X 2009, The perturbed photometric-magnetic dynamical model for the sunspot evolution. in G Contopoulos & PA Patsis (eds), Astrophysics and Space Science Proceedings. Astrophysics and Space Science Proceedings, vol. 0, Springer Science and Business Media B.V., pp. 455-459, Conference on Chaos in Astronomy, 2007, Athens, Greece, 9/17/07. https://doi.org/10.1007/978-3-540-75826-6_46

The perturbed photometric-magnetic dynamical model for the sunspot evolution. / Livadiotis, G.; Moussas, X.
Astrophysics and Space Science Proceedings. ed. / G. Contopoulos; P.A. Patsis. Springer Science and Business Media B.V., 2009. p. 455-459 (Astrophysics and Space Science Proceedings; Vol. 0).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

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N2 - We present the perturbed version of the Photometric-Magnetic Dynamical (PhMD) model for describing the sunspot evolution. This involves fluctuating the magnetic flux inflow into the sunspot, by a harmonic perturbation with frequency equal to that of the solar rotation. The nonlinear dynamical system is studied either for the conservative or for the dissipative case.

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PB - Springer Science and Business Media B.V.

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ER -

The perturbed photometric-magnetic dynamical model for the sunspot evolution

Abstract

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Conference

All Science Journal Classification (ASJC) codes

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