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Journal article

Multifractal properties of evolving active regions

Abstract:: Magnetohydrodynamic turbulence is thought to be responsible for producing complex, multiscale magnetic field distributions in solar active regions. Here we explore the multiscale properties of a number of evolving active regions using magnetograms from the Michelson Doppler Imager (MDI) on the Solar and Heliospheric Observatory (SOHO). The multifractal spectrum was obtained by using a modified box-counting method to study the relationship between magnetic-field multifractality and region evol...
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Publication status:: Published

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APA Style

Conlon, P., Gallagher, P., McAteer, R., Ireland, J., Young, C., Kestener, P., Hewett, R., & Maguire, K. (2008). Multifractal properties of evolving active regions. SOLAR PHYSICS, 248(2), 297–309.

MLA Style

Conlon, P., et al. “Multifractal Properties of Evolving Active Regions.” SOLAR PHYSICS, vol. 248, no. 2, 2008, pp. 297–309.

Chicago Style

Conlon, P, P Gallagher, R McAteer, J Ireland, C Young, P Kestener, R Hewett, and K Maguire. 2008. “Multifractal Properties of Evolving Active Regions.” SOLAR PHYSICS 248 (2): 297–309.
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Publisher copy:: 10.1007/s11207-007-9074-7

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+ Conlon, P More by this author

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+ Gallagher, P More by this author

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+ McAteer, R More by this author

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+ Ireland, J More by this author

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+ Young, C More by this author

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Bibliographic Details

Journal:: SOLAR PHYSICS
Volume:: 248
Issue:: 2
Pages:: 297-309
Publication date:: 2008-04-01
DOI:: 10.1007/s11207-007-9074-7
EISSN:: 1573-093X
ISSN:: 0038-0938

Item Description

Keywords:: magnetic fields

active regions

turbulence
Pubs id:: pubs:187618
UUID:: uuid:cd6a2b76-ab6a-4dfb-b233-f770961d1f81
Local pid:: pubs:187618
Source identifiers:: 187618
Deposit date:: 2012-12-19

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Copyright date:: 2008

Licence:: Terms and Conditions of Use for Oxford University Research Archive

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