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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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Publisher copy:
10.1007/s11207-007-9074-7

Authors


Journal:
SOLAR PHYSICS More from this journal
Volume:
248
Issue:
2
Pages:
297-309
Publication date:
2008-04-01
DOI:
EISSN:
1573-093X
ISSN:
0038-0938
Keywords:
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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