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Multi-fractality of Multi-fractality of Solar Magnetic Fields: Solar Magnetic Fields: New Progress with HMI New Progress with HMI Valentina I. Abramenko Big Bear Solar Observatory of NJIT Poster #40

Multi-fractality of Solar Magnetic Fields: New Progress with HMI Valentina I. Abramenko Big Bear Solar Observatory of NJIT Poster #40

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Page 1: Multi-fractality of Solar Magnetic Fields: New Progress with HMI Valentina I. Abramenko Big Bear Solar Observatory of NJIT Poster #40

Multi-fractality of Solar Multi-fractality of Solar Magnetic Fields: New Progress Magnetic Fields: New Progress

with HMIwith HMI

Valentina I. AbramenkoBig Bear Solar Observatory of NJIT

Poster #40

Page 2: Multi-fractality of Solar Magnetic Fields: New Progress with HMI Valentina I. Abramenko Big Bear Solar Observatory of NJIT Poster #40

Flatness function as an indicator of multifractalityFlatness function as an indicator of multifractality

Fatness F( r ) is a constant for a Gaussian variable

and grows as a power lawpower law when scale r vanishes for a multi-fractal field:

Inertial range

Scale, r

F( r ) ~ r-κ

F( r ) =S ( r ) / (S ( r ) )6

32

The multifractality index, κ

κ

Page 3: Multi-fractality of Solar Magnetic Fields: New Progress with HMI Valentina I. Abramenko Big Bear Solar Observatory of NJIT Poster #40

Power Spectrumcutoff

Page 4: Multi-fractality of Solar Magnetic Fields: New Progress with HMI Valentina I. Abramenko Big Bear Solar Observatory of NJIT Poster #40

AR 11166

Power Spectrum Index Flatness Function Index

Page 5: Multi-fractality of Solar Magnetic Fields: New Progress with HMI Valentina I. Abramenko Big Bear Solar Observatory of NJIT Poster #40
Page 6: Multi-fractality of Solar Magnetic Fields: New Progress with HMI Valentina I. Abramenko Big Bear Solar Observatory of NJIT Poster #40

About 1.8 days prior to a strong flarewe observe a period of enhanced multi-fractalityin the photosphere

AR 11158

Power Spectrum IndexFlatness FunctionIndex

Page 7: Multi-fractality of Solar Magnetic Fields: New Progress with HMI Valentina I. Abramenko Big Bear Solar Observatory of NJIT Poster #40

NOAA 10930: intermittency/multifractality in the

photosphere and corona

1.3 days