Multi-fractality of Solar Magnetic Fields: New Progress with HMI Valentina I. Abramenko Big Bear...
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Transcript of Multi-fractality of Solar Magnetic Fields: New Progress with HMI Valentina I. Abramenko Big Bear...
![Page 1: Multi-fractality of Solar Magnetic Fields: New Progress with HMI Valentina I. Abramenko Big Bear Solar Observatory of NJIT Poster #40.](https://reader035.fdocuments.us/reader035/viewer/2022062407/56649d565503460f94a34755/html5/thumbnails/1.jpg)
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.](https://reader035.fdocuments.us/reader035/viewer/2022062407/56649d565503460f94a34755/html5/thumbnails/2.jpg)
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.](https://reader035.fdocuments.us/reader035/viewer/2022062407/56649d565503460f94a34755/html5/thumbnails/3.jpg)
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.](https://reader035.fdocuments.us/reader035/viewer/2022062407/56649d565503460f94a34755/html5/thumbnails/4.jpg)
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.](https://reader035.fdocuments.us/reader035/viewer/2022062407/56649d565503460f94a34755/html5/thumbnails/5.jpg)
![Page 6: Multi-fractality of Solar Magnetic Fields: New Progress with HMI Valentina I. Abramenko Big Bear Solar Observatory of NJIT Poster #40.](https://reader035.fdocuments.us/reader035/viewer/2022062407/56649d565503460f94a34755/html5/thumbnails/6.jpg)
About 1.8 days prior to a strong flarewe observe a period of enhanced multi-fractalityin the photosphere
AR 11158
Power Spectrum IndexFlatness FunctionIndex
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NOAA 10930: intermittency/multifractality in the
photosphere and corona
1.3 days