Scale invariant images in astronomy through ...
Document type :
Communication dans un congrès avec actes
Title :
Scale invariant images in astronomy through the lens of multifractal modeling
Author(s) :
Chainais, Pierre [Auteur]
Centrale Lille
Centre de Recherche en Informatique, Signal et Automatique de Lille - UMR 9189 [CRIStAL]
LAGIS-SI
Delouille, Véronique [Auteur]
Solar Physics Department [Brussels]
Hochedez, Jean-François [Auteur]
HELIOS - LATMOS
Centrale Lille
Centre de Recherche en Informatique, Signal et Automatique de Lille - UMR 9189 [CRIStAL]
LAGIS-SI
Delouille, Véronique [Auteur]
Solar Physics Department [Brussels]
Hochedez, Jean-François [Auteur]
HELIOS - LATMOS
Conference title :
18th IEEE International Conference on Image Processing (ICIP2011),
City :
Brussels
Country :
Belgique
Start date of the conference :
2011-09-12
Publication date :
2011
English keyword(s) :
self-similarity
multifractal analysis
stochastic processes
extrapolation
solar corona
multifractal analysis
stochastic processes
extrapolation
solar corona
HAL domain(s) :
Informatique [cs]/Traitement des images [eess.IV]
Sciences de l'ingénieur [physics]/Traitement du signal et de l'image [eess.SP]
Informatique [cs]/Traitement du signal et de l'image [eess.SP]
Planète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR]
Physique [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR]
Physique [physics]/Physique [physics]/Physique Atmosphérique et Océanique [physics.ao-ph]
Sciences de l'ingénieur [physics]/Traitement du signal et de l'image [eess.SP]
Informatique [cs]/Traitement du signal et de l'image [eess.SP]
Planète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR]
Physique [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR]
Physique [physics]/Physique [physics]/Physique Atmosphérique et Océanique [physics.ao-ph]
English abstract : [en]
The mystery of the dynamics of the Sun is even deeper when it is quiet, i.e. when there are no coherent areas structured by strong magnetic field and called active regions. The solar corona is observed by extreme UV spatial ...
Show more >The mystery of the dynamics of the Sun is even deeper when it is quiet, i.e. when there are no coherent areas structured by strong magnetic field and called active regions. The solar corona is observed by extreme UV spatial telescopes for which higher resolutions are always desired: the best pixel resolution currently achievable is 500 km which still leaves room for crucial hidden details. We present our work on the analysis of quiet Sun images of the corona. These images exhibit multifractal properties and a model based on scale invariant stochastic processes, called fractionally integrated compound Poisson cascades, reproduces their main statistical properties. We show that it can be used to develop a virtual super-resolution method that proposes plausible predictions of the high resolution information hidden below the pixel size of present observations. Such images may help physicists to test and calibrate on-board processing algorithms for future missions.Show less >
Show more >The mystery of the dynamics of the Sun is even deeper when it is quiet, i.e. when there are no coherent areas structured by strong magnetic field and called active regions. The solar corona is observed by extreme UV spatial telescopes for which higher resolutions are always desired: the best pixel resolution currently achievable is 500 km which still leaves room for crucial hidden details. We present our work on the analysis of quiet Sun images of the corona. These images exhibit multifractal properties and a model based on scale invariant stochastic processes, called fractionally integrated compound Poisson cascades, reproduces their main statistical properties. We show that it can be used to develop a virtual super-resolution method that proposes plausible predictions of the high resolution information hidden below the pixel size of present observations. Such images may help physicists to test and calibrate on-board processing algorithms for future missions.Show less >
Language :
Anglais
Peer reviewed article :
Oui
Audience :
Internationale
Popular science :
Non
Comment :
4 pages
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