Supervised classification of solar features using prior information

Context: The Sun as seen by Extreme Ultraviolet (EUV) telescopes exhibits a variety of large-scale structures. Of particular interest for space-weather applications is the extraction of active regions (AR) and coronal holes (CH). The next generation of GOES-R satellites will provide continuous monit...

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Main Authors: De Visscher Ruben, Delouille Véronique, Dupont Pierre, Deledalle Charles-Alban
Format: Article
Language:English
Published: EDP Sciences 2015-01-01
Series:Journal of Space Weather and Space Climate
Subjects:
Online Access:http://dx.doi.org/10.1051/swsc/2015033
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spelling doaj-eb13c8a6be5a4cdda0202114090609552021-04-02T10:18:17ZengEDP SciencesJournal of Space Weather and Space Climate2115-72512015-01-015A3410.1051/swsc/2015033swsc140058Supervised classification of solar features using prior informationDe Visscher RubenDelouille VéroniqueDupont PierreDeledalle Charles-AlbanContext: The Sun as seen by Extreme Ultraviolet (EUV) telescopes exhibits a variety of large-scale structures. Of particular interest for space-weather applications is the extraction of active regions (AR) and coronal holes (CH). The next generation of GOES-R satellites will provide continuous monitoring of the solar corona in six EUV bandpasses that are similar to the ones provided by the SDO-AIA EUV telescope since May 2010. Supervised segmentations of EUV images that are consistent with manual segmentations by for example space-weather forecasters help in extracting useful information from the raw data. Aims: We present a supervised segmentation method that is based on the Maximum A Posteriori rule. Our method allows integrating both manually segmented images as well as other type of information. It is applied on SDO-AIA images to segment them into AR, CH, and the remaining Quiet Sun (QS) part. Methods: A Bayesian classifier is applied on training masks provided by the user. The noise structure in EUV images is non-trivial, and this suggests the use of a non-parametric kernel density estimator to fit the intensity distribution within each class. Under the Naive Bayes assumption we can add information such as latitude distribution and total coverage of each class in a consistent manner. Those information can be prescribed by an expert or estimated with an Expectation-Maximization algorithm. Results: The segmentation masks are in line with the training masks given as input and show consistency over time. Introduction of additional information besides pixel intensity improves upon the quality of the final segmentation. Conclusions: Such a tool can aid in building automated segmentations that are consistent with some ground truth’ defined by the users.http://dx.doi.org/10.1051/swsc/2015033Solar image processingCoronaStatistics and probabilityClassification
collection DOAJ
language English
format Article
sources DOAJ
author De Visscher Ruben
Delouille Véronique
Dupont Pierre
Deledalle Charles-Alban
spellingShingle De Visscher Ruben
Delouille Véronique
Dupont Pierre
Deledalle Charles-Alban
Supervised classification of solar features using prior information
Journal of Space Weather and Space Climate
Solar image processing
Corona
Statistics and probability
Classification
author_facet De Visscher Ruben
Delouille Véronique
Dupont Pierre
Deledalle Charles-Alban
author_sort De Visscher Ruben
title Supervised classification of solar features using prior information
title_short Supervised classification of solar features using prior information
title_full Supervised classification of solar features using prior information
title_fullStr Supervised classification of solar features using prior information
title_full_unstemmed Supervised classification of solar features using prior information
title_sort supervised classification of solar features using prior information
publisher EDP Sciences
series Journal of Space Weather and Space Climate
issn 2115-7251
publishDate 2015-01-01
description Context: The Sun as seen by Extreme Ultraviolet (EUV) telescopes exhibits a variety of large-scale structures. Of particular interest for space-weather applications is the extraction of active regions (AR) and coronal holes (CH). The next generation of GOES-R satellites will provide continuous monitoring of the solar corona in six EUV bandpasses that are similar to the ones provided by the SDO-AIA EUV telescope since May 2010. Supervised segmentations of EUV images that are consistent with manual segmentations by for example space-weather forecasters help in extracting useful information from the raw data. Aims: We present a supervised segmentation method that is based on the Maximum A Posteriori rule. Our method allows integrating both manually segmented images as well as other type of information. It is applied on SDO-AIA images to segment them into AR, CH, and the remaining Quiet Sun (QS) part. Methods: A Bayesian classifier is applied on training masks provided by the user. The noise structure in EUV images is non-trivial, and this suggests the use of a non-parametric kernel density estimator to fit the intensity distribution within each class. Under the Naive Bayes assumption we can add information such as latitude distribution and total coverage of each class in a consistent manner. Those information can be prescribed by an expert or estimated with an Expectation-Maximization algorithm. Results: The segmentation masks are in line with the training masks given as input and show consistency over time. Introduction of additional information besides pixel intensity improves upon the quality of the final segmentation. Conclusions: Such a tool can aid in building automated segmentations that are consistent with some ground truth’ defined by the users.
topic Solar image processing
Corona
Statistics and probability
Classification
url http://dx.doi.org/10.1051/swsc/2015033
work_keys_str_mv AT devisscherruben supervisedclassificationofsolarfeaturesusingpriorinformation
AT delouilleveronique supervisedclassificationofsolarfeaturesusingpriorinformation
AT dupontpierre supervisedclassificationofsolarfeaturesusingpriorinformation
AT deledallecharlesalban supervisedclassificationofsolarfeaturesusingpriorinformation
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