IMPLEMENTATION OF CONVOLUTIONAL NEURAL NETWORK MODEL ON HMI AND AIA IMAGES FOR M AND X CLASS SOLAR FLARE DETECTION

<p align="justify">In recent years, interest in Solar data processing has increased rapidly. This data processing aims to monitor and understand Solar activity, including solar flares. Monitoring and understanding solar flare occurrences are important because these events determine s...

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Main Author: Lee, Sylvie
Format: Final Project
Language:Indonesia
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Online Access:https://digilib.itb.ac.id/gdl/view/81221
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Institution: Institut Teknologi Bandung
Language: Indonesia
id id-itb.:81221
spelling id-itb.:812212024-05-22T15:34:59ZIMPLEMENTATION OF CONVOLUTIONAL NEURAL NETWORK MODEL ON HMI AND AIA IMAGES FOR M AND X CLASS SOLAR FLARE DETECTION Lee, Sylvie Astronomi Indonesia Final Project solar flare, deep learning, Convolutional Neural Network (CNN), Solar Dynamics Observatory (SDO), Python, HMI, AIA. INSTITUT TEKNOLOGI BANDUNG https://digilib.itb.ac.id/gdl/view/81221 <p align="justify">In recent years, interest in Solar data processing has increased rapidly. This data processing aims to monitor and understand Solar activity, including solar flares. Monitoring and understanding solar flare occurrences are important because these events determine space weather, which impacts infrastructure and technology used in communication, satellite navigation, and space missions. Manual monitoring of solar flares by humans cannot be fully relied upon. This is because detection and identification by humans are highly dependent on the observer's abilities and are time-consuming. Therefore, the development of automatic solar flare detection without human intervention is a challenge in this regard. The focus of automatic solar flare detection lies in developing efficient feature-based classification. Various automatic solar flare detection techniques that have been developed and implemented mostly use deep learning approaches. In this final project research, the author employs image processing techniques to make the analysis process more efficient by applying a Convolutional Neural Network (CNN) approach directly to raw pixels. The input data used in this system are daily solar flare activity data from Space Weather Live and raw image data from the Solar Dynamics Observatory (SDO; Pesnell et al., 2012). There are two algorithms that the author applies in this final project research: 1) The first system is designed to recognize solar flares through the analysis of active region data extracted from full-disk magnetogram images (HMI). 2) The second system is designed to recognize solar flares through the analysis of ultraviolet intensity data extracted from full-disk ultraviolet intensity images (AIA). From this research, the author found that a CNN model with a ResNet-50 architecture using AIA data from 2020-2023 provided the best prediction performance among other architecture models. Additionally, the author also found that the choice between using HMI or AIA data and augmentation variations showed no correlation with model performance, but this depends on the architecture influencing the model's performance. Furthermore, the author also found that an increase in the amount of data improves the model's generalization ability.<p align="justify"> text
institution Institut Teknologi Bandung
building Institut Teknologi Bandung Library
continent Asia
country Indonesia
Indonesia
content_provider Institut Teknologi Bandung
collection Digital ITB
language Indonesia
topic Astronomi
spellingShingle Astronomi
Lee, Sylvie
IMPLEMENTATION OF CONVOLUTIONAL NEURAL NETWORK MODEL ON HMI AND AIA IMAGES FOR M AND X CLASS SOLAR FLARE DETECTION
description <p align="justify">In recent years, interest in Solar data processing has increased rapidly. This data processing aims to monitor and understand Solar activity, including solar flares. Monitoring and understanding solar flare occurrences are important because these events determine space weather, which impacts infrastructure and technology used in communication, satellite navigation, and space missions. Manual monitoring of solar flares by humans cannot be fully relied upon. This is because detection and identification by humans are highly dependent on the observer's abilities and are time-consuming. Therefore, the development of automatic solar flare detection without human intervention is a challenge in this regard. The focus of automatic solar flare detection lies in developing efficient feature-based classification. Various automatic solar flare detection techniques that have been developed and implemented mostly use deep learning approaches. In this final project research, the author employs image processing techniques to make the analysis process more efficient by applying a Convolutional Neural Network (CNN) approach directly to raw pixels. The input data used in this system are daily solar flare activity data from Space Weather Live and raw image data from the Solar Dynamics Observatory (SDO; Pesnell et al., 2012). There are two algorithms that the author applies in this final project research: 1) The first system is designed to recognize solar flares through the analysis of active region data extracted from full-disk magnetogram images (HMI). 2) The second system is designed to recognize solar flares through the analysis of ultraviolet intensity data extracted from full-disk ultraviolet intensity images (AIA). From this research, the author found that a CNN model with a ResNet-50 architecture using AIA data from 2020-2023 provided the best prediction performance among other architecture models. Additionally, the author also found that the choice between using HMI or AIA data and augmentation variations showed no correlation with model performance, but this depends on the architecture influencing the model's performance. Furthermore, the author also found that an increase in the amount of data improves the model's generalization ability.<p align="justify">
format Final Project
author Lee, Sylvie
author_facet Lee, Sylvie
author_sort Lee, Sylvie
title IMPLEMENTATION OF CONVOLUTIONAL NEURAL NETWORK MODEL ON HMI AND AIA IMAGES FOR M AND X CLASS SOLAR FLARE DETECTION
title_short IMPLEMENTATION OF CONVOLUTIONAL NEURAL NETWORK MODEL ON HMI AND AIA IMAGES FOR M AND X CLASS SOLAR FLARE DETECTION
title_full IMPLEMENTATION OF CONVOLUTIONAL NEURAL NETWORK MODEL ON HMI AND AIA IMAGES FOR M AND X CLASS SOLAR FLARE DETECTION
title_fullStr IMPLEMENTATION OF CONVOLUTIONAL NEURAL NETWORK MODEL ON HMI AND AIA IMAGES FOR M AND X CLASS SOLAR FLARE DETECTION
title_full_unstemmed IMPLEMENTATION OF CONVOLUTIONAL NEURAL NETWORK MODEL ON HMI AND AIA IMAGES FOR M AND X CLASS SOLAR FLARE DETECTION
title_sort implementation of convolutional neural network model on hmi and aia images for m and x class solar flare detection
url https://digilib.itb.ac.id/gdl/view/81221
_version_ 1822009415691141120