A new approach to automatically segment the solar coronal loop structures from intensity images of the Sun’s corona is described. The approach is based on the active contour models (snakes) and exploits the Gaussian-like shape of the coronal loop cross-sectional intensity profile to refine the snake’s position. The approach utilizes the principal component analysis to automatically initialize the snake’s position. It then uses a greedy minimization method to attract the snake toward the center of coronal loop structures in each image. Its effectiveness is evaluated through experiments on synthetic and real images
This paper proposes enhancements to the deformable models. Focusing on the problem of vessel segment...
Identification and tracking of solar coronal loops is key to understanding solar magnetic field. Slo...
This is an open access article, original content from this work may be used under the terms of the C...
A new approach to automatically segment the solar coronal loop structures from intensity images of t...
This paper presents a deep convolutional neural network (CNN) based method that automatically segmen...
An automated technique to segment solar coronal loops from intensity images of the Sun s corona is i...
Astrophysicists currently study NASA\u27s extensive databases of solar satellite images, in part bec...
Solar-flare UV and EUV images show elongated bright "ribbons" that move over time. If these ribbons ...
Coronal loops are especially important in analyzing some important phenomena related to the Sun such...
In this paper, the method of identifying of the similar solar flux tubes from image sequence EUVI/ST...
Developing specialized software tools is essential to support studies of solar activity evolution. W...
Knowing the three dimensional structure of plasma filaments in the uppermost part of the solar atmos...
An alternative solution to active contours is proposed. Segmentation is achieved continuously by cha...
Abstract — We present our preliminary findings as part of a new data mining application aiming at th...
The study of the variability of the solar corona and the monitoring of its traditional regions (Coro...
This paper proposes enhancements to the deformable models. Focusing on the problem of vessel segment...
Identification and tracking of solar coronal loops is key to understanding solar magnetic field. Slo...
This is an open access article, original content from this work may be used under the terms of the C...
A new approach to automatically segment the solar coronal loop structures from intensity images of t...
This paper presents a deep convolutional neural network (CNN) based method that automatically segmen...
An automated technique to segment solar coronal loops from intensity images of the Sun s corona is i...
Astrophysicists currently study NASA\u27s extensive databases of solar satellite images, in part bec...
Solar-flare UV and EUV images show elongated bright "ribbons" that move over time. If these ribbons ...
Coronal loops are especially important in analyzing some important phenomena related to the Sun such...
In this paper, the method of identifying of the similar solar flux tubes from image sequence EUVI/ST...
Developing specialized software tools is essential to support studies of solar activity evolution. W...
Knowing the three dimensional structure of plasma filaments in the uppermost part of the solar atmos...
An alternative solution to active contours is proposed. Segmentation is achieved continuously by cha...
Abstract — We present our preliminary findings as part of a new data mining application aiming at th...
The study of the variability of the solar corona and the monitoring of its traditional regions (Coro...
This paper proposes enhancements to the deformable models. Focusing on the problem of vessel segment...
Identification and tracking of solar coronal loops is key to understanding solar magnetic field. Slo...
This is an open access article, original content from this work may be used under the terms of the C...