Coronal loops are especially important in analyzing some important phenomena related to the Sun such as the controversial coronal heating problem. The analysis requires astrophysicists to manually sift through thousands of images in order to acquire images containing coronal loops. Thus, the motivation to detect these loops automatically. Since coronal loops do not have a perfect shape and are easy to confuse with other solar events, feature selection to learn characteristics of loops requires special care. In this study, we explore standard image features as well as specialized image features considering coronal loop characteristics. Our experiments confirm the success of our explored features in coronal loop detection
The identification of solar coronal holes (CHs) observed in Extreme Ultraviolet (EUV) intensity imag...
Context. Coronal loop oscillations can be triggered by solar eruptions, for example, and are observe...
We report results of an in-depth numerical investigation of three-dimensional projection effects whi...
Abstract — We present our preliminary findings as part of a new data mining application aiming at th...
Astrophysicists currently study NASA\u27s extensive databases of solar satellite images, in part bec...
In this paper, the method of identifying of the similar solar flux tubes from image sequence EUVI/ST...
An automated technique to segment solar coronal loops from intensity images of the Sun s corona is i...
Identification and tracking of solar coronal loops is key to understanding solar magnetic field. Slo...
New and advanced space-based observing facilities continue to lower the resolution limit and detect ...
This is an open access article, original content from this work may be used under the terms of the C...
This dissertation describes two aspects of solar coronal dynamics: waves in coronal loops (Part I) a...
A new method for automated coronal loop tracking, in both spatial and temporal domains, is presented...
Aims. We use new data from the High-resolution Coronal Imager (Hi-C) with its unprecedented spatial ...
A new method for automated coronal loop tracking, in both spatial and temporal domains, is presented...
This paper presents a deep convolutional neural network (CNN) based method that automatically segmen...
The identification of solar coronal holes (CHs) observed in Extreme Ultraviolet (EUV) intensity imag...
Context. Coronal loop oscillations can be triggered by solar eruptions, for example, and are observe...
We report results of an in-depth numerical investigation of three-dimensional projection effects whi...
Abstract — We present our preliminary findings as part of a new data mining application aiming at th...
Astrophysicists currently study NASA\u27s extensive databases of solar satellite images, in part bec...
In this paper, the method of identifying of the similar solar flux tubes from image sequence EUVI/ST...
An automated technique to segment solar coronal loops from intensity images of the Sun s corona is i...
Identification and tracking of solar coronal loops is key to understanding solar magnetic field. Slo...
New and advanced space-based observing facilities continue to lower the resolution limit and detect ...
This is an open access article, original content from this work may be used under the terms of the C...
This dissertation describes two aspects of solar coronal dynamics: waves in coronal loops (Part I) a...
A new method for automated coronal loop tracking, in both spatial and temporal domains, is presented...
Aims. We use new data from the High-resolution Coronal Imager (Hi-C) with its unprecedented spatial ...
A new method for automated coronal loop tracking, in both spatial and temporal domains, is presented...
This paper presents a deep convolutional neural network (CNN) based method that automatically segmen...
The identification of solar coronal holes (CHs) observed in Extreme Ultraviolet (EUV) intensity imag...
Context. Coronal loop oscillations can be triggered by solar eruptions, for example, and are observe...
We report results of an in-depth numerical investigation of three-dimensional projection effects whi...