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STEREOSocietal event
In this paper, the method of identifying of the similar solar flux tubes from image sequence EUVI/STEREO is presented. Using the oriented coronal curved loop tracing, the loops of an image are labeled. Based on local maxima intensities, the width of loops is determined. The Zernike moments of each loop are calculated and fed to probabilistic network classifier. Also, 588 loops from STEREO are studied
Aims. Detailed analysis of 11 transverse coronal loop oscillations in three events observed with the...
We transition from two-dimensional (2D) imaging observations of kink-mode loop oscillations in the s...
Aims. We use new data from the High-resolution Coronal Imager (Hi-C) with its unprecedented spatial ...
Identification and tracking of solar coronal loops is key to understanding solar magnetic field. Slo...
Coronal loops are especially important in analyzing some important phenomena related to the Sun such...
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...
Abstract — We present our preliminary findings as part of a new data mining application aiming at th...
This is an open access article, original content from this work may be used under the terms of the C...
This paper presents a deep convolutional neural network (CNN) based method that automatically segmen...
Knowing the three dimensional structure of plasma filaments in the uppermost part of the solar atmos...
Abstract. In this study, we describe and evaluate shape measures for distinguishing between coronal ...
A new approach to automatically segment the solar coronal loop structures from intensity images of t...
International audiencePrevious studies have found that coronal loops have a nearly uniform thickness...
We present an automated extraction method based on the continuous wavelet transform (CWT) for analyz...
Aims. Detailed analysis of 11 transverse coronal loop oscillations in three events observed with the...
We transition from two-dimensional (2D) imaging observations of kink-mode loop oscillations in the s...
Aims. We use new data from the High-resolution Coronal Imager (Hi-C) with its unprecedented spatial ...
Identification and tracking of solar coronal loops is key to understanding solar magnetic field. Slo...
Coronal loops are especially important in analyzing some important phenomena related to the Sun such...
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...
Abstract — We present our preliminary findings as part of a new data mining application aiming at th...
This is an open access article, original content from this work may be used under the terms of the C...
This paper presents a deep convolutional neural network (CNN) based method that automatically segmen...
Knowing the three dimensional structure of plasma filaments in the uppermost part of the solar atmos...
Abstract. In this study, we describe and evaluate shape measures for distinguishing between coronal ...
A new approach to automatically segment the solar coronal loop structures from intensity images of t...
International audiencePrevious studies have found that coronal loops have a nearly uniform thickness...
We present an automated extraction method based on the continuous wavelet transform (CWT) for analyz...
Aims. Detailed analysis of 11 transverse coronal loop oscillations in three events observed with the...
We transition from two-dimensional (2D) imaging observations of kink-mode loop oscillations in the s...
Aims. We use new data from the High-resolution Coronal Imager (Hi-C) with its unprecedented spatial ...
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