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.
Taran,S. and Safari,H. (2019). Identification of solar coronal loops based on moments of image. Iranian Journal of Physics Research, 12(3), 231-236.
MLA
Taran,S. , and Safari,H. . "Identification of solar coronal loops based on moments of image", Iranian Journal of Physics Research, 12, 3, 2019, 231-236.
HARVARD
Taran S., Safari H. (2019). 'Identification of solar coronal loops based on moments of image', Iranian Journal of Physics Research, 12(3), pp. 231-236.
CHICAGO
S. Taran and H. Safari, "Identification of solar coronal loops based on moments of image," Iranian Journal of Physics Research, 12 3 (2019): 231-236,
VANCOUVER
Taran S., Safari H. Identification of solar coronal loops based on moments of image. Dear user; Recently we have changed our software to Sinaweb. If you had already registered with the old site, you may use the same USERNAME but you need to change your password. To do so at the first use, please choose, 2019; 12(3): 231-236.
