Automated tracking of solar coronal loops and detection of their oscillations

Identification and tracking of solar coronal loops is key to understanding solar magnetic field. Slow and fast Magnetohydrodynamic oscillation of tracked loops from sequence 171Å extreme ultra – violet images was detected. The method was demonstrated using 171Å images taken by SDO/AIA on 14 August...

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Bibliographic Details
Main Authors: S. Taran, H. Safari, N. Farhangh
Format: Article
Language:English
Published: Isfahan University of Technology 2014-04-01
Series:Iranian Journal of Physics Research
Subjects:
sun
Online Access:http://ijpr.iut.ac.ir/browse.php?a_code=A-10-1-641&slc_lang=en&sid=1