Gradient Path Labelling method and tracking method for calculation of solar differential rotation using coronal bright points

Author:

Dorotovič I.,Coelho A.,Rybák J.,Mora A.,Ribeiro R.ORCID

Funder

SRDA (APVV) Bratislava

FCT Lisbon

Scientific Grant Agency

European Regional Development Fund.

Publisher

Elsevier BV

Subject

Computer Science Applications,Astronomy and Astrophysics,Space and Planetary Science

Reference34 articles.

1. Identification of photospheric activity features from SOHO/MDI data using the ASAP tool;Ashamari;J. Space Weather Space Clim.,2015

2. The morphological approach to segmentation: the watershed transformation;Beucher,1993

3. Preliminary results on the solar rotation determined tracing SDO/AIA coronal bright points;Brajša;Cent. Eur. Astrophys. Bull.,2014

4. Solar differential rotation determined by tracing coronal bright points in SOHO-EIT images. I. Interactive and automatic methods of data reduction;Brajša;Astron. Astrophys.,2001

5. Proper motions of coronal bright points;Brajša;Cent. Eur. Astrophys. Bull.,2008

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1. CBP detection using template matching to compute the solar rotation profile;2024 8th International Young Engineers Forum on Electrical and Computer Engineering (YEF-ECE);2024-07-05

2. A Solar-cycle Study of Coronal Rotation: Large Variations, Rapid Changes, and Implications for Solar-wind Models;The Astrophysical Journal;2022-03-01

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