What is it about?
It is a graphical user interface that let to users calculate proper motions in time series of solar data sets.
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Why is it important?
It is a easy and practical way to get information about for example photospheric proper motions on the Sun.
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This page is a summary of: A Python-based interface to examine motions in time series of solar images, Proceedings of the International Astronomical Union, October 2016, Cambridge University Press,
DOI: 10.1017/s1743921317003568.
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