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In this paper, we study the scaling relations for the triggering of the fast, or “ideal,” tearing instability starting from equilibrium configurations relevant to astrophysical as well as laboratory plasmas that differ from the simple Harris current sheet configuration.
This paper reports initial results from the analysis of this deep-field image sequence. In Section 2 , we describe the data from the COR2 deep-field campaign and how we prepared them. In Section 3 , we derive quantitative results on the structuring of the outer corona and discuss the wind-speed results created during data preparation.
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