A solar coronal loop in a box: Energy generation and heating

Open Access

This article has an erratum: [https://doi.org/10.1051/0004-6361/202141451e]

Fig. 6.

Normalized intensity integrated over the coronal part of the simulation domain as a function of time. The vertical dashed lines highlight the same strong heating events as in Fig. 5. For a discussion of the time evolution see Sects. 3.1 and 4.1.

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