Abstract
The scales on the images of the current density in the original version of the paper were missing a factor of c. The estimated value for the effective diffusivity needs to be corrected by a factor of 4π and should be replaced by νeff= 1.6×1011cm2s-1. Finally, the units on the y-axis of Fig. 16 should have been DN pix-1s-1instead of DN pix s. The new versions of the figures presented here have been corrected. These corrections do not affect the conclusions of the original paper.
| Original language | English |
|---|---|
| Article number | C1 |
| Journal | Astronomy and Astrophysics |
| Volume | 669 |
| DOIs |
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| State | Published - Jan 1 2023 |
Keywords
- Errata, addenda
- Magnetohydrodynamics (MHD)
- Sun: corona
- Sun: magnetic fields