Erratum: A solar coronal loop in a box: Energy generationand heating (A&A (2022) 658 (A45) DOI: 10.1051/0004-6361/202141451)

  • C. Breu
  • , H. Peter
  • , R. Cameron
  • , S. K. Solanki
  • , D. Przybylski
  • , M. Rempel
  • , L. P. Chitta

Research output: Contribution to journalComment/debate

1 Scopus citations

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 languageEnglish
Article numberC1
JournalAstronomy and Astrophysics
Volume669
DOIs
StatePublished - Jan 1 2023

Keywords

  • Errata, addenda
  • Magnetohydrodynamics (MHD)
  • Sun: corona
  • Sun: magnetic fields

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