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

doi:10.1051/0004-6361/202141451e

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

HAO Administrative Office

Max Planck Institute for Solar System Research
Kyung Hee University

Research output: Contribution to journal › Comment/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 ν_eff= 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	https://doi.org/10.1051/0004-6361/202141451e
State	Published - Jan 1 2023

Keywords

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

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10.1051/0004-6361/202141451e

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

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.",

keywords = "Errata, addenda, Magnetohydrodynamics (MHD), Sun: corona, Sun: magnetic fields",

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T2 - A solar coronal loop in a box: Energy generationand heating (A&A (2022) 658 (A45) DOI: 10.1051/0004-6361/202141451)

AU - Breu, C.

AU - Peter, H.

AU - Cameron, R.

AU - Solanki, S. K.

AU - Przybylski, D.

AU - Rempel, M.

AU - Chitta, L. P.

PY - 2023/1/1

Y1 - 2023/1/1

N2 - 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.

AB - 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.

KW - Errata, addenda

KW - Magnetohydrodynamics (MHD)

KW - Sun: corona

KW - Sun: magnetic fields

UR - https://www.scopus.com/pages/publications/85145466759

U2 - 10.1051/0004-6361/202141451e

DO - 10.1051/0004-6361/202141451e

M3 - Comment/debate

AN - SCOPUS:85145466759

SN - 0004-6361

VL - 669

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

M1 - C1

ER -

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

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Keywords

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