Erratum: A Study of Sunspot 3 Minute Oscillations Using ALMA and GST (Astrophysical Journal (2022) 924 (100) DOI: 10.3847/1538-4357/ac34f7)

Yi Chai; Dale E. Gary; Kevin P. Reardon; Vasyl Yurchyshyn

doi:10.3847/1538-4357/ac7c1c

Erratum: A Study of Sunspot 3 Minute Oscillations Using ALMA and GST (Astrophysical Journal (2022) 924 (100) DOI: 10.3847/1538-4357/ac34f7)

Yi Chai
, Dale E. Gary
, Kevin P. Reardon
, Vasyl Yurchyshyn

Research output: Contribution to journal › Comment/debate › peer-review

1 Scopus citations

Abstract

The published article used the RH code (Rybicki & Hummer 1991, 1992; Uitenbroek 2000) to calculate emergent intensity at millimeter wavelengths from a model solar atmosphere. In calculating the brightness temperature from this emergent intensity, we inadvertently omitted the factor 2 in the Rayleigh Jeans approximation of the Planck function, which is correctly written as (Formula Presented) (Figure Presented).

Original language	English (US)
Article number	247
Journal	Astrophysical Journal
Volume	933
Issue number	2
DOIs	https://doi.org/10.3847/1538-4357/ac7c1c
State	Published - Jul 1 2022

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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title = "Erratum: A Study of Sunspot 3 Minute Oscillations Using ALMA and GST (Astrophysical Journal (2022) 924 (100) DOI: 10.3847/1538-4357/ac34f7)",

abstract = "The published article used the RH code (Rybicki \& Hummer 1991, 1992; Uitenbroek 2000) to calculate emergent intensity at millimeter wavelengths from a model solar atmosphere. In calculating the brightness temperature from this emergent intensity, we inadvertently omitted the factor 2 in the Rayleigh Jeans approximation of the Planck function, which is correctly written as (Formula Presented) (Figure Presented).",

author = "Yi Chai and Gary, \{Dale E.\} and Reardon, \{Kevin P.\} and Vasyl Yurchyshyn",

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AU - Chai, Yi

AU - Gary, Dale E.

AU - Reardon, Kevin P.

AU - Yurchyshyn, Vasyl

PY - 2022/7/1

Y1 - 2022/7/1

N2 - The published article used the RH code (Rybicki & Hummer 1991, 1992; Uitenbroek 2000) to calculate emergent intensity at millimeter wavelengths from a model solar atmosphere. In calculating the brightness temperature from this emergent intensity, we inadvertently omitted the factor 2 in the Rayleigh Jeans approximation of the Planck function, which is correctly written as (Formula Presented) (Figure Presented).

AB - The published article used the RH code (Rybicki & Hummer 1991, 1992; Uitenbroek 2000) to calculate emergent intensity at millimeter wavelengths from a model solar atmosphere. In calculating the brightness temperature from this emergent intensity, we inadvertently omitted the factor 2 in the Rayleigh Jeans approximation of the Planck function, which is correctly written as (Formula Presented) (Figure Presented).

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UR - https://www.scopus.com/pages/publications/85135339797#tab=citedBy

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DO - 10.3847/1538-4357/ac7c1c

M3 - Comment/debate

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Erratum: A Study of Sunspot 3 Minute Oscillations Using ALMA and GST (Astrophysical Journal (2022) 924 (100) DOI: 10.3847/1538-4357/ac34f7)

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