Erratum: A Study of Sunspot 3 Minute Oscillations Using ALMA and GST (Astrophysical Journal (2022) 924 (100) DOI: 10.3847/1538-4357/ac34f7)
Document Type
Syllabus
Publication Date
7-1-2022
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).
Identifier
85135339797 (Scopus)
Publication Title
Astrophysical Journal
External Full Text Location
https://doi.org/10.3847/1538-4357/ac7c1c
e-ISSN
15384357
ISSN
0004637X
Issue
2
Volume
933
Recommended Citation
Chai, Yi; Gary, Dale E.; Reardon, Kevin P.; and Yurchyshyn, Vasyl, "Erratum: A Study of Sunspot 3 Minute Oscillations Using ALMA and GST (Astrophysical Journal (2022) 924 (100) DOI: 10.3847/1538-4357/ac34f7)" (2022). Faculty Publications. 2844.
https://digitalcommons.njit.edu/fac_pubs/2844