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Correction to: Solar Physics (2015) 290: 3221–3256(Article I) https://doi.org/10.1007/s11207-015-0792-y
In the first paragraph of Section 2, we gave an end date of 2001:
This has been corrected to 2011.
In Section 3.3 it was stated that we use \(\Delta m = m - m^{\prime}\) in the range \(\pm 15\):
A code inspection has revealed that a parameter was not set correctly and that a range of \(\pm 10\) was used.
In Equation 26 we gave integration limits of 0 to 1:
The upper integration limit has been changed to \(r_{\rm max}\) (which is slightly larger than 1.0) and the associated text has been updated.
Equation 28 also used this integration limit and did not include weighting terms:
A code inspection has revealed that the default regularization used by the inversion code includes weighting terms of \(r\) for the first term and \(r^{-4}\) for the second. This has been corrected, the equation has been reformatted to correct the integrals, and the associated text updated.
With these changes the relevant parts of the analysis performed in Article I are now correctly described.
We note that Article II (Larson and Schou, 2018) refers back to Article I and that the same inaccuracies are thus indirectly present there.
Finally we wish to call the reader’s attention to the fact that a small fraction of the fitted modes appear to be affected by a systematic error during the times when MDI had a low duty cycle (A. Kosovichev and K. Mandal, private communication, 2019, 2023). In particular, the series with starting days of 3952, 4096, 4168, and 4240 show apparent artifacts for a number of modes within about 300 μHz of 3500 μHz for \(\ell \ge 30\). The problem appears to be due to an unusual gap structure that is not being filled correctly. As the exact cause is not understood, caution is warranted for all modes in any timeseries where the gap-filling results in a substantially increased duty cycle (see Table 1 of Article I), which also includes the series starting on day 6472.
References
Larson, T.P., Schou, J.: 2015, Improved helioseismic analysis of medium-\(\ell \) data from the Michelson Doppler Imager (Article I). Solar Phys. 290, 3221. DOI. ADS.
Larson, T.P., Schou, J.: 2018, Global-mode analysis of full-disk data from the Michelson Doppler Imager and the Helioseismic and Magnetic Imager (Article II). Solar Phys. 293, 29. DOI. ADS.
Acknowledgments
T.P. Larson would like to thank the Max Planck Institute for Solar System Research for supporting a visit there in July 2023, during which the most important of these errors was discovered.
Funding
T.P. Larson is funded by NASA Contract NAS5-02139.
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Larson, T.P., Schou, J. Correction to: Improved Helioseismic Analysis of Medium-\(\ell \) Data from the Michelson Doppler Imager. Sol Phys 299, 61 (2024). https://doi.org/10.1007/s11207-024-02258-2
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DOI: https://doi.org/10.1007/s11207-024-02258-2