Correction: The effect of initial and prior models on phase tensor inversion of distorted magnetotelluric data (Earth, Planets and Space, (2022), 74, 1, (51), 10.1186/s40623-022-01611-8)
dc.contributor.author | Rung‐Arunwan T. | |
dc.contributor.author | Siripunvaraporn W. | |
dc.contributor.author | Utada H. | |
dc.contributor.other | Mahidol University | |
dc.date.accessioned | 2023-12-08T18:01:37Z | |
dc.date.available | 2023-12-08T18:01:37Z | |
dc.date.issued | 2023-12-01 | |
dc.description.abstract | In the version of this article that was originally published (Rung-Arunwan et al. 2022), there were errors in the captions of Figs. 9, 10, 11, and 12. The caption of Fig. 9 should have been: “Data RMS misfits and the model recovery factors of the inverted models shown in Fig. 8 obtained by inverting PTATAN (black), ZLOGA (red), and ZLOGO (blue).” The caption of Fig. 10 should have been: “NS cross-sections at the easting of 200 m of the models inverted from all elements of the distorted MT impedance tensor (ZLOGA) using different initial models.” The caption of Fig. 11 should have been: “NS cross-sections at the easting of 200 m of the models inverted from the off-diagonal elements (ZLOGO) of the distorted MT impedance tensor using differential initial models.” The caption of Fig. 12 should have been: “Data RMS misfits and the model recovery factors for different initial (prior) models obtained from inverting a all elements (ZLOGA) and b off-diagonal elements (ZLOGO) of the distorted MT impedance tensor. Orange, red, and blue curves correspond to three different levels of distortion, as represented by SD = 0.1, 0.3, and 0.5, respectively.” The authors apologise for these errors. The original article (Rung-Arunwan et al. 2022) has been updated. | |
dc.identifier.citation | Earth, Planets and Space Vol.75 No.1 (2023) | |
dc.identifier.doi | 10.1186/s40623-023-01922-4 | |
dc.identifier.eissn | 18805981 | |
dc.identifier.issn | 13438832 | |
dc.identifier.scopus | 2-s2.0-85177802320 | |
dc.identifier.uri | https://repository.li.mahidol.ac.th/handle/20.500.14594/91303 | |
dc.rights.holder | SCOPUS | |
dc.subject | Earth and Planetary Sciences | |
dc.title | Correction: The effect of initial and prior models on phase tensor inversion of distorted magnetotelluric data (Earth, Planets and Space, (2022), 74, 1, (51), 10.1186/s40623-022-01611-8) | |
dc.type | Erratum | |
mu.datasource.scopus | https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85177802320&origin=inward | |
oaire.citation.issue | 1 | |
oaire.citation.title | Earth, Planets and Space | |
oaire.citation.volume | 75 | |
oairecerif.author.affiliation | The University of Tokyo | |
oairecerif.author.affiliation | Mahidol University | |
oairecerif.author.affiliation | Ministry of Higher Education, Science, Research and Innovation | |
oairecerif.author.affiliation | Ltd. |