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DOI10.1016/j.epsl.2020.116259
Corrigendum: “Analysis of geomagnetic field intensity variations in Mesopotamia during the third millennium BC with archeological implications” (Earth and Planetary Science Letters (2020) 537, (S0012821X20301266), (10.1016/j.epsl.2020.116183))
Gallet Y.; Fortin M.; Fournier A.; Le Goff M.; Livermore P.
发表日期2020
ISSN0012821X
卷号540
英文摘要The authors regret that an error occurred in Fig. 8a regarding the error bars associated with the intensity values expected at our reference site (i.e. Mari in Syria) as derived from the global geomagnetic field model called SHA.DIF.14k (orange curve; Pavón-Carrasco et al., 2014). This should appear as follows. The authors apologise for any inconvenience caused. © 2020 Elsevier B.V.
语种英语
来源期刊Earth and Planetary Science Letters
文献类型期刊论文
条目标识符http://gcip.llas.ac.cn/handle/2XKMVOVA/202593
作者单位Université de Paris, Institut de Physique du Globe de Paris, CNRS, Paris, France; Faculté des lettres et des sciences humaines, Département des sciences historiques, Université Laval, Québec, Canada; School of Earth & Environment, University of Leeds, Leeds, United Kingdom
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Gallet Y.,Fortin M.,Fournier A.,等. Corrigendum: “Analysis of geomagnetic field intensity variations in Mesopotamia during the third millennium BC with archeological implications” (Earth and Planetary Science Letters (2020) 537, (S0012821X20301266), (10.1016/j.epsl.2020.116183))[J],2020,540.
APA Gallet Y.,Fortin M.,Fournier A.,Le Goff M.,&Livermore P..(2020).Corrigendum: “Analysis of geomagnetic field intensity variations in Mesopotamia during the third millennium BC with archeological implications” (Earth and Planetary Science Letters (2020) 537, (S0012821X20301266), (10.1016/j.epsl.2020.116183)).Earth and Planetary Science Letters,540.
MLA Gallet Y.,et al."Corrigendum: “Analysis of geomagnetic field intensity variations in Mesopotamia during the third millennium BC with archeological implications” (Earth and Planetary Science Letters (2020) 537, (S0012821X20301266), (10.1016/j.epsl.2020.116183))".Earth and Planetary Science Letters 540(2020).
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