No abstract

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This is a PDF file of an unedited manuscript that has been accepted for publication. As a service to our customers we are providing this early version of the manuscript. The manuscript will undergo copyediting, typesetting, and review of the resulting proof before it is published in its final form. Please note that during the production process errors may be discovered which could affect the content, and all legal disclaimers that apply to the journal pertain. reverse directions were sampled from flows ranging between 1.9 and 0.9 Ma, this can be interpreted as an 31 interval of low paleomagnetic secular variation. Additional data, also with accurate time constraints, are 32 obviously needed to better support this observation. Finally, no convincing evidence for a complex time average 33 field significantly different from the axial dipole can be supported by this study for the last 2 Myr. 34 35