日本地球惑星科学連合2016年大会

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インターナショナルセッション(口頭発表)

セッション記号 S (固体地球科学) » S-EM 固体地球電磁気学

[S-EM05] Full vector geomagnetic and paleomagnetic secular variation: direction, intensity and dynamo simulations

2016年5月22日(日) 09:00 〜 10:30 105 (1F)

コンビーナ:*渋谷 秀敏(熊本大学大学院自然科学研究科)、山本 裕二(高知大学 海洋コア総合研究センター)、Paterson Greig(Institute of Geology and Geophysics Chinese Academy of Sciences)、Brown Maxwell(GFZ German Research Centre for Geosciences)、座長:Paterson Greig A(Institute of Geology and Geophysics, Chinese Academy of Sciences)、山本 裕二(高知大学 海洋コア総合研究センター)、福間 浩司(同志社大学理工学部環境システム学科)

09:20 〜 09:40

[SEM05-02] New Palaeosecular Variation Master Records for New Zealand – Applications for Dating and Field Modelling

★招待講演

*Gillian M Turner1Gino de Gelder2Jamie Howarth3Annika Greve1Rimpy Kinger1Ruth Corkill1Andreas Nilsson4Sean Fitzsimons5 (1.Victoria University of Wellington, New Zealand、2.Institut de Physique du Globe, Paris、3.Geological and Nuclear Sciences, New Zealand、4.Lund University, Sweden、5.Otago University, New Zealand)

キーワード:Palaeomagnetism, Secular variation, New Zealand

We present new palaeosecular variation master records for New Zealand on both archaeological and Holocene timescales. These have been compiled using continuous data from the detrital remanent magnetization of lake sediment cores with high-resolution C-14 based chronology, and are constrained and calibrated using directions and absolute palaeointensities obtained from the thermoremanent magnetizations of archaeological materials and volcanic rocks. All data has been “relocated” to a standard geographical location (40°S, 175°E) using a virtual geomagnetic pole (VGP) transformation. By a reciprocal VGP process, the master records can be used to calculate accurate palaeosecular variation records for all locations within the New Zealand region. The geomagnetic field alternates between active periods of high amplitude swings from 12000 to 8000 BP and over the past 4000 years, and a relatively inactive period between 8000 and 4000 BP. The current field (Dec = 21.5° E, Inc = - 65.4°, F = 55.4 micro T at 40°S, 175°E) represents a rare steep and easterly extreme in direction, but is close to average in intensity. The palaeointensity record mirrors to some extent the variation of the virtual axial geomagnetic moment seen in the global dataset, but shows some notable differences. We also investigate the effect of including the Holocene record in global spherical harmonic-based and regional field models.