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    Please use this identifier to cite or link to this item: http://utaipeir.lib.utaipei.edu.tw/dspace/handle/987654321/2619


    Title: Astronomically calibrated ages for geomagnetic reversals within the Matuyama chron
    Authors: Chorng-Shern Horng
    Meng-Yang Lee
    Heiko P¨alike
    Kuo-Yen Wei
    Wen-Tzong Liang
    Yoshiyuki Iizuka
    Masayuki Torii
    飯塚義之
    李孟陽
    梁文宗
    Contributors: 臺北市立教育大學自然科學系
    Date: 2002
    Issue Date: 2009-07-31 10:34:39 (UTC+8)
    Abstract: We present a magnetostratigraphic record from the western Philippine Sea that is tied to a marine δ18O record for
    the past 2.14 million years. The ages of geomagnetic reversals were astronomically calibrated by tuning the oxygen
    isotopic stratigraphy, yielding a chronology for the following subchrons: Matuyama/Brunhes boundary, 781±3 ka
    (slightly above δ18O Stage 19.3); top of the Santa Rosa polarity interval, 920 ± 2 ka (Stage 23/24); base of the
    Santa Rosa polarity interval, 925 ± 1 ka (Stage 24); top of the Jaramillo subchron, 988 ± 3 ka (Stage 27); base of
    the Jaramillo subchron, 1072 ± 2 ka (Stage 31); top of the Cobb Mountain subchron, 1173 ± 4 ka (Stage 35/36);
    base of the Cobb Mountain subchron, 1185 ± 5 ka (Stage 36); top of the Olduvai subchron, 1778 ± 3 ka (Stage
    63/64); base of the Olduvai subchron, 1945 ± 4 ka (Stage 71/72); top of the R´eunion II subchron, 2118 ± 3 ka
    (Stage 80/81); and base of the R´eunion II subchron, 2133 ± 5 ka (Stage 81). This astronomically calibrated
    chronology independently confirms the ages of major reversals in recently published astronomically calibrated
    polarity timescales for the Matuyama chron. It also provides the first astronomically calibrated dates for the lower
    and upper reversals associated with the Cobb Mountain and Santa Rosa polarity intervals, respectively.
    Relation: Earth Planets Space, 54, p.679–690
    Appears in Collections:[Department of Applied Physics and Chemistry] Periodical Articles

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