Astronomically calibrated ages for geomagnetic reversals within the Matuyama chron
| Type | Article | ||||||||
|---|---|---|---|---|---|---|---|---|---|
| Date | 2002 | ||||||||
| Language | English | ||||||||
| Author(s) | Horng Cs1, Lee My1, Palike H2, Wei Ky3, Liang Wt1, Lizuka Y1, Torii M4 | ||||||||
| Affiliation(s) | 1 : Acad Sinica, Inst Earth Sci, Taipei 115, Taiwan. 2 : Univ Cambridge, Dept Earth Sci, Godwin Inst, Cambridge CB2 3RS, England. 3 : Natl Taiwan Univ, Dept Geosci, Taipei 10764, Taiwan. 4 : Okayama Univ Sci, Fac Informat, Dept Bioshere Geosphere Syst Sci, Okayama 7000005, Japan. |
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| Source | Earth Planets And Space (1343-8832) (Terra Scientific Publ Co), 2002 , Vol. 54 , N. 6 , P. 679-690 | ||||||||
| DOI | 10.1186/BF03351719 | ||||||||
| WOS© Times Cited | 101 | ||||||||
| Abstract | We present a magnetostratigraphic record from the western Philippine Sea that is tied to a marine delta(18)O 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 delta(18)O 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 3 1); top of the Cobb Mountain subchron, 1173 +/- 4 ka (Stage 35/36); base of the Cobb Mountain subehron, 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 Reunion II subchron, 2118 +/-3 ka. (Stage 80/81); and base of the Reunion 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. | ||||||||
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