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Absolute palaeointensity variation during a precursor to the Matuyama-Brunhes transition recorded in Chilean lavas
Following a detailed radioisotropic dating and palaeomagnetic investigation of transitional polarity lava flows of the Tatara-San Pedro volcanic complex (36°S, 71°W), in the Quebrada Turbia valley, Central Chile ( Brown et al., 2004), palaeointensity analysis has been carried out to complete a chara...
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Published in: | Physics of the earth and planetary interiors 2007-06, Vol.162 (1), p.61-72 |
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description | Following a detailed radioisotropic dating and palaeomagnetic investigation of transitional polarity lava flows of the Tatara-San Pedro volcanic complex (36°S, 71°W), in the Quebrada Turbia valley, Central Chile (
Brown et al., 2004), palaeointensity analysis has been carried out to complete a characterisation of the full geomagnetic field vector during a period of transitional geomagnetic field behaviour at 791.7
±
3.0
ka, 16
ky before the full Matuyama-Brunhes transition (MBT). Seventy-one samples from 30 lava flows were analysed in total, with 34 found suitable for palaeointensity experiments. After conducting microwave palaeointensity experiments, 16 lava flows from two sections (2
km apart) yielded 31 successful individual palaeointensity determinations which record consistently weak field intensity values during the transitional directions (mean value of 5
±
1.1
μT from 11 flows), excluding a flow immediately above a reversed polarity flow). Palaeointensity values are nearly an order of magnitude lower than the overlying normal polarity lavas (ranging from 30 to 47
μT), and half the values recorded in the underlying reversed polarity lavas (7 and 13
μT). These post-transitional field high palaeointensity values and comparisons with relative palaeointensity records from sedimentary rocks suggest that the Quebrada Turbia lavas may document a partial record of the MBT precursor and the latter stages of the MBT itself. |
doi_str_mv | 10.1016/j.pepi.2007.03.003 |
format | article |
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Brown et al., 2004), palaeointensity analysis has been carried out to complete a characterisation of the full geomagnetic field vector during a period of transitional geomagnetic field behaviour at 791.7
±
3.0
ka, 16
ky before the full Matuyama-Brunhes transition (MBT). Seventy-one samples from 30 lava flows were analysed in total, with 34 found suitable for palaeointensity experiments. After conducting microwave palaeointensity experiments, 16 lava flows from two sections (2
km apart) yielded 31 successful individual palaeointensity determinations which record consistently weak field intensity values during the transitional directions (mean value of 5
±
1.1
μT from 11 flows), excluding a flow immediately above a reversed polarity flow). Palaeointensity values are nearly an order of magnitude lower than the overlying normal polarity lavas (ranging from 30 to 47
μT), and half the values recorded in the underlying reversed polarity lavas (7 and 13
μT). These post-transitional field high palaeointensity values and comparisons with relative palaeointensity records from sedimentary rocks suggest that the Quebrada Turbia lavas may document a partial record of the MBT precursor and the latter stages of the MBT itself.</description><identifier>ISSN: 0031-9201</identifier><identifier>EISSN: 1872-7395</identifier><identifier>DOI: 10.1016/j.pepi.2007.03.003</identifier><language>eng</language><publisher>Elsevier B.V</publisher><subject>Geomagnetic reversals ; Matuyama-Bruhnes transition ; Microwave technique ; Palaeointensity ; Palaeomagnetism</subject><ispartof>Physics of the earth and planetary interiors, 2007-06, Vol.162 (1), p.61-72</ispartof><rights>2007 Elsevier B.V.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a420t-e59dfb754b8d7dc4178189b0aa093077fd34fe8ca9ca8cb0444068b9525d01403</citedby><cites>FETCH-LOGICAL-a420t-e59dfb754b8d7dc4178189b0aa093077fd34fe8ca9ca8cb0444068b9525d01403</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids></links><search><creatorcontrib>Gratton, Martin N.</creatorcontrib><creatorcontrib>Shaw, John</creatorcontrib><creatorcontrib>Brown, Laurie L.</creatorcontrib><title>Absolute palaeointensity variation during a precursor to the Matuyama-Brunhes transition recorded in Chilean lavas</title><title>Physics of the earth and planetary interiors</title><description>Following a detailed radioisotropic dating and palaeomagnetic investigation of transitional polarity lava flows of the Tatara-San Pedro volcanic complex (36°S, 71°W), in the Quebrada Turbia valley, Central Chile (
Brown et al., 2004), palaeointensity analysis has been carried out to complete a characterisation of the full geomagnetic field vector during a period of transitional geomagnetic field behaviour at 791.7
±
3.0
ka, 16
ky before the full Matuyama-Brunhes transition (MBT). Seventy-one samples from 30 lava flows were analysed in total, with 34 found suitable for palaeointensity experiments. After conducting microwave palaeointensity experiments, 16 lava flows from two sections (2
km apart) yielded 31 successful individual palaeointensity determinations which record consistently weak field intensity values during the transitional directions (mean value of 5
±
1.1
μT from 11 flows), excluding a flow immediately above a reversed polarity flow). Palaeointensity values are nearly an order of magnitude lower than the overlying normal polarity lavas (ranging from 30 to 47
μT), and half the values recorded in the underlying reversed polarity lavas (7 and 13
μT). These post-transitional field high palaeointensity values and comparisons with relative palaeointensity records from sedimentary rocks suggest that the Quebrada Turbia lavas may document a partial record of the MBT precursor and the latter stages of the MBT itself.</description><subject>Geomagnetic reversals</subject><subject>Matuyama-Bruhnes transition</subject><subject>Microwave technique</subject><subject>Palaeointensity</subject><subject>Palaeomagnetism</subject><issn>0031-9201</issn><issn>1872-7395</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2007</creationdate><recordtype>article</recordtype><recordid>eNp9kE1r3DAURUVoodO0f6Arrbqz82TJkQ3dpEO_ICGbdi2epeeMBo_kSvLA_PvaTNdZPXjcc-Eexj4JqAWI-7tjPdPs6wZA1yBrAHnDdqLTTaVl375hu_Ujqr4B8Y69z_kIAEI2csfSw5DjtBTiM05I0YdCIfty4WdMHouPgbsl-fDCkc-J7JJyTLxEXg7En7AsFzxh9TUt4UCZl4QbvVFrNiZHjvvA9wc_EQY-4RnzB_Z2xCnTx__3lv35_u33_mf1-Pzj1_7hsULVQKmo7d046FYNndPOKqE70fUDIEIvQevRSTVSZ7G32NkBlFJw3w1927QOhAJ5yz5fe-cU_y6Uizn5bGmaMFBcshG9WnXpLdhcgzbFnBONZk7-hOliBJhNrzmaTa_Z9BqQZpW5Ql-uEK0Tzp6SydZTsOT8urwYF_1r-D8lyIYO</recordid><startdate>20070615</startdate><enddate>20070615</enddate><creator>Gratton, Martin N.</creator><creator>Shaw, John</creator><creator>Brown, Laurie L.</creator><general>Elsevier B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope></search><sort><creationdate>20070615</creationdate><title>Absolute palaeointensity variation during a precursor to the Matuyama-Brunhes transition recorded in Chilean lavas</title><author>Gratton, Martin N. ; Shaw, John ; Brown, Laurie L.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a420t-e59dfb754b8d7dc4178189b0aa093077fd34fe8ca9ca8cb0444068b9525d01403</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2007</creationdate><topic>Geomagnetic reversals</topic><topic>Matuyama-Bruhnes transition</topic><topic>Microwave technique</topic><topic>Palaeointensity</topic><topic>Palaeomagnetism</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Gratton, Martin N.</creatorcontrib><creatorcontrib>Shaw, John</creatorcontrib><creatorcontrib>Brown, Laurie L.</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><jtitle>Physics of the earth and planetary interiors</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Gratton, Martin N.</au><au>Shaw, John</au><au>Brown, Laurie L.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Absolute palaeointensity variation during a precursor to the Matuyama-Brunhes transition recorded in Chilean lavas</atitle><jtitle>Physics of the earth and planetary interiors</jtitle><date>2007-06-15</date><risdate>2007</risdate><volume>162</volume><issue>1</issue><spage>61</spage><epage>72</epage><pages>61-72</pages><issn>0031-9201</issn><eissn>1872-7395</eissn><abstract>Following a detailed radioisotropic dating and palaeomagnetic investigation of transitional polarity lava flows of the Tatara-San Pedro volcanic complex (36°S, 71°W), in the Quebrada Turbia valley, Central Chile (
Brown et al., 2004), palaeointensity analysis has been carried out to complete a characterisation of the full geomagnetic field vector during a period of transitional geomagnetic field behaviour at 791.7
±
3.0
ka, 16
ky before the full Matuyama-Brunhes transition (MBT). Seventy-one samples from 30 lava flows were analysed in total, with 34 found suitable for palaeointensity experiments. After conducting microwave palaeointensity experiments, 16 lava flows from two sections (2
km apart) yielded 31 successful individual palaeointensity determinations which record consistently weak field intensity values during the transitional directions (mean value of 5
±
1.1
μT from 11 flows), excluding a flow immediately above a reversed polarity flow). Palaeointensity values are nearly an order of magnitude lower than the overlying normal polarity lavas (ranging from 30 to 47
μT), and half the values recorded in the underlying reversed polarity lavas (7 and 13
μT). These post-transitional field high palaeointensity values and comparisons with relative palaeointensity records from sedimentary rocks suggest that the Quebrada Turbia lavas may document a partial record of the MBT precursor and the latter stages of the MBT itself.</abstract><pub>Elsevier B.V</pub><doi>10.1016/j.pepi.2007.03.003</doi><tpages>12</tpages></addata></record> |
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source | ScienceDirect Freedom Collection 2022-2024 |
subjects | Geomagnetic reversals Matuyama-Bruhnes transition Microwave technique Palaeointensity Palaeomagnetism |
title | Absolute palaeointensity variation during a precursor to the Matuyama-Brunhes transition recorded in Chilean lavas |
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