Loading…
Long-term variations in palaeointensity
We compile a dataset of reliable palaeointensity estimates based both on published work and on new data from basaltic glass. The basaltic glass data more than double the number of reliable (Thellier method with pTRM checks) palaeointensity estimates available. Although the new data dramatically impr...
Saved in:
Published in: | Philosophical transactions of the Royal Society of London. Series A: Mathematical, physical, and engineering sciences physical, and engineering sciences, 2000-03, Vol.358 (1768), p.1065-1088 |
---|---|
Main Authors: | , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
cited_by | cdi_FETCH-LOGICAL-a493t-9562e5ea124fe94c8dd5ae6d13222d494332469f4bd535e5a2d68aed9d6a59b33 |
---|---|
cites | cdi_FETCH-LOGICAL-a493t-9562e5ea124fe94c8dd5ae6d13222d494332469f4bd535e5a2d68aed9d6a59b33 |
container_end_page | 1088 |
container_issue | 1768 |
container_start_page | 1065 |
container_title | Philosophical transactions of the Royal Society of London. Series A: Mathematical, physical, and engineering sciences |
container_volume | 358 |
creator | Selkin, Peter A. Tauxe, Lisa |
description | We compile a dataset of reliable palaeointensity estimates based both on published work and on new data from basaltic glass. The basaltic glass data more than double the number of reliable (Thellier method with pTRM checks) palaeointensity estimates available. Although the new data dramatically improve both spatial and temporal coverage, there is still a strong bias toward the most recent past. The last 0.3 Ma claim over half of the data in our combined database. We therefore divide the data into two groups, the densely sampled last 0.3 Myr and the more sparsely sampled period of time comprising roughly half of the data from 0.3 to 300 Ma. Separating them in this way, it is clear that the dipole moment of the Earth over the past 0.3 Myr (ca.8 × 1022 A m2) is dramatically higher than the average dipole moment over the preceding 300 Myr (ca.5 × 1022 A m2). Inclusion of poor-quality results leads to an overestimate of the average dipole moment. Interestingly, no other significant changes in the distribution of dipole moments are evident over the 300 million year span of the data. |
doi_str_mv | 10.1098/rsta.2000.0574 |
format | article |
fullrecord | <record><control><sourceid>jstor_highw</sourceid><recordid>TN_cdi_highwire_royalsociety_roypta_358_1768_1065</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><jstor_id>2666746</jstor_id><sourcerecordid>2666746</sourcerecordid><originalsourceid>FETCH-LOGICAL-a493t-9562e5ea124fe94c8dd5ae6d13222d494332469f4bd535e5a2d68aed9d6a59b33</originalsourceid><addsrcrecordid>eNp9UEtP3DAQjlArQSlXTj3siZ6y9TvxjRa1ULEVPdBqbyMTT8DbbBxsL23-fR1SIXEol_FY32NmvqI4pmRJia4_hJjMkhFClkRWYq84oKKiJdOKvco9V6KUhK_3izcxbgihVEl2ULxf-f62TBi2iwcTnEnO93Hh-sVgOoPe9Qn76NL4tnjdmi7i0b_3sPjx5fP12UW5ujr_evZxVRqheSq1VAwlGspEi1o0tbXSoLKUM8as0IJzJpRuxY2VXKI0zKraoNVWGalvOD8sTmbfIfj7HcYEWxcb7DrTo99FoBWvKOM0E5czsQk-xoAtDMFtTRiBEpjygCkPmPKAKY8s4LMg-DFf4BuHaYSN34U-f_-vejerNjH58DSDKaUqoTJczrCLCf88wSb8ApU3lfCzFvBpTb_rNf8Gl5l_OvPv3O3dbxcQnm3zOLzxU-gJuKzzuSoXoiS0u66DwbbZgr5o4cchmzwT878KeaXV</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>17371231</pqid></control><display><type>article</type><title>Long-term variations in palaeointensity</title><source>JSTOR Archival Journals and Primary Sources Collection</source><source>Royal Society Publishing Jisc Collections Royal Society Journals Read & Publish Transitional Agreement 2025 (reading list)</source><creator>Selkin, Peter A. ; Tauxe, Lisa</creator><contributor>Gubbins, D. ; Kent, D. V. ; Laj, C. ; Laj, C. ; Gubbins, D. ; Kent, D. V.</contributor><creatorcontrib>Selkin, Peter A. ; Tauxe, Lisa ; Gubbins, D. ; Kent, D. V. ; Laj, C. ; Laj, C. ; Gubbins, D. ; Kent, D. V.</creatorcontrib><description>We compile a dataset of reliable palaeointensity estimates based both on published work and on new data from basaltic glass. The basaltic glass data more than double the number of reliable (Thellier method with pTRM checks) palaeointensity estimates available. Although the new data dramatically improve both spatial and temporal coverage, there is still a strong bias toward the most recent past. The last 0.3 Ma claim over half of the data in our combined database. We therefore divide the data into two groups, the densely sampled last 0.3 Myr and the more sparsely sampled period of time comprising roughly half of the data from 0.3 to 300 Ma. Separating them in this way, it is clear that the dipole moment of the Earth over the past 0.3 Myr (ca.8 × 1022 A m2) is dramatically higher than the average dipole moment over the preceding 300 Myr (ca.5 × 1022 A m2). Inclusion of poor-quality results leads to an overestimate of the average dipole moment. Interestingly, no other significant changes in the distribution of dipole moments are evident over the 300 million year span of the data.</description><identifier>ISSN: 1364-503X</identifier><identifier>EISSN: 1471-2962</identifier><identifier>DOI: 10.1098/rsta.2000.0574</identifier><language>eng</language><publisher>The Royal Society</publisher><subject>Arithmetic mean ; Datasets ; Drilling ; Estimation methods ; Geomagnetic fields ; Magnetic fields ; Magnetization ; Oceans ; Palaeointensity ; Palaeomagnetism ; Specimens ; Submarine Basaltic Glass ; Thelliers' Method</subject><ispartof>Philosophical transactions of the Royal Society of London. Series A: Mathematical, physical, and engineering sciences, 2000-03, Vol.358 (1768), p.1065-1088</ispartof><rights>Copyright 2000 The Royal Society</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a493t-9562e5ea124fe94c8dd5ae6d13222d494332469f4bd535e5a2d68aed9d6a59b33</citedby><cites>FETCH-LOGICAL-a493t-9562e5ea124fe94c8dd5ae6d13222d494332469f4bd535e5a2d68aed9d6a59b33</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.jstor.org/stable/pdf/2666746$$EPDF$$P50$$Gjstor$$H</linktopdf><linktohtml>$$Uhttps://www.jstor.org/stable/2666746$$EHTML$$P50$$Gjstor$$H</linktohtml><link.rule.ids>314,780,784,27923,27924,58237,58470</link.rule.ids></links><search><contributor>Gubbins, D.</contributor><contributor>Kent, D. V.</contributor><contributor>Laj, C.</contributor><contributor>Laj, C.</contributor><contributor>Gubbins, D.</contributor><contributor>Kent, D. V.</contributor><creatorcontrib>Selkin, Peter A.</creatorcontrib><creatorcontrib>Tauxe, Lisa</creatorcontrib><title>Long-term variations in palaeointensity</title><title>Philosophical transactions of the Royal Society of London. Series A: Mathematical, physical, and engineering sciences</title><description>We compile a dataset of reliable palaeointensity estimates based both on published work and on new data from basaltic glass. The basaltic glass data more than double the number of reliable (Thellier method with pTRM checks) palaeointensity estimates available. Although the new data dramatically improve both spatial and temporal coverage, there is still a strong bias toward the most recent past. The last 0.3 Ma claim over half of the data in our combined database. We therefore divide the data into two groups, the densely sampled last 0.3 Myr and the more sparsely sampled period of time comprising roughly half of the data from 0.3 to 300 Ma. Separating them in this way, it is clear that the dipole moment of the Earth over the past 0.3 Myr (ca.8 × 1022 A m2) is dramatically higher than the average dipole moment over the preceding 300 Myr (ca.5 × 1022 A m2). Inclusion of poor-quality results leads to an overestimate of the average dipole moment. Interestingly, no other significant changes in the distribution of dipole moments are evident over the 300 million year span of the data.</description><subject>Arithmetic mean</subject><subject>Datasets</subject><subject>Drilling</subject><subject>Estimation methods</subject><subject>Geomagnetic fields</subject><subject>Magnetic fields</subject><subject>Magnetization</subject><subject>Oceans</subject><subject>Palaeointensity</subject><subject>Palaeomagnetism</subject><subject>Specimens</subject><subject>Submarine Basaltic Glass</subject><subject>Thelliers' Method</subject><issn>1364-503X</issn><issn>1471-2962</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2000</creationdate><recordtype>article</recordtype><recordid>eNp9UEtP3DAQjlArQSlXTj3siZ6y9TvxjRa1ULEVPdBqbyMTT8DbbBxsL23-fR1SIXEol_FY32NmvqI4pmRJia4_hJjMkhFClkRWYq84oKKiJdOKvco9V6KUhK_3izcxbgihVEl2ULxf-f62TBi2iwcTnEnO93Hh-sVgOoPe9Qn76NL4tnjdmi7i0b_3sPjx5fP12UW5ujr_evZxVRqheSq1VAwlGspEi1o0tbXSoLKUM8as0IJzJpRuxY2VXKI0zKraoNVWGalvOD8sTmbfIfj7HcYEWxcb7DrTo99FoBWvKOM0E5czsQk-xoAtDMFtTRiBEpjygCkPmPKAKY8s4LMg-DFf4BuHaYSN34U-f_-vejerNjH58DSDKaUqoTJczrCLCf88wSb8ApU3lfCzFvBpTb_rNf8Gl5l_OvPv3O3dbxcQnm3zOLzxU-gJuKzzuSoXoiS0u66DwbbZgr5o4cchmzwT878KeaXV</recordid><startdate>20000315</startdate><enddate>20000315</enddate><creator>Selkin, Peter A.</creator><creator>Tauxe, Lisa</creator><general>The Royal Society</general><scope>BSCLL</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope></search><sort><creationdate>20000315</creationdate><title>Long-term variations in palaeointensity</title><author>Selkin, Peter A. ; Tauxe, Lisa</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a493t-9562e5ea124fe94c8dd5ae6d13222d494332469f4bd535e5a2d68aed9d6a59b33</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2000</creationdate><topic>Arithmetic mean</topic><topic>Datasets</topic><topic>Drilling</topic><topic>Estimation methods</topic><topic>Geomagnetic fields</topic><topic>Magnetic fields</topic><topic>Magnetization</topic><topic>Oceans</topic><topic>Palaeointensity</topic><topic>Palaeomagnetism</topic><topic>Specimens</topic><topic>Submarine Basaltic Glass</topic><topic>Thelliers' Method</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Selkin, Peter A.</creatorcontrib><creatorcontrib>Tauxe, Lisa</creatorcontrib><collection>Istex</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><jtitle>Philosophical transactions of the Royal Society of London. Series A: Mathematical, physical, and engineering sciences</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Selkin, Peter A.</au><au>Tauxe, Lisa</au><au>Gubbins, D.</au><au>Kent, D. V.</au><au>Laj, C.</au><au>Laj, C.</au><au>Gubbins, D.</au><au>Kent, D. V.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Long-term variations in palaeointensity</atitle><jtitle>Philosophical transactions of the Royal Society of London. Series A: Mathematical, physical, and engineering sciences</jtitle><date>2000-03-15</date><risdate>2000</risdate><volume>358</volume><issue>1768</issue><spage>1065</spage><epage>1088</epage><pages>1065-1088</pages><issn>1364-503X</issn><eissn>1471-2962</eissn><abstract>We compile a dataset of reliable palaeointensity estimates based both on published work and on new data from basaltic glass. The basaltic glass data more than double the number of reliable (Thellier method with pTRM checks) palaeointensity estimates available. Although the new data dramatically improve both spatial and temporal coverage, there is still a strong bias toward the most recent past. The last 0.3 Ma claim over half of the data in our combined database. We therefore divide the data into two groups, the densely sampled last 0.3 Myr and the more sparsely sampled period of time comprising roughly half of the data from 0.3 to 300 Ma. Separating them in this way, it is clear that the dipole moment of the Earth over the past 0.3 Myr (ca.8 × 1022 A m2) is dramatically higher than the average dipole moment over the preceding 300 Myr (ca.5 × 1022 A m2). Inclusion of poor-quality results leads to an overestimate of the average dipole moment. Interestingly, no other significant changes in the distribution of dipole moments are evident over the 300 million year span of the data.</abstract><pub>The Royal Society</pub><doi>10.1098/rsta.2000.0574</doi><tpages>24</tpages></addata></record> |
fulltext | fulltext |
identifier | ISSN: 1364-503X |
ispartof | Philosophical transactions of the Royal Society of London. Series A: Mathematical, physical, and engineering sciences, 2000-03, Vol.358 (1768), p.1065-1088 |
issn | 1364-503X 1471-2962 |
language | eng |
recordid | cdi_highwire_royalsociety_roypta_358_1768_1065 |
source | JSTOR Archival Journals and Primary Sources Collection; Royal Society Publishing Jisc Collections Royal Society Journals Read & Publish Transitional Agreement 2025 (reading list) |
subjects | Arithmetic mean Datasets Drilling Estimation methods Geomagnetic fields Magnetic fields Magnetization Oceans Palaeointensity Palaeomagnetism Specimens Submarine Basaltic Glass Thelliers' Method |
title | Long-term variations in palaeointensity |
url | http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-10T14%3A15%3A39IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-jstor_highw&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Long-term%20variations%20in%20palaeointensity&rft.jtitle=Philosophical%20transactions%20of%20the%20Royal%20Society%20of%20London.%20Series%20A:%20Mathematical,%20physical,%20and%20engineering%20sciences&rft.au=Selkin,%20Peter%20A.&rft.date=2000-03-15&rft.volume=358&rft.issue=1768&rft.spage=1065&rft.epage=1088&rft.pages=1065-1088&rft.issn=1364-503X&rft.eissn=1471-2962&rft_id=info:doi/10.1098/rsta.2000.0574&rft_dat=%3Cjstor_highw%3E2666746%3C/jstor_highw%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-a493t-9562e5ea124fe94c8dd5ae6d13222d494332469f4bd535e5a2d68aed9d6a59b33%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=17371231&rft_id=info:pmid/&rft_jstor_id=2666746&rfr_iscdi=true |