Amplitudes of oceanic magnetic anomalies and the chemistry of oceanic crust: Synthesis and review of 'magnetic telechemistry'
A growing body of evidence suggests that certain areas of high-amplitude (H) sea-floor spreading-type magnetic anomalies reflect FeTi-enriched basalts of high remanent magnetization. A worldwide tabulation of these 'H-zones' is presented, together with a review of pertinent geochemical, ro...
Published in: | Canadian Journal of Earth Sciences |
---|---|
Main Author: | |
Format: | Article in Journal/Newspaper |
Language: | English |
Published: |
Canadian Science Publishing
1979
|
Subjects: | |
Online Access: | http://dx.doi.org/10.1139/e79-210 http://www.nrcresearchpress.com/doi/pdf/10.1139/e79-210 |
id |
crcansciencepubl:10.1139/e79-210 |
---|---|
record_format |
openpolar |
spelling |
crcansciencepubl:10.1139/e79-210 2023-12-17T10:26:44+01:00 Amplitudes of oceanic magnetic anomalies and the chemistry of oceanic crust: Synthesis and review of 'magnetic telechemistry' Vogt, P. R. 1979 http://dx.doi.org/10.1139/e79-210 http://www.nrcresearchpress.com/doi/pdf/10.1139/e79-210 en eng Canadian Science Publishing http://www.nrcresearchpress.com/page/about/CorporateTextAndDataMining Canadian Journal of Earth Sciences volume 16, issue 12, page 2236-2262 ISSN 0008-4077 1480-3313 General Earth and Planetary Sciences journal-article 1979 crcansciencepubl https://doi.org/10.1139/e79-210 2023-11-19T13:39:28Z A growing body of evidence suggests that certain areas of high-amplitude (H) sea-floor spreading-type magnetic anomalies reflect FeTi-enriched basalts of high remanent magnetization. A worldwide tabulation of these 'H-zones' is presented, together with a review of pertinent geochemical, rock magnetic, and deep-tow data relevant to the hypothesis of magnetic telechemistry.' H-zones are found in two tectonic settings: (1) along 10 2 –10 3 km long sections of spreading axis close to hot spots; and (2) in narrow bands extending a few hundred kilometres along the edges of some fracture zones. Amplitudes in both provinces are 1.5 to 5, typically 2 to 3 times normal, and the hot spot H-zones are known from spreading half-rates of 0.6 to 3.7 cm yr −1 The highest amplitudes, magnetizations, and FeTi enrichment (up to 15–18% FeO T and 2–3% TiO 2 ) seem to occur where both provinces overlap, i.e., where fracture zones occur near hot spots, for example along the Blanco Fracture Zone south of the Juan de Fuca hot spot and along the Inca Fracture Zone east of the Galapagos hot spot. The FeTi enrichment appears to reflect shallow-depth crystal fractionation (plagioclase, augite, and olivine), which is more extensive near hot spots, and more generally for fast-spreading ridges. H-zones presently affect at least 2.6 × 10 3 km, or 6.5% of the Mid-Ocean Ridge axis. However, the total known H-area of 8.5 × 10 5 km 2 represents only 0.3% of oceanic crust. This suggests that older H-zones remain to be discovered, or/and that conditions favoring the formation of FeTi basalt and H-anomalies are more prevalent now than they have been on the average for the last 10 8 years. Evidence for the latter is provided by the known expansion of the magnetically well surveyed Juan de Fuca, Galapagos, and Yermak (Arctic) H-zones in the last 5 million years. Article in Journal/Newspaper Arctic Canadian Science Publishing (via Crossref) Arctic Galapagos Blanco ENVELOPE(-55.233,-55.233,-61.250,-61.250) Inca ENVELOPE(-59.194,-59.194,-62.308,-62.308) Canadian Journal of Earth Sciences 16 12 2236 2262 |
institution |
Open Polar |
collection |
Canadian Science Publishing (via Crossref) |
op_collection_id |
crcansciencepubl |
language |
English |
topic |
General Earth and Planetary Sciences |
spellingShingle |
General Earth and Planetary Sciences Vogt, P. R. Amplitudes of oceanic magnetic anomalies and the chemistry of oceanic crust: Synthesis and review of 'magnetic telechemistry' |
topic_facet |
General Earth and Planetary Sciences |
description |
A growing body of evidence suggests that certain areas of high-amplitude (H) sea-floor spreading-type magnetic anomalies reflect FeTi-enriched basalts of high remanent magnetization. A worldwide tabulation of these 'H-zones' is presented, together with a review of pertinent geochemical, rock magnetic, and deep-tow data relevant to the hypothesis of magnetic telechemistry.' H-zones are found in two tectonic settings: (1) along 10 2 –10 3 km long sections of spreading axis close to hot spots; and (2) in narrow bands extending a few hundred kilometres along the edges of some fracture zones. Amplitudes in both provinces are 1.5 to 5, typically 2 to 3 times normal, and the hot spot H-zones are known from spreading half-rates of 0.6 to 3.7 cm yr −1 The highest amplitudes, magnetizations, and FeTi enrichment (up to 15–18% FeO T and 2–3% TiO 2 ) seem to occur where both provinces overlap, i.e., where fracture zones occur near hot spots, for example along the Blanco Fracture Zone south of the Juan de Fuca hot spot and along the Inca Fracture Zone east of the Galapagos hot spot. The FeTi enrichment appears to reflect shallow-depth crystal fractionation (plagioclase, augite, and olivine), which is more extensive near hot spots, and more generally for fast-spreading ridges. H-zones presently affect at least 2.6 × 10 3 km, or 6.5% of the Mid-Ocean Ridge axis. However, the total known H-area of 8.5 × 10 5 km 2 represents only 0.3% of oceanic crust. This suggests that older H-zones remain to be discovered, or/and that conditions favoring the formation of FeTi basalt and H-anomalies are more prevalent now than they have been on the average for the last 10 8 years. Evidence for the latter is provided by the known expansion of the magnetically well surveyed Juan de Fuca, Galapagos, and Yermak (Arctic) H-zones in the last 5 million years. |
format |
Article in Journal/Newspaper |
author |
Vogt, P. R. |
author_facet |
Vogt, P. R. |
author_sort |
Vogt, P. R. |
title |
Amplitudes of oceanic magnetic anomalies and the chemistry of oceanic crust: Synthesis and review of 'magnetic telechemistry' |
title_short |
Amplitudes of oceanic magnetic anomalies and the chemistry of oceanic crust: Synthesis and review of 'magnetic telechemistry' |
title_full |
Amplitudes of oceanic magnetic anomalies and the chemistry of oceanic crust: Synthesis and review of 'magnetic telechemistry' |
title_fullStr |
Amplitudes of oceanic magnetic anomalies and the chemistry of oceanic crust: Synthesis and review of 'magnetic telechemistry' |
title_full_unstemmed |
Amplitudes of oceanic magnetic anomalies and the chemistry of oceanic crust: Synthesis and review of 'magnetic telechemistry' |
title_sort |
amplitudes of oceanic magnetic anomalies and the chemistry of oceanic crust: synthesis and review of 'magnetic telechemistry' |
publisher |
Canadian Science Publishing |
publishDate |
1979 |
url |
http://dx.doi.org/10.1139/e79-210 http://www.nrcresearchpress.com/doi/pdf/10.1139/e79-210 |
long_lat |
ENVELOPE(-55.233,-55.233,-61.250,-61.250) ENVELOPE(-59.194,-59.194,-62.308,-62.308) |
geographic |
Arctic Galapagos Blanco Inca |
geographic_facet |
Arctic Galapagos Blanco Inca |
genre |
Arctic |
genre_facet |
Arctic |
op_source |
Canadian Journal of Earth Sciences volume 16, issue 12, page 2236-2262 ISSN 0008-4077 1480-3313 |
op_rights |
http://www.nrcresearchpress.com/page/about/CorporateTextAndDataMining |
op_doi |
https://doi.org/10.1139/e79-210 |
container_title |
Canadian Journal of Earth Sciences |
container_volume |
16 |
container_issue |
12 |
container_start_page |
2236 |
op_container_end_page |
2262 |
_version_ |
1785578472487256064 |