2010
DOI: 10.1093/petrology/egp088
|View full text |Cite
|
Sign up to set email alerts
|

Mantle Melting, Melt Transport, and Delivery Beneath a Slow-Spreading Ridge: The Paleo-MAR from 23 15'N to 23 45'N

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1
1
1

Citation Types

5
84
0
1

Year Published

2011
2011
2017
2017

Publication Types

Select...
7
1
1

Relationship

0
9

Authors

Journals

citations
Cited by 136 publications
(90 citation statements)
references
References 100 publications
5
84
0
1
Order By: Relevance
“…Nickel contents of olivines of site A and B generally range from 0.38 to 0.46 wt.% NiO, and extend to lower values (reaching 0.26 wt.%) in compositelherzolites of site A, with a maximum NiO content (0.54 wt.%) in a lherzolite spatially associated with hornblendite at site B (04LH04). This range of Mg# and Ni contents is similar to those reported for in olivine-websterites and peridotites of abyssal peridotites, forearc peridotites, ophiolite sequences, and cratonic xenoliths (e.g., Kelemen et al, 1998;O'Hara and Ishii, 1998;Suhr et al, 2003;Dick et al, 2010;Warren and Shimizu, 2010).…”
Section: Olivine and Spinel Compositionssupporting
confidence: 85%
“…Nickel contents of olivines of site A and B generally range from 0.38 to 0.46 wt.% NiO, and extend to lower values (reaching 0.26 wt.%) in compositelherzolites of site A, with a maximum NiO content (0.54 wt.%) in a lherzolite spatially associated with hornblendite at site B (04LH04). This range of Mg# and Ni contents is similar to those reported for in olivine-websterites and peridotites of abyssal peridotites, forearc peridotites, ophiolite sequences, and cratonic xenoliths (e.g., Kelemen et al, 1998;O'Hara and Ishii, 1998;Suhr et al, 2003;Dick et al, 2010;Warren and Shimizu, 2010).…”
Section: Olivine and Spinel Compositionssupporting
confidence: 85%
“…3), and we use it to calculate precision in our corrected measurements of Fe 3+ /ΣFe ratios of unknown spinel samples. Deviations of each session average (Supplementary 1 Table S2) from their respective multisession means (Table 4) (2016): (Prinz et al 1976;Hamlyn and Bonatti 1980;Dick and Bullen 1984;Michael and Bonatti 1985;Shibata and Thompson 1986;Dick 1989;Bryndzia and Wood 1990;Johnson et al 1990;Juteau et al 1990;Komor et al 1990;Bonatti et al 1992Bonatti et al , 1993Cannat et al 1992;Johnson and Dick 1992;Snow 1993;Constantin et al 1995;Arai and Matsukage 1996;Dick and Natland 1996;Ghose et al 1996;Jaroslow et al 1996;Niida 1997;Ross and Elthon 1997;Stephens 1997;Hellebrand et al 2002aHellebrand et al , 2002bBrunelli et al 2003;Hellebrand and Snow 2003;Seyler et al 2003Seyler et al , 2007Coogan et al 2004;Workman and Hart 2005;Morishita et al 2007;Cipriani et al 2009;Warren et al 2009;Brunelli and Seyler 2010;Dick et al 2010;Warren and Shimizu 2010;…”
Section: /σFementioning
confidence: 99%
“…We also discuss several models for the origin of depleted peridotites in the studied area because peridotites with depleted signatures in melt components were recently reported from oceanic core complexes where fertile peridotites are expected to be recovered (Seyler et al 2007;Tamura et al 2008;Dick et al 2010) (Fig. 14.9).…”
Section: The Primary Features Of Peridotites: Implications For the Fomentioning
confidence: 97%
“…Romanche fracture zone (FZ) are from Bonatti et al (1993), FifteenTwenty FZ are from Godard et al (2008), and Kane megamullion (oceanic core complex) are from Dick et al (2010). The Garret and Hess Deep of East Pacific Rise (EPR) are from Constantin (1999) and Dick and Natland (Dick and Natland 1996), respectively.…”
mentioning
confidence: 99%