1989
DOI: 10.1016/0264-3707(89)90009-4
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Heat flow and the Eurasian-African plate boundary in the eastern part of the Azores-Gibraltar fracture zone

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Cited by 13 publications
(10 citation statements)
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“…The Bouguer gravity anomaly also shows a maximum of ∼380 mGal on the Gorringe Bank, and the maximum variation relative to the abyssal plains is ∼120 mGal. We have compiled surface heat flow measurements in the area from different authors (colored circles in Figure 4b) [ Verzhbitsky and Zolotarev , 1989; Polyak et al , 1996; Fernàndez et al , 1998; Rimi et al , 1998; Grevemeyer et al , 2009]. Around the Gorringe Bank there are a few measurements, which vary between 40 and 65 mW/m 2 .…”
Section: Present‐day Lithospheric Structurementioning
confidence: 99%
“…The Bouguer gravity anomaly also shows a maximum of ∼380 mGal on the Gorringe Bank, and the maximum variation relative to the abyssal plains is ∼120 mGal. We have compiled surface heat flow measurements in the area from different authors (colored circles in Figure 4b) [ Verzhbitsky and Zolotarev , 1989; Polyak et al , 1996; Fernàndez et al , 1998; Rimi et al , 1998; Grevemeyer et al , 2009]. Around the Gorringe Bank there are a few measurements, which vary between 40 and 65 mW/m 2 .…”
Section: Present‐day Lithospheric Structurementioning
confidence: 99%
“…Source: TOPEX [ Smith and Sandwell , 1997]. Azores‐Gibraltar Fracture Zone after Verhbitsky and Zolotarev [1989]. Proposed Madeira hotspot track shown as thin dotted line (oldest available radiometric ages for each volcano are given in Ma; see text for details).…”
Section: Introductionmentioning
confidence: 99%
“…Some correlation between the heat flow in the four cells and the timing of magmatism exists, as well. In western Alps (with the oldest lamproites), the average heat flow is 50-70 mW/m 2 (Della Vedova et al 1991), in the cells with intermediate age lamproites (Betics and Cornacya) the heat flow varies between 70 and 120 mW/m 2 (Verzhbitsky and Zolotarev 1989;Fernandez et al 1998;Della Vedova et al 1991), and in the Tuscany cell with the younger lamproites the heat flow is between 80 and 200 mW/m 2 , with local values above 400 mW/m 2 (Della Vedova et al 1991). Therefore, the sequence of structures reported in Fig.…”
Section: Discussionmentioning
confidence: 98%