NissirosV1, Istex, Corpus, bibRecord, 000154

Mediterranean island arcs and origin of high potash volcanoes

Identifieur interne : 000154 ( Istex/Corpus ); précédent : 000153; suivant : 000155

Mediterranean island arcs and origin of high potash volcanoes

Auteurs : Dragoslav Ninkovich ; James D. Hays

Source :

Earth and Planetary Science Letters [ 0012-821X ] ; 1972.

RBID : ISTEX:2A025C5FE6777D443AC94AC2C46402F47609326D

English descriptors

KwdEn :
- Active volcanoes, Aegean seas, Aleutian, Aleutian islands, Aleutians, Antiparos, Asthenosphere, Batu tara, Benioff, Benioff zone, Calabrian, Chemical analyses, Chile, Crust, Deep earthquakes, Dickinson, Earthquake, Earthquake foci, Eolian islands, Focal depth, Focal depths, Geol, Geophys, Hatherton, High potash, High potash volcanoes, Indonesian, Indonesian volcanoes, Intermediate depth earthquakes, Intermediate earthquakes, Lithosphere, Magma, Main chain, Mediterranean, Mediterranean arcs, Mediterranean suite, Neapolitan, Neapolitan area, Ninkovich, Phlegrean, Phlegrean fields, Potash, Potash content, Praktika acad, Relative motion, Rubidium, Seismic, Seismic zone, Silica, Silica value, Sio2, Sio2 content, Survey bull, Trace elements, Trench, Tyrrhenian, Underlain, Underthrusting, Value increases, Vesuvius, Volcanic, Volcanic arcs, Volcanic rocks, Volcano, Volcanoes underlain.
Teeft :
- Active volcanoes, Aegean seas, Aleutian, Aleutian islands, Aleutians, Antiparos, Asthenosphere, Batu tara, Benioff, Benioff zone, Calabrian, Chemical analyses, Chile, Crust, Deep earthquakes, Dickinson, Earthquake, Earthquake foci, Eolian islands, Focal depth, Focal depths, Geol, Geophys, Hatherton, High potash, High potash volcanoes, Indonesian, Indonesian volcanoes, Intermediate depth earthquakes, Intermediate earthquakes, Lithosphere, Magma, Main chain, Mediterranean, Mediterranean arcs, Mediterranean suite, Neapolitan, Neapolitan area, Ninkovich, Phlegrean, Phlegrean fields, Potash, Potash content, Praktika acad, Relative motion, Rubidium, Seismic, Seismic zone, Silica, Silica value, Sio2, Sio2 content, Survey bull, Trace elements, Trench, Tyrrhenian, Underlain, Underthrusting, Value increases, Vesuvius, Volcanic, Volcanic arcs, Volcanic rocks, Volcano, Volcanoes underlain.

Abstract

Abstract: Active volcanoes of the Mediterranean Sea are distributed along two arc structures: the Hellenic arc in the Aegean Sea and the Calabrian arc in the Tyrrhenian Sea. The active volcanoes in both arcs lie above earthquakes with focal depth greater than 100 km. The depth of these earthquakes increases generally northward reaching a maximum depth of about 200 km in the Aegean Sea and more than 300 km in the Tyrrhenian Sea.The K2O versus SiO2 value in volcanic rocks of the active volcanoes of the Hellenic and Calabrin arcs increases with increasing depth of underlying earthquakes which is similar to the pattern found in Pacific and Indonesian volcanic arcs. The high potash rocks of the Mediterranean suite are the culmination of this trend toward increasing potash as earthquake depth increases. The ratio of the trace element rubidium to silica also increases with increasing depth of earthquakes.Both the intermediate earthquakes and volcanic activity in the Mediterranean, as in Indo-Pacific volcanic arcs, are considered to have originated in dehydration of oceanic crust underthrusting the Aegean and Tyrrhenian Seas as a consequence of a counterclockwise rotation of Africa relative to Eurasia. The released water, we believe, works its way toward the surface in a hydrous melt scavenging potash and other alkali on the way. The ultimate ratio of K2O versus SiO2 and Rb versus SiO2 will be determined by the temperature of the hydrous melt and the distance traveled through the asthenosphere.

Url:

https://api.istex.fr/document/2A025C5FE6777D443AC94AC2C46402F47609326D/fulltext/pdf

DOI: 10.1016/0012-821X(72)90151-3

Links to Exploration step

ISTEX:2A025C5FE6777D443AC94AC2C46402F47609326D

Le document en format XML

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<ce:author><ce:given-name>James</ce:given-name>
<ce:surname>D. Hays</ce:surname>
</ce:author>
<ce:affiliation><ce:textfn>Lamont-Doherty Geological Observatory, Columbia University, Palisades, New York 10964, USA</ce:textfn>
</ce:affiliation>
</ce:author-group>
<ce:date-received day="17" month="7" year="1972"></ce:date-received>
<ce:abstract id="ab1" class="author" xml:lang="en"><ce:section-title>Abstract</ce:section-title>
<ce:abstract-sec><ce:simple-para>Active volcanoes of the Mediterranean Sea are distributed along two arc structures: the Hellenic arc in the Aegean Sea and the Calabrian arc in the Tyrrhenian Sea. The active volcanoes in both arcs lie above earthquakes with focal depth greater than 100 km. The depth of these earthquakes increases generally northward reaching a maximum depth of about 200 km in the Aegean Sea and more than 300 km in the Tyrrhenian Sea.</ce:simple-para>
<ce:simple-para>The K<ce:inf>2</ce:inf>
O versus SiO<ce:inf>2</ce:inf>
 value in volcanic rocks of the active volcanoes of the Hellenic and Calabrin arcs increases with increasing depth of underlying earthquakes which is similar to the pattern found in Pacific and Indonesian volcanic arcs. The high potash rocks of the Mediterranean suite are the culmination of this trend toward increasing potash as earthquake depth increases. The ratio of the trace element rubidium to silica also increases with increasing depth of earthquakes.</ce:simple-para>
<ce:simple-para>Both the intermediate earthquakes and volcanic activity in the Mediterranean, as in Indo-Pacific volcanic arcs, are considered to have originated in dehydration of oceanic crust underthrusting the Aegean and Tyrrhenian Seas as a consequence of a counterclockwise rotation of Africa relative to Eurasia. The released water, we believe, works its way toward the surface in a hydrous melt scavenging potash and other alkali on the way. The ultimate ratio of K<ce:inf>2</ce:inf>
O versus SiO<ce:inf>2</ce:inf>
 and Rb versus SiO<ce:inf>2</ce:inf>
 will be determined by the temperature of the hydrous melt and the distance traveled through the asthenosphere.</ce:simple-para>
</ce:abstract-sec>
</ce:abstract>
</head>
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<mods version="3.6"><titleInfo lang="en"><title>Mediterranean island arcs and origin of high potash volcanoes</title>
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<titleInfo type="alternative" lang="en" contentType="CDATA"><title>Mediterranean island arcs and origin of high potash volcanoes</title>
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<name type="personal"><namePart type="given">Dragoslav</namePart>
<namePart type="family">Ninkovich</namePart>
<affiliation>Lamont-Doherty Geological Observatory, Columbia University, Palisades, New York 10964, USA</affiliation>
<role><roleTerm type="text">author</roleTerm>
</role>
</name>
<name type="personal"><namePart type="given">James</namePart>
<namePart type="family">D. Hays</namePart>
<affiliation>Lamont-Doherty Geological Observatory, Columbia University, Palisades, New York 10964, USA</affiliation>
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<abstract lang="en">Abstract: Active volcanoes of the Mediterranean Sea are distributed along two arc structures: the Hellenic arc in the Aegean Sea and the Calabrian arc in the Tyrrhenian Sea. The active volcanoes in both arcs lie above earthquakes with focal depth greater than 100 km. The depth of these earthquakes increases generally northward reaching a maximum depth of about 200 km in the Aegean Sea and more than 300 km in the Tyrrhenian Sea.The K2O versus SiO2 value in volcanic rocks of the active volcanoes of the Hellenic and Calabrin arcs increases with increasing depth of underlying earthquakes which is similar to the pattern found in Pacific and Indonesian volcanic arcs. The high potash rocks of the Mediterranean suite are the culmination of this trend toward increasing potash as earthquake depth increases. The ratio of the trace element rubidium to silica also increases with increasing depth of earthquakes.Both the intermediate earthquakes and volcanic activity in the Mediterranean, as in Indo-Pacific volcanic arcs, are considered to have originated in dehydration of oceanic crust underthrusting the Aegean and Tyrrhenian Seas as a consequence of a counterclockwise rotation of Africa relative to Eurasia. The released water, we believe, works its way toward the surface in a hydrous melt scavenging potash and other alkali on the way. The ultimate ratio of K2O versus SiO2 and Rb versus SiO2 will be determined by the temperature of the hydrous melt and the distance traveled through the asthenosphere.</abstract>
<note>L.D.G.O. Contribution No. 1808.</note>
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Mediterranean island arcs and origin of high potash volcanoes

Mediterranean island arcs and origin of high potash volcanoes

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