Matches in SemOpenAlex for { <https://semopenalex.org/work/W1527760338> ?p ?o ?g. }
Showing items 1 to 83 of
83
with 100 items per page.
- W1527760338 endingPage "500" @default.
- W1527760338 startingPage "470" @default.
- W1527760338 abstract "The resistivity structure of the South African crust and upper mantle is being studied by deep and ultradeep electrical soundings (Schlumberger array). Deep electrical soundings are carried out by laying out cable for emission lines (maximum current electrode spacing AB of ∼40 km), while ultradeep soundings are made by using overhead telephone or power lines (maximum AB of ∼1000 km). Sounding results have been obtained on a variety of tectonic provinces that are given here with the age of the main metamorphic event shown in parentheses: the Rhodesian and Kaapvaal cratons (>2600 m.y.), the Limpopo Mobile Belt (>2700 m.y.), the Namaqua Mobile Belt (1000 m.y.), and the Damara Orogen (500 m.y.). The results show that the cratons are characterized by a highly resistive zone extending downward from the surface to a depth of 5–10 km depending on the locality. The average resistivity of this zone is about 100,000 ohm m with values varying between 30,000 and 400,000 ohm m. In contrast, the mobile belts invariably indicate the presence of a thick but only moderately resistive zone with a resistivity ranging from 2000 to 10,000 ohm m (average, 5000 ohm m) extending from the surface to a depth of 25–30 km. An important feature, deduced from the electrical results, is that this zone continues laterally into the cratons, where it underlies the highly resistive zone. Correlation of these electrical zones with geological information implies that first, the highly resistive zone in cratonic type terrain is associated with vast amounts of massive, strongly consolidated unfractured granitoid material in the form of granitic intrusions, gneisses, and migmatites, second, the moderate resistivities in mobile belts are due to the presence of intensely deformed, fractured, and highly metamorphosed rocks, and third, the lower crust under both cratons and mobile belts is metamorphic and fractured, consisting mainly of a refractory residuum which has been depleted of lighter granitic components. A surprising feature of the electrical sounding results is that a major portion of the upper crust (in mobile belts) and the entire lower crust to a depth of 25–30 km is only moderately resistive, and this provides strong evidence for the presence of free water in these zones. Calculations based on measurements of subsurface water resistivities and the electrical results have provided some crude constraints on the distribution of porosity in the crust. The highly resistive zone of the cratonic terrains has a porosity of less than 0.5%, but there is a severalfold increase in porosity at the transition to the moderately resistive zone which occurs at a depth ranging from 5–10 km. In the mobile belts the porosity varies from about 3% near the surface to 1% at a depth of 25 km. If water is present in the lower crust as is suggested by the electrical results, it may provide a means of explaining the origin of the conductive zone of variable conductance that has been recognized in the depth range 25–40 km. The preferred explanation at this stage is that the conductive zone forms by hydration, and it is shown that serpentinite (hydrated mantle rock) could account for its electrical properties. It is also tentatively suggested that water, by preferential movement, may determine the heat flow pattern observed in cratons and mobile belts. Finally, it is shown that the uppermost mantle is characterized by a thick, highly resistive zone which becomes more conductive as the depth and temperature increase. Its electrical resistivity suggests that it is dry." @default.
- W1527760338 created "2016-06-24" @default.
- W1527760338 creator A5017840345 @default.
- W1527760338 creator A5023866684 @default.
- W1527760338 date "2013-03-19" @default.
- W1527760338 modified "2023-09-26" @default.
- W1527760338 title "Electrical Studies of the Deep Crust in Various Tectonic Provinces of Southern Africa" @default.
- W1527760338 cites W1913990972 @default.
- W1527760338 cites W1965208709 @default.
- W1527760338 cites W1965699906 @default.
- W1527760338 cites W1967949701 @default.
- W1527760338 cites W1976011966 @default.
- W1527760338 cites W1987717268 @default.
- W1527760338 cites W2009617051 @default.
- W1527760338 cites W2018316497 @default.
- W1527760338 cites W2020769378 @default.
- W1527760338 cites W2025244783 @default.
- W1527760338 cites W2029942586 @default.
- W1527760338 cites W2035085561 @default.
- W1527760338 cites W2035931153 @default.
- W1527760338 cites W2072929359 @default.
- W1527760338 cites W2087586470 @default.
- W1527760338 cites W2096394838 @default.
- W1527760338 cites W2134319234 @default.
- W1527760338 cites W2134408726 @default.
- W1527760338 cites W2135094821 @default.
- W1527760338 cites W2142083960 @default.
- W1527760338 cites W2163401173 @default.
- W1527760338 cites W2168490532 @default.
- W1527760338 cites W2169878445 @default.
- W1527760338 cites W2270692314 @default.
- W1527760338 doi "https://doi.org/10.1029/gm020p0470" @default.
- W1527760338 hasPublicationYear "2013" @default.
- W1527760338 type Work @default.
- W1527760338 sameAs 1527760338 @default.
- W1527760338 citedByCount "30" @default.
- W1527760338 countsByYear W15277603382023 @default.
- W1527760338 crossrefType "book-chapter" @default.
- W1527760338 hasAuthorship W1527760338A5017840345 @default.
- W1527760338 hasAuthorship W1527760338A5023866684 @default.
- W1527760338 hasConcept C112313211 @default.
- W1527760338 hasConcept C119599485 @default.
- W1527760338 hasConcept C127313418 @default.
- W1527760338 hasConcept C127413603 @default.
- W1527760338 hasConcept C147717901 @default.
- W1527760338 hasConcept C165205528 @default.
- W1527760338 hasConcept C16942324 @default.
- W1527760338 hasConcept C2776698055 @default.
- W1527760338 hasConcept C67236022 @default.
- W1527760338 hasConcept C69990965 @default.
- W1527760338 hasConcept C77928131 @default.
- W1527760338 hasConcept C8058405 @default.
- W1527760338 hasConceptScore W1527760338C112313211 @default.
- W1527760338 hasConceptScore W1527760338C119599485 @default.
- W1527760338 hasConceptScore W1527760338C127313418 @default.
- W1527760338 hasConceptScore W1527760338C127413603 @default.
- W1527760338 hasConceptScore W1527760338C147717901 @default.
- W1527760338 hasConceptScore W1527760338C165205528 @default.
- W1527760338 hasConceptScore W1527760338C16942324 @default.
- W1527760338 hasConceptScore W1527760338C2776698055 @default.
- W1527760338 hasConceptScore W1527760338C67236022 @default.
- W1527760338 hasConceptScore W1527760338C69990965 @default.
- W1527760338 hasConceptScore W1527760338C77928131 @default.
- W1527760338 hasConceptScore W1527760338C8058405 @default.
- W1527760338 hasLocation W15277603381 @default.
- W1527760338 hasOpenAccess W1527760338 @default.
- W1527760338 hasPrimaryLocation W15277603381 @default.
- W1527760338 hasRelatedWork W1550144040 @default.
- W1527760338 hasRelatedWork W2163588067 @default.
- W1527760338 hasRelatedWork W2336057781 @default.
- W1527760338 hasRelatedWork W2369297125 @default.
- W1527760338 hasRelatedWork W2582821614 @default.
- W1527760338 hasRelatedWork W2888355352 @default.
- W1527760338 hasRelatedWork W4283574305 @default.
- W1527760338 hasRelatedWork W4285298697 @default.
- W1527760338 hasRelatedWork W4384700560 @default.
- W1527760338 hasRelatedWork W949230443 @default.
- W1527760338 isParatext "false" @default.
- W1527760338 isRetracted "false" @default.
- W1527760338 magId "1527760338" @default.
- W1527760338 workType "book-chapter" @default.