FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2015120417> ?p ?o ?g. }

• W2015120417 endingPage "614" @default.
• W2015120417 startingPage "598" @default.
• W2015120417 abstract "Thermal stresses are potentially important drivers of Io's tectonics and mountain building. It has been hypothesized that sustained local or regional shut down of heat-pipe volcanism on Io could lead to deep crustal heating and large compressive stresses [McKinnon, W.B., Schenk, P.M., Dombard, A.J., 2001. Geology 29, 103–106]. Such large stresses would then be relieved by thrust faulting and uplifting of crustal blocks, producing mountains like those observed on Io. Here we analyze the tectonic consequences of the heat-pipe model in detail, considering both the initial thermal stress state of a basalt or peridotite crust created by heat-pipe volcanism, and relative roles of subsidence stresses (due to burial of preexisting layers) and thermal stresses arising from variable volcanism and changes in crustal (∼lithosphere) thickness. We limit the magnitude of the potential subsidence stresses in our study, because the magnitude of subsidence stresses can be quite large, if not dominant. Results indicate that for a fixed crustal thickness, the region of failure and faulting moves closer to the surface as eruption rate decreases and time increases. When the crust melts at its base as volcanism decreases (as might occur under steady state tidal heating), resulting in crustal thinning, the region of failure is brought even closer to the surface. Naturally, when compressive, subsidence stresses are included, the vertical extent of crust in brittle failure thickens to include most of the lithosphere. In contrast, increases in eruption rate cause the extent of the region in compressional failure to decrease and be driven very deep in the crust (in the absence of sufficient subsidence stress). Therefore, regions of declining volcanism are more likely to produce mountains, whereas regions of extensive or increasing volcanism are less likely to do so. This is consistent with the observation of a global anticorrelation between mountains and volcanic centers on Io. Finally, we find that the choice of crustal composition/rheology (dry basalt vs. dry peridotite) has little effect on our results implying that basalt, peridotite and komatiite are all similarly “stiff” in the Io environment." @default.
• W2015120417 created "2016-06-24" @default.
• W2015120417 creator A5085917274 @default.
• W2015120417 creator A5090022166 @default.
• W2015120417 date "2009-06-01" @default.
• W2015120417 modified "2023-10-16" @default.
• W2015120417 title "Formation of mountains on Io: Variable volcanism and thermal stresses" @default.
• W2015120417 cites W1965578459 @default.
• W2015120417 cites W1972955272 @default.
• W2015120417 cites W1975288940 @default.
• W2015120417 cites W1977156689 @default.
• W2015120417 cites W1980859843 @default.
• W2015120417 cites W1985236692 @default.
• W2015120417 cites W1986413464 @default.
• W2015120417 cites W1987092092 @default.
• W2015120417 cites W1991791979 @default.
• W2015120417 cites W1991827373 @default.
• W2015120417 cites W1994635685 @default.
• W2015120417 cites W1999290715 @default.
• W2015120417 cites W1999750279 @default.
• W2015120417 cites W2001163525 @default.
• W2015120417 cites W2001375321 @default.
• W2015120417 cites W2009610178 @default.
• W2015120417 cites W2011767508 @default.
• W2015120417 cites W2016297755 @default.
• W2015120417 cites W2021319608 @default.
• W2015120417 cites W2023812212 @default.
• W2015120417 cites W2030250571 @default.
• W2015120417 cites W2033136430 @default.
• W2015120417 cites W2033916216 @default.
• W2015120417 cites W2034355816 @default.
• W2015120417 cites W2041554536 @default.
• W2015120417 cites W2044166855 @default.
• W2015120417 cites W2046857064 @default.
• W2015120417 cites W2046984304 @default.
• W2015120417 cites W2049676529 @default.
• W2015120417 cites W2052916940 @default.
• W2015120417 cites W2053747921 @default.
• W2015120417 cites W2054804874 @default.
• W2015120417 cites W2062677185 @default.
• W2015120417 cites W2069863674 @default.
• W2015120417 cites W2073222324 @default.
• W2015120417 cites W2074338804 @default.
• W2015120417 cites W2075881015 @default.
• W2015120417 cites W2076369329 @default.
• W2015120417 cites W2081012183 @default.
• W2015120417 cites W2082275824 @default.
• W2015120417 cites W2091635199 @default.
• W2015120417 cites W2092342290 @default.
• W2015120417 cites W2095466448 @default.
• W2015120417 cites W2099949247 @default.
• W2015120417 cites W2119026758 @default.
• W2015120417 cites W2122061674 @default.
• W2015120417 cites W2122990823 @default.
• W2015120417 cites W2129641844 @default.
• W2015120417 cites W2145761095 @default.
• W2015120417 cites W2147453360 @default.
• W2015120417 cites W2152741759 @default.
• W2015120417 cites W4211123977 @default.
• W2015120417 doi "https://doi.org/10.1016/j.icarus.2009.02.006" @default.
• W2015120417 hasPublicationYear "2009" @default.
• W2015120417 type Work @default.
• W2015120417 sameAs 2015120417 @default.
• W2015120417 citedByCount "29" @default.
• W2015120417 countsByYear W20151204172012 @default.
• W2015120417 countsByYear W20151204172013 @default.
• W2015120417 countsByYear W20151204172014 @default.
• W2015120417 countsByYear W20151204172015 @default.
• W2015120417 countsByYear W20151204172016 @default.
• W2015120417 countsByYear W20151204172017 @default.
• W2015120417 countsByYear W20151204172018 @default.
• W2015120417 countsByYear W20151204172019 @default.
• W2015120417 countsByYear W20151204172020 @default.
• W2015120417 countsByYear W20151204172021 @default.
• W2015120417 countsByYear W20151204172022 @default.
• W2015120417 crossrefType "journal-article" @default.
• W2015120417 hasAuthorship W2015120417A5085917274 @default.
• W2015120417 hasAuthorship W2015120417A5090022166 @default.
• W2015120417 hasConcept C109007969 @default.
• W2015120417 hasConcept C114793014 @default.
• W2015120417 hasConcept C119477230 @default.
• W2015120417 hasConcept C127313418 @default.
• W2015120417 hasConcept C161509811 @default.
• W2015120417 hasConcept C165205528 @default.
• W2015120417 hasConcept C16942324 @default.
• W2015120417 hasConcept C180851071 @default.
• W2015120417 hasConcept C2776698055 @default.
• W2015120417 hasConcept C5900021 @default.
• W2015120417 hasConcept C6363049 @default.
• W2015120417 hasConcept C77928131 @default.
• W2015120417 hasConcept C8058405 @default.
• W2015120417 hasConceptScore W2015120417C109007969 @default.
• W2015120417 hasConceptScore W2015120417C114793014 @default.
• W2015120417 hasConceptScore W2015120417C119477230 @default.
• W2015120417 hasConceptScore W2015120417C127313418 @default.
• W2015120417 hasConceptScore W2015120417C161509811 @default.
• W2015120417 hasConceptScore W2015120417C165205528 @default.
• W2015120417 hasConceptScore W2015120417C16942324 @default.

• next