FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3090751296> ?p ?o ?g. }

• W3090751296 endingPage "106606" @default.
• W3090751296 startingPage "106606" @default.
• W3090751296 abstract "Deposition of early Holocene Eastern Mediterranean S1 tephra and a Black Sea cryptotephra coincides with cultural transitions in the Fertile Crescent termed the Neolithic Revolution as well as sapropel formation during climate variability of the African humid period, classifying them as paramount regional marker horizons for archaeology as well as paleoclimatology. Their correlations with specific eruptions of the Mt. Erciyes stratovolcanic complex (Central Anatolia) remained inconclusive though. Here, we use zircon double-dating by (U–Th)/He and U–Th disequilibrium methods, major and trace element tephra glass geochemistry, and probabilistic modeling of tephra dispersal in an attempt to characterize all major late Quaternary proximal tephras of Mt. Erciyes, and to correlate them with distal deposits. Furthermore, we discuss contrasting proximal and distal tephra dispersal. Three nearly-coeval rhyolitic satellite domes (Dikkartın, Perikartın, and Karagüllü) erupted at Mt. Erciyes in the early Holocene, and their dome extrusions were all preceded by explosive phases producing pyroclastic material that formed tephra fall and pyroclastic flow deposits. The new eruption age of 9.03 ± 0.55 ka (1σ uncertainty here and elsewhere) for proximal Dikkartın pumice is consistent with 14C-based S1 tephra chronologies in distal locations averaging 8.92 ± 0.03 cal ka BP. Perikartın pyroclastic flow deposits predate S1 tephra by ca. 0.8 ka according to a pair of published 14C ages, and stratigraphically overlie Karagüllü fall-out, here dated to 8.2 ± 1.8 ka. Previously undated proximal tephras of Mt. Erciyes erupted in the Late (85.2 ± 4.9 ka) and Middle Pleistocene (154.5 ± 5.3 ka). S1 tephra glass is chemically similar to that of Dikkartın fall-out, but also indistinguishable from that of Perikartın fall-out. Karagüllü pumice is characterized by a distinct glass chemical composition, which correlates with that of unnamed cryptotephra reported for the southeastern Black Sea instead, where these results call for a re-evaluation of existing age models. Maximum lithic clast size isopleths for proximal Dikkartın fall-out indicate eastward dispersal of a 20 ± 5 km high eruption plume by stratospheric winds, in agreement with results of probabilistic tephra dispersal modeling. This azimuth contrasts with the known distribution of S1 tephra at distal locations that are all south of Mt. Erciyes. Significant tephra occurrences at up to 1300 km distance and orthogonal to prevalent stratospheric wind directions either result from very atypical wind conditions (probability ≪10 %), or are caused by tephra transport by prevailing low altitude winds. Two scenarios are proposed for low altitude transport: eolian reworking of primary fall-out (more likely from the more widespread Dikkartın deposits), or co-ignimbrite ash cloud dispersal (more likely from the Perikartın eruption which predominantly produced pyroclastic flows). Because S1 tephra is chemically indistinguishable from both Dikkartın and Perikartın by major and trace element glass compositions, its exact source and dispersal mechanism remain ambiguous, although existing 14C ages for Perikartın predating those for S1 tephra favor Dikkartın as its source." @default.
• W3090751296 created "2020-10-08" @default.
• W3090751296 creator A5010757634 @default.
• W3090751296 creator A5015202816 @default.
• W3090751296 creator A5026147972 @default.
• W3090751296 creator A5030394446 @default.
• W3090751296 creator A5035377215 @default.
• W3090751296 creator A5037491853 @default.
• W3090751296 creator A5043039632 @default.
• W3090751296 creator A5043716768 @default.
• W3090751296 creator A5078860738 @default.
• W3090751296 creator A5082011068 @default.
• W3090751296 creator A5082300127 @default.
• W3090751296 creator A5089230336 @default.
• W3090751296 date "2020-12-01" @default.
• W3090751296 modified "2023-10-16" @default.
• W3090751296 title "New insights into source and dispersal of Mediterranean S1 tephra, an early Holocene marker horizon erupted at Mt. Erciyes (Turkey)" @default.
• W3090751296 cites W1576391386 @default.
• W3090751296 cites W1772666815 @default.
• W3090751296 cites W1794463924 @default.
• W3090751296 cites W1832756902 @default.
• W3090751296 cites W1882796292 @default.
• W3090751296 cites W1963578784 @default.
• W3090751296 cites W1965580809 @default.
• W3090751296 cites W1978126824 @default.
• W3090751296 cites W1981100101 @default.
• W3090751296 cites W1984571476 @default.
• W3090751296 cites W1987734384 @default.
• W3090751296 cites W1987748614 @default.
• W3090751296 cites W1988620901 @default.
• W3090751296 cites W1991921692 @default.
• W3090751296 cites W1993749617 @default.
• W3090751296 cites W1995490465 @default.
• W3090751296 cites W2004824771 @default.
• W3090751296 cites W2006896663 @default.
• W3090751296 cites W2007492863 @default.
• W3090751296 cites W2011219267 @default.
• W3090751296 cites W2012295549 @default.
• W3090751296 cites W2014866349 @default.
• W3090751296 cites W2015779193 @default.
• W3090751296 cites W2017386389 @default.
• W3090751296 cites W2019192079 @default.
• W3090751296 cites W2027453465 @default.
• W3090751296 cites W2031267260 @default.
• W3090751296 cites W2033687291 @default.
• W3090751296 cites W2033989348 @default.
• W3090751296 cites W2040235128 @default.
• W3090751296 cites W2048802985 @default.
• W3090751296 cites W2049111217 @default.
• W3090751296 cites W2049425791 @default.
• W3090751296 cites W2052552450 @default.
• W3090751296 cites W2053711969 @default.
• W3090751296 cites W2067511405 @default.
• W3090751296 cites W2068397892 @default.
• W3090751296 cites W2076081783 @default.
• W3090751296 cites W2076529043 @default.
• W3090751296 cites W2076919476 @default.
• W3090751296 cites W2077530697 @default.
• W3090751296 cites W2078013548 @default.
• W3090751296 cites W2082755294 @default.
• W3090751296 cites W2083714209 @default.
• W3090751296 cites W2085064498 @default.
• W3090751296 cites W2086474520 @default.
• W3090751296 cites W2087274923 @default.
• W3090751296 cites W2091350276 @default.
• W3090751296 cites W2094665897 @default.
• W3090751296 cites W2117138976 @default.
• W3090751296 cites W2121745948 @default.
• W3090751296 cites W2122798313 @default.
• W3090751296 cites W2123008518 @default.
• W3090751296 cites W2131280929 @default.
• W3090751296 cites W2131308757 @default.
• W3090751296 cites W2137107847 @default.
• W3090751296 cites W2145180142 @default.
• W3090751296 cites W2163313249 @default.
• W3090751296 cites W2277674898 @default.
• W3090751296 cites W2407293154 @default.
• W3090751296 cites W2512570582 @default.
• W3090751296 cites W2514365797 @default.
• W3090751296 cites W2529945619 @default.
• W3090751296 cites W2538569938 @default.
• W3090751296 cites W2587639639 @default.
• W3090751296 cites W2731402290 @default.
• W3090751296 cites W2762632887 @default.
• W3090751296 cites W2810279480 @default.
• W3090751296 cites W2883351308 @default.
• W3090751296 cites W2895060011 @default.
• W3090751296 cites W2902589023 @default.
• W3090751296 cites W2913109044 @default.
• W3090751296 cites W2982555460 @default.
• W3090751296 cites W2993392114 @default.
• W3090751296 cites W2995376276 @default.
• W3090751296 cites W94878182 @default.
• W3090751296 doi "https://doi.org/10.1016/j.quascirev.2020.106606" @default.
• W3090751296 hasPublicationYear "2020" @default.
• W3090751296 type Work @default.
• W3090751296 sameAs 3090751296 @default.
• W3090751296 citedByCount "6" @default.

• next