Duration and dynamics of the best orbital analogue to the present interglacial

Autor: Giaccio B.[1], Regattieri E.[1, 2, Zanchetta G.[1, Nomade S.[4], Renne P.R.[5, Sprain C.J.[5, Drysdale R.N.[7, Tzedakis P.C.[9], Messina P.[1], Scardia G.[1, 10], Sposato A.[1], Bassinot F.[4]

Publikováno v: Geology
Geology, 2015, 43 (7), pp.603-606. ⟨10.1130/G36677.1⟩
Geology, Geological Society of America, 2015, 43 (7), pp.603-606. ⟨10.1130/G36677.1⟩
Geology, vol 43, iss 7
Geology (Boulder Colo.) 43 (2015): 603–606. doi:10.1130/G36677.1
info:cnr-pdr/source/autori:Giaccio B.[1], Regattieri E.[1,2,3], Zanchetta G.[1,2,3], Nomade S.[4], Renne P.R.[5,6], Sprain C.J.[5,6], Drysdale R.N.[7,8], Tzedakis P.C.[9], Messina P.[1], Scardia G.[1,10], Sposato A.[1], Bassinot F.[4]/titolo:Duration and dynamics of the best orbital analogue to the present interglacial/doi:10.1130%2FG36677.1/rivista:Geology (Boulder Colo.)/anno:2015/pagina_da:603/pagina_a:606/intervallo_pagine:603–606/volume:43

Past orbital analogues to the current interglacial, such as Marine Isotope Stage 19c (MIS 19c, ca. 800 ka), can provide reliable reference intervals for evaluating the timing and the duration of the Holocene and factors inherent in its climatic progr

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::02fc8c1f8aa8ef7e9dd21490f5637b40
https://doi.org/10.1130/g36677.1