Late Cretaceous climate and vegetation interactions: Cold continental interior paradox

The Campanian age of the Late Cretaceous was warm, with no evidence for permanent or seasonal sea ice at high latitudes. Sea level was high, creating extensive epicontinental and shallow shelf seas. Very low meridional thermal gradients existed in the oceans and on land. Campanian (80 Ma) climate an...

Full description

Bibliographic Details
Main Authors: DeConto, R. M., Hay, William W., Thompson, S. L., Bergengren, J.
Other Authors: Barrera, Enriqueta, Johnson, Claudia C.
Format: Book Part
Language:English
Published: The Geological Society of America 1999
Subjects:
Online Access:https://oceanrep.geomar.de/id/eprint/34732/
https://oceanrep.geomar.de/id/eprint/34732/1/scan_2016-12-05_13-42-05r.1.pdf
https://doi.org/10.1130/0-8137-2332-9.391
id ftoceanrep:oai:oceanrep.geomar.de:34732
record_format openpolar
spelling ftoceanrep:oai:oceanrep.geomar.de:34732 2023-05-15T18:18:08+02:00 Late Cretaceous climate and vegetation interactions: Cold continental interior paradox DeConto, R. M. Hay, William W. Thompson, S. L. Bergengren, J. Barrera, Enriqueta Johnson, Claudia C. 1999 text https://oceanrep.geomar.de/id/eprint/34732/ https://oceanrep.geomar.de/id/eprint/34732/1/scan_2016-12-05_13-42-05r.1.pdf https://doi.org/10.1130/0-8137-2332-9.391 en eng The Geological Society of America https://oceanrep.geomar.de/id/eprint/34732/1/scan_2016-12-05_13-42-05r.1.pdf DeConto, R. M., Hay, W. W., Thompson, S. L. and Bergengren, J. (1999) Late Cretaceous climate and vegetation interactions: Cold continental interior paradox. In: Evolution of the Cretaceous Ocean-Climate System. , ed. by Barrera, E. and Johnson, C. C. Geological Society of America Special Paper, 332 . The Geological Society of America, Boulder, Colo., pp. 391-406. ISBN 0-521-64142-X DOI 10.1130/0-8137-2332-9.391 <https://doi.org/10.1130/0-8137-2332-9.391>. doi:10.1130/0-8137-2332-9.391 info:eu-repo/semantics/restrictedAccess Book chapter NonPeerReviewed 1999 ftoceanrep https://doi.org/10.1130/0-8137-2332-9.391 2023-04-07T15:29:06Z The Campanian age of the Late Cretaceous was warm, with no evidence for permanent or seasonal sea ice at high latitudes. Sea level was high, creating extensive epicontinental and shallow shelf seas. Very low meridional thermal gradients existed in the oceans and on land. Campanian (80 Ma) climate and vegetation have been simulated using GENESIS (Global ENvironmental and Ecological Simulation of Interactive Systems) Version 2.0 and EVE (Equilibrium Vegetation Ecology model), developed by the Climate Change Research section of the Climate and Global Dynamics division at NCAR (National Center for Atmospheric Research). GENESIS is a comprehensive Earth system model, requiring high resolution (2^circ by 2^circ) solid earth boundary condition data as input for paleoclimate simulations. Boundary condition data define certain prescribed global fields such as the distribution of land-sea-ice, topography, orographic roughness, and soil texture, as well as atmospheric chemistry, the solar constant, and orbital parameters that define the latitudinal distribution of solar insolation. A comprehensive, high resolution paleogeography has been reconstructed for the Campanian. The paleogeography, based on a new global plate tectonic model, provides the framework for the solid earth boundary conditions used in the paleoclimate simulation. Because terrestrial ecosystems influence global climate by affecting the exchange of energy, water and momentum between the land surface and the atmosphere, the distribution of global vegetation should be included in pre-Quaternary paleoclimate simulations. However, reconstructing global vegetation distributions from the fossil record is difficult. EVE predicts the equilibrium state of plant community structure as a function of climate and fundamental ecological principles. The model has been modified to reproduce a vegetation distribution based on life forms that existed in the Late Cretaceous. EVE has been applied as a fully interactive component of the Campanian simulation. 1500 ppm CO_2 and a ... Book Part Sea ice OceanRep (GEOMAR Helmholtz Centre für Ocean Research Kiel)
institution Open Polar
collection OceanRep (GEOMAR Helmholtz Centre für Ocean Research Kiel)
op_collection_id ftoceanrep
language English
description The Campanian age of the Late Cretaceous was warm, with no evidence for permanent or seasonal sea ice at high latitudes. Sea level was high, creating extensive epicontinental and shallow shelf seas. Very low meridional thermal gradients existed in the oceans and on land. Campanian (80 Ma) climate and vegetation have been simulated using GENESIS (Global ENvironmental and Ecological Simulation of Interactive Systems) Version 2.0 and EVE (Equilibrium Vegetation Ecology model), developed by the Climate Change Research section of the Climate and Global Dynamics division at NCAR (National Center for Atmospheric Research). GENESIS is a comprehensive Earth system model, requiring high resolution (2^circ by 2^circ) solid earth boundary condition data as input for paleoclimate simulations. Boundary condition data define certain prescribed global fields such as the distribution of land-sea-ice, topography, orographic roughness, and soil texture, as well as atmospheric chemistry, the solar constant, and orbital parameters that define the latitudinal distribution of solar insolation. A comprehensive, high resolution paleogeography has been reconstructed for the Campanian. The paleogeography, based on a new global plate tectonic model, provides the framework for the solid earth boundary conditions used in the paleoclimate simulation. Because terrestrial ecosystems influence global climate by affecting the exchange of energy, water and momentum between the land surface and the atmosphere, the distribution of global vegetation should be included in pre-Quaternary paleoclimate simulations. However, reconstructing global vegetation distributions from the fossil record is difficult. EVE predicts the equilibrium state of plant community structure as a function of climate and fundamental ecological principles. The model has been modified to reproduce a vegetation distribution based on life forms that existed in the Late Cretaceous. EVE has been applied as a fully interactive component of the Campanian simulation. 1500 ppm CO_2 and a ...
author2 Barrera, Enriqueta
Johnson, Claudia C.
format Book Part
author DeConto, R. M.
Hay, William W.
Thompson, S. L.
Bergengren, J.
spellingShingle DeConto, R. M.
Hay, William W.
Thompson, S. L.
Bergengren, J.
Late Cretaceous climate and vegetation interactions: Cold continental interior paradox
author_facet DeConto, R. M.
Hay, William W.
Thompson, S. L.
Bergengren, J.
author_sort DeConto, R. M.
title Late Cretaceous climate and vegetation interactions: Cold continental interior paradox
title_short Late Cretaceous climate and vegetation interactions: Cold continental interior paradox
title_full Late Cretaceous climate and vegetation interactions: Cold continental interior paradox
title_fullStr Late Cretaceous climate and vegetation interactions: Cold continental interior paradox
title_full_unstemmed Late Cretaceous climate and vegetation interactions: Cold continental interior paradox
title_sort late cretaceous climate and vegetation interactions: cold continental interior paradox
publisher The Geological Society of America
publishDate 1999
url https://oceanrep.geomar.de/id/eprint/34732/
https://oceanrep.geomar.de/id/eprint/34732/1/scan_2016-12-05_13-42-05r.1.pdf
https://doi.org/10.1130/0-8137-2332-9.391
genre Sea ice
genre_facet Sea ice
op_relation https://oceanrep.geomar.de/id/eprint/34732/1/scan_2016-12-05_13-42-05r.1.pdf
DeConto, R. M., Hay, W. W., Thompson, S. L. and Bergengren, J. (1999) Late Cretaceous climate and vegetation interactions: Cold continental interior paradox. In: Evolution of the Cretaceous Ocean-Climate System. , ed. by Barrera, E. and Johnson, C. C. Geological Society of America Special Paper, 332 . The Geological Society of America, Boulder, Colo., pp. 391-406. ISBN 0-521-64142-X DOI 10.1130/0-8137-2332-9.391 <https://doi.org/10.1130/0-8137-2332-9.391>.
doi:10.1130/0-8137-2332-9.391
op_rights info:eu-repo/semantics/restrictedAccess
op_doi https://doi.org/10.1130/0-8137-2332-9.391
_version_ 1766194565096669184