Characterizing the Atmospheric Dynamics of HD 209458b-like Hot Jupiters Using AI-driven Image Recognition/Categorization

Autor: F. Sainsbury-Martinez, P. Tremblin, M. Mancip, S. Donfack, E. Honore, M. Bourenane

Publikováno v: The Astrophysical Journal, Vol 958, Iss 1, p 68 (2023)

In order to understand the results of recent observations of exoplanets, models have become increasingly complex. Unfortunately, this increases both the computational cost and output size of said models. We intend to explore if AI image recognition c

Externí odkaz: https://doaj.org/article/41112b0e53324a5f8a930fe71c71bc18

Impact of CO2 and climate on the Last Glacial Maximum vegetation: results from the ORCHIDEE/IPSL models

Autor: N. Viovy, N. de Noblet-Ducoudré, G. Krinner, M. Kageyama, M.-N. Woillez, M. Mancip

Publikováno v: Climate of the Past, Vol 7, Iss 2, Pp 557-577 (2011)

Vegetation reconstructions from pollen data for the Last Glacial Maximum (LGM), 21 ky ago, reveal lanscapes radically different from the modern ones, with, in particular, a massive regression of forested areas in both hemispheres. Two main factors ha

Externí odkaz: https://doaj.org/article/d4f3b6b21f6b4a40a483d756b47ae863

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Evaluation of a Global Vegetation Model using time series of satellite vegetation indices

Autor: Fabienne Maignan, M. Mancip, Frédéric Chevallier, C. Garrec, F. M. Bréon, Nicolas Viovy, J. Trules, P. Ciais

Publikováno v: Geoscientific Model Development
Geoscientific Model Development, 2011, 4 (4), pp.1103-1114. ⟨10.5194/gmd-4-1103-2011⟩
Geoscientific Model Development, Vol 4, Iss 4, Pp 1103-1114 (2011)
Geoscientific Model Development, European Geosciences Union, 2011, 4 (4), pp.1103-1114. ⟨10.5194/gmd-4-1103-2011⟩

Atmospheric CO2 drives most of the greenhouse effect increase. One major uncertainty on the future rate of increase of CO2 in the atmosphere is the impact of the anticipated climate change on the vegetation. Dynamic Global Vegetation Models (DGVM) ar

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c9ef4cffbd1b8bb9de7237b70402fc2c
https://hal.science/hal-02928990/document

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