دورية أكاديمية
Transient climate simulations of the Holocene (version 1) – experimental design and boundary conditions
| العنوان: | Transient climate simulations of the Holocene (version 1) – experimental design and boundary conditions |
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| المؤلفون: | Z. Tian, D. Jiang, R. Zhang, B. Su |
| المصدر: | Geoscientific Model Development, Vol 15, Pp 4469-4487 (2022) |
| بيانات النشر: | Copernicus Publications, 2022. |
| سنة النشر: | 2022 |
| المجموعة: | LCC:Geology |
| مصطلحات موضوعية: | Geology, QE1-996.5 |
| الوصف: | The Holocene, which started approximately 11.5 ka, is the latest interglacial period with several rapid climate changes with timescales, from decades to centuries, superimposed on the millennium-scale mean climate trend. Climate models provide useful tools to investigate the underlying dynamic mechanisms for the climate change during this well-studied time period. Thanks to the improvements in the climate model and computational power, transient simulation of the Holocene offers an opportunity to investigate the climate evolution in response to time-varying external forcings and feedbacks. Here, we present the design of a new set of transient experiments for the whole Holocene from 11.5 ka to the preindustrial period (1850; HT-11.5 ka) to investigate both the combined and separated effects of the main external forcing of orbital insolation, atmospheric greenhouse gas (GHG) concentrations, and ice sheets on the climate evolution over the Holocene. The HT-11.5 ka simulations are performed with a relatively high-resolution version of the comprehensive Earth system model CESM1.2.1 without acceleration, both fully and singly forced by time-varying boundary conditions of orbital configurations, atmospheric GHGs, and ice sheets. Preliminary simulation results show a slight decrease in the global annual mean surface air temperature from 11.5 to 7.5 ka due to both changes in orbital insolation and GHG concentrations, with an abrupt cooling at approximately 7.5 ka, which is followed by a continuous warming until the preindustrial period, mainly due to increased GHG concentrations. Both at global and zonal mean scales, the simulated annual and seasonal temperature changes at 6 ka lie within the range of the 14 PMIP4 model results and are overall stronger than their arithmetic mean results for the Middle Holocene simulations. Further analyses on the HT-11.5 ka transient simulation results will be covered by follow-up studies. |
| نوع الوثيقة: | article |
| وصف الملف: | electronic resource |
| اللغة: | English |
| تدمد: | 1991-959X 1991-9603 |
| Relation: | https://gmd.copernicus.org/articles/15/4469/2022/gmd-15-4469-2022.pdf; https://doaj.org/toc/1991-959X; https://doaj.org/toc/1991-9603 |
| DOI: | 10.5194/gmd-15-4469-2022 |
| URL الوصول: | https://doaj.org/article/17837897438542beb2f25407f507cc52 |
| رقم الأكسشن: | edsdoj.17837897438542beb2f25407f507cc52 |
| قاعدة البيانات: | Directory of Open Access Journals |
Full Text Finder | تدمد: | 1991959X 19919603 |
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| DOI: | 10.5194/gmd-15-4469-2022 |