Abstract

Abstract. Using the Community Climate System Model version 3 (CCSM3) including a dynamic global vegetation model, a set of 13 time slice experiments was carried out to study global climate variability between and within the Quaternary interglacials of Marine Isotope Stages (MISs) 1, 5, 11, 13, and 15. The selection of interglacial time slices was based on different aspects of inter- and intra-interglacial variability and associated astronomical forcing. The different effects of obliquity, precession, and greenhouse gas (GHG) forcing on global surface temperature and precipitation fields are illuminated. In most regions seasonal surface temperature anomalies can largely be explained by local insolation anomalies induced by the astronomical forcing. Climate feedbacks, however, may modify the surface temperature response in specific regions, most pronounced in the monsoon domains and the polar oceans. GHG forcing may also play an important role for seasonal temperature anomalies, especially at high latitudes and early Brunhes interglacials (MIS 13 and 15) when GHG concentrations were much lower than during the later interglacials. High- versus low-obliquity climates are generally characterized by strong warming over the Northern Hemisphere extratropics and slight cooling in the tropics during boreal summer. During boreal winter, a moderate cooling over large portions of the Northern Hemisphere continents and a strong warming at high southern latitudes is found. Beside the well-known role of precession, a significant role of obliquity in forcing the West African monsoon is identified. Other regional monsoon systems are less sensitive or not sensitive at all to obliquity variations during interglacials. Moreover, based on two specific time slices (394 and 615 ka), it is explicitly shown that the West African and Indian monsoon systems do not always vary in concert, challenging the concept of a global monsoon system on astronomical timescales. High obliquity can also explain relatively warm Northern Hemisphere high-latitude summer temperatures despite maximum precession around 495 ka (MIS 13). It is hypothesized that this obliquity-induced high-latitude warming may have prevented a glacial inception at that time.

Highlights

  • The Quaternary period is characterized by the cyclic growth and decay of continental ice sheets associated with global environmental changes

  • While it is commonly accepted that the transitions between glacial and interglacial stages are triggered by varying astronomical insolation forcings (Hays et al, 1976), climate research is just beginning to understand the internal climate feedbacks that are required to shift the Earth system from one state to the other

  • The selection of interglacial time slices was based on different aspects of inter- and intra-interglacial variability and associated astronomical forcing

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Summary

Introduction

The Quaternary period is characterized by the cyclic growth and decay of continental ice sheets associated with global environmental changes (see, e.g., Lisiecki and Raymo, 2005; Tzedakis et al, 2006; Jouzel et al, 2007; Lang and Wolff, 2011). 19 and 23 kyr (precession) as in Berger (1978), acts as an external driver for long-term climate change within the interglacials (i.e. the long-term intra-interglacial climate variability) and likely contributes to interglacial diversity since the evolution of astronomical parameters differs between all Quaternary interglacial stages (cf Tzedakis et al, 2009; Yin and Berger, 2015). Understanding both interglacial climate diversity and intra-interglacial variability helps to estimate the sensitivity of the Earth system to differ-. Rachmayani et al.: Intra-interglacial climate variability: model simulations of MIS 1, 5, 11, 13, and 15 ent forcings and to assess the rate and magnitude of current climate change relative to natural variability

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