The interglacial climates of the past 1 million years are characterized by a transition, about 430 ka ago, between the older ones, which were relatively cool, and the more recent ones, which were relatively warm. This transition corresponds to the so-called mid-Brunhes Event (MBE;Jansen et al., 1986) or mid-Brunhes Transition (MBT; Yin, 2013). Marine Isotope Stage (MIS) 9, an interglacial roughly covers from 331 to 303 ka BP (Railsback et al., 2015), is relatively less investigated compared to other post-MBE interglacials. The orbital configuration during MIS-9 is characterized by an in-phase relationship between maximum obliquity and minimum precession (northern Hemisphere [NH] summer occurring at perihelion) leading to a high summer insolation in the NH (Yin & Berger, 2010; Figures 1a and 1b). The climatic background condition of MIS-9 has been considered as an analog of the present interglacial and the future climates (Ruddiman et al., 2016). The geological records from global ocean and Antarctica show that it is a relatively strong interglacial according to the benthic δ 18 O records (e.g., Lisiecki & Raymo, 2005; Figure 1c), and it is also one of the warmest interglacials in Antarctica over the last 800 ka (Figure 1d;Jouzel et al., 2007) with almost the highest greenhouse gasses (GHGs) concentrations of all interglacial periods (Figure 1e; e.g., Loulergue et al., 2008;Lüthi et al., 2008). Climate simulation results show that MIS-9 is the simulated warmest interglacial in global annual mean temperature among the last nine ones as a result of both its high CO 2 concentrations and its insolation configuration (Yin & Berger, 2012). However, the paleosol S3, corresponding to MIS-9, from the Chinese Loess Plateau (CLP), is not the strongest soil, and it is obviously weaker than the S4 (corresponding to MIS-11) and the S5-1 (corresponding to MIS-13) paleosol units (Figure 1f), suggesting relatively weaker East Asian summer monsoon (EASM) precipitation (e.g.,