“…The influence of Earth orbital forcing on the long-term evolution of Indian monsoon has been recorded in deep-sea cores, lake sediments and stalagmites (Ziegler et al, 2010a;Cai et al, 2010;An et al, 2011). Previous researches demonstrated that the climate evolution of Indian monsoon is dominated by precession (~23 ka), obliquity (~41 ka) and eccentricity (~100 ka) cycles (e.g., Clemens et al, 1996;Clemens and Prell, 2003;Kelly et al, 2005;Kunkelova et al, 2018;Lindhorst et al, 2019;Lu et al, 2020). Previous orbital-scale studies of the ISM mainly used proxies of phytoplankton (G. bulloides) from the northern Arabian Sea (Prell et al, 1984;Prell and Van Campo, 1986;, grain size (Clemens and Prell, 1990;Krissek and Clemens, 1992), Ti/Al and excess Ba MAR (Shimmield et al, 1990), biogenic opal and organic carbon MAR (Murray and Prell, 1991).…”