02654nas a2200349 4500000000100000000000100001008004100002260000800043653006600051653005200117653004300169653004100212653001500253653001500268653001400283100001700297700001300314700001600327700001400343700001500357700001800372700001400390700001400404700001500418700001500433245010600448856004300554300001100597490000700608520167500615020001402290 2008 d bAGU10a1512 Geomagnetism and Paleomagnetism: Environmental magnetism10a1605 Global Change: Abrupt/rapid climate change10a1621 Global Change: Cryospheric change10a1641 Global Change: Sea level change10achronology10aQuaternary10asea level1 aE.J. Rohling1 aK. Grant1 aC. Hemleben1 aM. Kucera1 aA. Roberts1 aI. Schmeltzer1 aH. Schulz1 aM. Siccha1 aM. Siddall1 aG. Trommer00aNew constraints on the timing of sea level fluctuations during early to middle marine isotope stage 3 uhttp://dx.doi.org/10.1029/2008PA001617 aPA32190 v233 aTo settle debate on the timing of sea level fluctuations during marine isotope stage (MIS) 3, we present records of δ18Oruber (sea level proxy) and magnetic susceptibility from the same samples within the single sediment archive (i.e., \textquotedblleftcoregistered\textquotedblright) of central Red Sea core GeoTü-KL11. Core-scanning X-ray fluorescence and environmental magnetic data establish the suitability of magnetic susceptibility as a proxy for eolian dust content in Red Sea sediments. The eolian dust data record similar variability as Greenland δ18Oice during early to middle MIS 3, in agreement with previous observations that regional Arabian Sea climate fluctuated with a timing similar to that of Greenland climate variations. In contrast, the sea level record fluctuates with a timing similar to that of Antarctic-style climate variations. The coregistered nature of the two records in core KL11 unambiguously reveals a distinct offset in the phase relationship between sea level and eolian dust fluctuations. The results confirm that sea level rises, indicated by shifts in Red Sea δ18Oruber to lighter values, occurred during cold episodes in Greenland during early to middle MIS 3. This indicates that the amplitudes of the reconstructed MIS 3 sea level fluctuations would not be reduced by inclusion of regional climate fluctuations in the Red Sea sea level method. Our analysis comprehensively supports our earlier conclusions of large-amplitude sea level variations during MIS 3 with a timing that is strongly similar to Antarctic-style climate variations. a0883-8305