We assigned preliminary
ages to our samples from paleomagnetic identification of the Brunhes/Matuyama
Chron (81.21 mcd; Heider et al., Chap. 28, this volume) and assuming a constant
sedimentation rate of ~10 cm/k.y. The complete 18O
record from Site 1020 is not yet available as this is written. Data are
available for isotope Stages 1.0-3.3, 5.1-6.4, 7.1-8.4, and 8.5-10.2 (A. Mix,
pers. comm., 1998). Our spliced record (Fig.
3) bears a striking resemblance to ice-volume changes as inferred from
SPECMAP
18O
and other Brunhes Chron
18O
records. We have matched our
SST estimates to the SPECMAP composite (Imbrie et al., 1984), Site 677 (Shackleton
et al., 1990), and to the preliminary benthic
18O
record from Site 1020 (A. Mix, pers. comm., 1998). The most striking feature is
the co-occurrence of maximum
SST and interglacial
18O.
This correlation is documented directly at Site 1020 for benthic
18O
Stages 5.1-5.5 and 7.1-8.4 (A. Mix, pers. comm., 1998). Based on this
relationship between warmest
SST and lightest benthic
18O,
we tied our warmest
SSTs from Site 1020 with Site 677 interglacial
18O
(Shackleton et al., 1990) at Stages 5.5, 7.0, 9.0, 11.1, 15.1, 15.3, 17.0, and
19.0. We linearly interpolated ages using the Site 677 time scale (Shackleton et
al., 1990) between oxygen isotope Stages (OIS) 5.5, 7.0, 11.1, 15.1, 15.3, and
17.0 at Site 677 and the Brunhes/Matuyama boundary at Site 1020 (Fig.
5). We remind the reader that Site 677
18O
is used only because its length is similar to our alkenone record. Our
references to "leads" or "lags" are speculative, but we are
confident that we will observe similar phase relationships with the complete
Site 1020
18O
record when it becomes available.