High-resolution sediment archives from small alpine lakes in the Alaskan Arctic and tropical Andes were used to investigate Holocene climate change in these climatically sensitive and important regions. Varved minerogenic sediments from glacial-fed Blue Lake, Brooks Range Alaska (1275 m asl), were used to derive a proxy temperature record between AD 730-2005. Cool temperatures characterize the late Holocene (last millennial average, or LMA = 4.2 °C) with 20th century warming anomalous within the context of the last 1275 years (0.8°C above LMA). However, temperatures between AD 1350-1450 and AD 1500-1620 approached modern values (0.4 and 0.3°C above LMA, respectively). Prolonged cooling at Blue Lake occurred from AD 1620-1880, during the Little Ice Age (LIA). LIA cooling and 20th century warming correspond to radiative minima and maxima, respectively. However, the relationship between radiative forcing and temperature is not consistent through the record, suggesting that other factors contributed to temperature variability in this region. In the tropics, South American summer monsoon (SASM) variability during the last 2300 years was reconstructed from oxygen isotope ratios of authigenic carbonate (δ18Ocal) preserved in varved sediments from Laguna Pumacocha (4300 m asl), Peru. High δ18Ocal values and reduced variability during the Medieval Climate Anomaly (MCA; AD 920-1050) suggest that the SASM and El Niño-Southern Oscillation (ENSO) were weak due to reduced easterly tropospheric flow and cooling within the eastern tropical Pacific (ETP). Low δ18Ocal from during the LIA (AD 1415-1820) and enhanced variability from AD 1415-1770 suggest that the SASM and ENSO were strong as a result of enhanced easterly tropospheric flow and warm, but variable, sea surface temperatures in the ETP, respectively. These ocean-atmosphere responses reflect the tropical Pacifics response to radiative forcing described by the ocean dynamical thermostat model (Clement et al. 1996). Long-term δ18Ocal trends at Pumacocha suggest that the SASM was weak during the early Holocene and then strengthened through the Holocene as Southern Hemisphere insolation increased. This confirms the importance of orbital controls on SASM dynamics. However, the Andean SASM strengthened to a greater extent than the SASM over the Amazon basin, indicating that these regions respond differently to similar forcing mechanisms.
| Identifer | oai:union.ndltd.org:PITT/oai:PITTETD:etd-07152009-163200 |
| Date | 30 September 2009 |
| Creators | Bird, Broxton Williams |
| Contributors | Brian Stewart, Mark Abbott, Emily Elliott, Michael Rosenmeier, Mathias Vuille |
| Publisher | University of Pittsburgh |
| Source Sets | University of Pittsburgh |
| Language | English |
| Detected Language | English |
| Type | text |
| Format | application/pdf |
| Source | http://etd.library.pitt.edu/ETD/available/etd-07152009-163200/ |
| Rights | restricted, I hereby certify that, if appropriate, I have obtained and attached hereto a written permission statement from the owner(s) of each third party copyrighted matter to be included in my thesis, dissertation, or project report, allowing distribution as specified below. I certify that the version I submitted is the same as that approved by my advisory committee. I hereby grant to University of Pittsburgh or its agents the non-exclusive license to archive and make accessible, under the conditions specified below, my thesis, dissertation, or project report in whole or in part in all forms of media, now or hereafter known. I retain all other ownership rights to the copyright of the thesis, dissertation or project report. I also retain the right to use in future works (such as articles or books) all or part of this thesis, dissertation, or project report. |
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