Hostname: page-component-586b7cd67f-dsjbd Total loading time: 0 Render date: 2024-11-25T07:28:03.139Z Has data issue: false hasContentIssue false

Paleoenvironment in Dae-Am San High Moor in the Korean Peninsula

Published online by Cambridge University Press:  18 July 2016

T Yoshioka
Affiliation:
Institute for Hydrospheric-Atmospheric Sciences, Nagoya University, Nagoya 464-8601, Japan
J-Y Lee
Affiliation:
Institute for Hydrospheric-Atmospheric Sciences, Nagoya University, Nagoya 464-8601, Japan
H A Takahashi
Affiliation:
Department of Earth and Planetary Sciences, Graduate School of Science, Nagoya University, Nagoya 464-8602, Japan
S-J Kang
Affiliation:
Department of Science Education, Chungbuk National University, Chongju, Chungbuk-do, Korea
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We discuss paleoenvironmental changes at the Dae-Am San high moor, located near the Demilitarized Zone at 38°N. This area has been reported to be the only high moor in the Korean peninsula. The 14C age of the bottom sediment (75–80 cm in depth) at this site is about 1900 BP. Since the radiocarbon ages for the intervals at 50–55 cm and 75–80 cm were almost the same, we conclude that the deep layers (55–80 cm) in the high moor were all part of the original soil. Low organic C and N contents in the deeper layers support this inference. The 50–55-cm layer consists of sandy material with very low organic content, suggesting erosion from the surrounding area. The surface layer (0–5 cm) was measured as 190 BP, and the middle layer (30–35 cm) was 870 BP. The bulk sedimentation rate was estimated to be about 0.4 mm yr−1 for the 0–30-cm interval. The δ13C value of organic carbon in the sediments fluctuated with depth. The δ13C profile of the Dae-Am San high moor may be explained by climatic changes which occurred during the Little Ice Age and Medieval Warm Period.

Type
I. Our ‘Dry’ Environment: Above Sea Level
Copyright
Copyright © 2001 by the Arizona Board of Regents on behalf of the University of Arizona 

References

Benner, R, Fogel, ML, Sprague, EK, Hodson, RE. 1987. Depletion of 13C in lignin and its implications for stable carbon isotope studies. Nature 329:708–10.CrossRefGoogle Scholar
Environmental Agency, Korea. 1988. Report on the research of the natural ecosystem in Dae-Am mountain. 230 p. In Korean.Google Scholar
Keigwin, LD. 1996. The Little Ice Age and Medieval Warm Period in the Sargasso Sea. Science 274:1504–8.CrossRefGoogle ScholarPubMed
Kitagawa, H, Masuzawa, T, Nakamura, T, Matsumoto, E. 1993. A batch preparation method for graphite targets with low background for AMS 14C measurements. Radiocarbon 35(2):295300.CrossRefGoogle Scholar
Kitagawa, H, Matsumoto, E. 1995. Climatic implications of δ13C variations in a Japanese cedar Cryptomeria japonica during the last two millenia. Geophysical Research Letters 22:2155–58.CrossRefGoogle Scholar
Kreutz, KJ, Mayewski, PA, Meeker, LD, Twickler, MS, Whitlow, SI, Pittalwala, II. 1997. Bipolar changes in atmospheric circulation during the Little Ice Age. Science 277:1294–6.CrossRefGoogle Scholar
Minagawa, M, Winter, DA, Kaplan, IR. 1984. Comparison of Kjeldahl and combustion methods for measurement of nitrogen isotope ratios in organic matter. Analytical Chemistry 56:1859–61.Google Scholar
Minomo, K, Akagi, T, Yonemura, S, Yoh, M, Turuta, H, Nakamura, T. 1997. δ13C vertical change of peat in the Ozegahara wetland. Summaries of Researches Using AMS at Nagoya University (III). Dating and Materials Research Center, Nagoya University. p 146–51. In Japanese with English abstract.Google Scholar
White, JWC, Ciais, P, Figge, RA, Kenny, R, Markgraf, V. 1994. A high-resolution record of atmospheric CO2 content from carbon isotopes in peat. Nature 367:153–6.CrossRefGoogle Scholar
Williams, DF, Peck, J, Karabanov, EB, Prokopenko, AA, Kravchinsky, V, King, J, Kuzmin, MI. 1997. Lake Baikal record of continental climate response to orbital insolation during the past 5 million yrs. Science 278:1114–7.CrossRefGoogle Scholar