Relative stability of soil carbon revealed by shifts in δ15N and C:N ratio

F Conen, M Zimmermann, J Leifeld, B Seth… - …, 2008 - bg.copernicus.org
F Conen, M Zimmermann, J Leifeld, B Seth, C Alewell
Biogeosciences, 2008bg.copernicus.org
Life on earth drives a continuous exchange of carbon between soils and the atmosphere.
Some forms of soil carbon, or organic matter, are more stable and have a longer residence
time in soil than others. Relative differences in stability have often been derived from shifts in
δ 13 C (which is bound to a vegetation change from C3 to C4 type) or through 14 C-dating
(which is bound to small sample numbers because of high measurement costs). Here, we
propose a new concept based on the increase in δ 15 N and the decrease in C: N ratio with …
Life on earth drives a continuous exchange of carbon between soils and the atmosphere. Some forms of soil carbon, or organic matter, are more stable and have a longer residence time in soil than others. Relative differences in stability have often been derived from shifts in δ13C (which is bound to a vegetation change from C3 to C4 type) or through 14C-dating (which is bound to small sample numbers because of high measurement costs). Here, we propose a new concept based on the increase in δ15N and the decrease in C:N ratio with increasing stability. We tested the concept on grasslands at different elevations in the Swiss Alps. Depending on elevation and soil depth, it predicted mineral-associated organic carbon to be 3 to 73 times more stable than particulate organic carbon. Analysis of 14C-ages generally endorsed these predictions.
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