Abstract
Radiocarbon signatures (Delta C-14) of carbon dioxide (CO2) provide a measure of the age of C being decomposed by microbes or respired by living plants. Over a 2-year period, we measured Delta C-14 of soil respiration and soil CO2 in boreal forest sites in Canada, which varied primarily in the amount of time since the last stand-replacing fire. Comparing bulk respiration Delta C-14 with Delta C-14 of CO2 evolved in incubations of heterotrophic (decomposing organic horizons) and autotrophic (root and moss) components allowed us to estimate the relative contributions of O horizon decomposition vs. plant sources. Although soil respiration fluxes did not vary greatly, differences in Delta C-14 of respired CO2 indicated marked variation in respiration sources in space and time. The C-14 signature of respired CO2 respired from O horizon decomposition depended on the age of C substrates. These varied with time since fire, but consistently had Delta C-14 greater (averaging similar to 120 parts per thousand) than autotrophic respiration. The Delta C-14 of autotrophically respired CO2 in young stands equaled those expected for recent photosynthetic products (70 parts per thousand in 2003, 64 parts per thousand in 2004). CO2 respired by black spruce roots in stands > 40 years old had Delta C-14 up to 30 parts per thousand higher than recent photosynthates, indicating a significant contribution of C stored at least several years in plants. Decomposition of O horizon organic matter made up 20% or less of soil respiration in the younger (< 40 years since fire) stands, increasing to similar to 50% in mature stands. This is a minimum for total heterotrophic contribution, since mineral soil CO2 had Delta C-14 close to or less than those we have assigned to autotrophic respiration. Decomposition of old organic matter in mineral soils clearly contributed to soil respiration in younger stands in 2003, a very dry year, when Delta C-14 of soil respiration in younger successional stands dropped below those of the atmospheric CO2.
