Pyrogenic carbon from tropical savanna burning: production and stable isotope composition

Saiz, G.; Wynn, J. G.; Wurster, C. M.; Goodrick, I.; Nelson, P. N.; Bird, M. I.

Abstract

Widespread burning of mixed tree grass ecosystems represents the major natural locus of pyrogenic carbon (PyC) production. PyC is a significant, pervasive and yet poorly understood "slow-cycling" form of carbon present in the atmosphere, hydrosphere, soils and sediments. We conducted 16 experimental burns on a rainfall transect through northern Australian savannas with C-4 grasses ranging from 35 to 99% of total biomass Residues from each fire were partitioned into PyC and further into recalcitrant (HyPyC) components, with each of these fluxes also partitioned into proximal components (> 125 mu m), likely to remain close to the site of burning, and distal components ( 125 mu m), likely to be transported from the site of burning. The median (range) PyC production across all burns was 16.0 (11.5)% of total carbon exposed (TCE), with HyPyC accounting for 2.5 (4.9) % of TCE. Both PyC and HyPyC were dominantly partitioned into the proximal flux. Production of HyPyC was strongly related to fire residence time, with shorter duration fires resulting in higher HyPyC yields. The carbon isotope (delta C-13) compositions of PyC and HyPyC were generally lower by 1-3 parts per thousand relative to the original biomass, with marked depletion up to 7 %0 for grasslands dominated by C4 biomass delta C-13 values of CO2 produced by combustion were computed by mass balance and ranged from similar to 0.4 to 1.3 parts per thousand . The depletion of 13C in PyC and HyPyC relative to the original biomass has significant implications for the interpretation of delta C-13 values of savanna soil organic carbon and of ancient PyC preserved in the geologic record, as well as for global C-13 isotopic disequilibria calculations.

Más información

Título según WOS: ID WOS:000352112900015 Not found in local WOS DB
Título de la Revista: BIOGEOSCIENCES
Volumen: 12
Número: 6
Editorial: Copernicus Gesellschaft mbH
Fecha de publicación: 2015
Página de inicio: 1849
Página final: 1863
DOI:

10.5194/bg-12-1849-2015

Notas: ISI