Abstract
Satellite measurements of fire radiative power (FRP) are increasingly used to estimate the contribution of biomass burning to local and global carbon budgets. Without an associated uncertainty, however, FRP-based biomass burning estimates cannot be confidently compared across space and time, or against estimates derived from alternative methodologies. This work addresses this issue and quantifies the precision of Moderate Resolution Imaging Spectroradiometer (MODIS) measurements of FRP by collecting duplicate, off-nadir, overlapping observations of the same fires. Differences in the per-pixel FRP measured near-simultaneously in consecutive MODIS scans are approximately normally distributed with a standard deviation (sigma) of 26.6%. Simulations demonstrate that this uncertainty decreases to less than similar to 5% (at 1 sigma) for aggregations larger than similar to 50 MODIS active fire pixels. Although FRP uncertainties limit the confidence in flux estimates on a per-pixel basis, the sensitivity of biomass burning estimates to FRP uncertainties can be mitigated by conducting inventories at coarser spatiotemporal resolutions.
Original language | English |
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Pages (from-to) | 1988-1994 |
Number of pages | 7 |
Journal | GEOPHYSICAL RESEARCH LETTERS |
Volume | 41 |
Issue number | 6 |
DOIs | |
Publication status | Published - 28 Mar 2014 |
Keywords
- MODIS
- FRP
- uncertainty
- bow-tie effect
- biomass burning
- active fire characterization
- ENERGY
- ALGORITHM
- AMERICA
- HEIGHTS
- AFRICA
- SYSTEM
- NORTH