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7th Workshop on Forest Fire Management - EARSeL, European ...

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188<br />

III - FIRE DETECTION AND FIRE MONITORING<br />

a gradient of fire types); (ii) Airborne Hyperspectral Sensor (AHS) data<br />

(opportunistic imaging of several vegetati<strong>on</strong> fires at ~1.5m resoluti<strong>on</strong>);<br />

(iii) China-Brazil Earth Resources Satellite (CBERS) (burned area mapping<br />

at 20m resoluti<strong>on</strong> with 26 day repeat cycle); (iv) Advanced Spaceborne<br />

Thermal Emissi<strong>on</strong> and Reflecti<strong>on</strong> Radiometer and Landsat Thematic Mapper<br />

(TM and ETM+) (active fire detecti<strong>on</strong> and burned area mapping at 30m resoluti<strong>on</strong><br />

with 16 day repeat cycle); (v) Moderate Resoluti<strong>on</strong> Imaging<br />

Spectroradiometer (MODIS) <strong>on</strong>board Terra and Aqua satellites (1km active<br />

fire detecti<strong>on</strong> and characterizati<strong>on</strong> from the Thermal Anomalies (TA) product<br />

– 12hour interval (can be reduced depending <strong>on</strong> use); and (vi)<br />

Geostati<strong>on</strong>ary Operati<strong>on</strong>al Envir<strong>on</strong>mental Satellite (GOES) imager (4km<br />

active fire detecti<strong>on</strong> and characterizati<strong>on</strong> from the Wild<strong>Fire</strong> Automated<br />

Biomass Burning Algorithm (WF-ABBA) – 30min interval).<br />

2.1 - <strong>Fire</strong> Product Assessment<br />

Our assessment of the TA and WF-ABBA fire products built <strong>on</strong> the study of<br />

Morisette et al. (2005). We used coincident and near coincident higher spatial<br />

resoluti<strong>on</strong> data to map sub-pixel fires within the MODIS and GOES imager<br />

footprints (see Giglio et al., 2008; Csiszar et al., 2006; Schroeder et al.,<br />

2008c). The effects of short-term variati<strong>on</strong>s in fire behavior were analyzed<br />

using Landsat ETM+ and ASTER data acquired 30min apart (see Csiszar and<br />

Schroeder, 2008). We used the Vegetati<strong>on</strong> C<strong>on</strong>tinuous Fields (VCF) product<br />

to stratify our results in terms of the percentage tree cover found in and<br />

around the fire pixel area.<br />

2.2 - C<strong>on</strong>siderati<strong>on</strong> of Cloud Obscurati<strong>on</strong> Omissi<strong>on</strong> Errors<br />

Opaque clouds can greatly reduce the ability to detect fires using spaceborne<br />

instruments due to severe attenuati<strong>on</strong> of the spectral signal emitted<br />

by either flaming or smoldering phases of biomass combusti<strong>on</strong>. In order<br />

account for the resulting omissi<strong>on</strong> errors, we applied a probabilistic<br />

approach to the WF-ABBA product over Brazilian Amaz<strong>on</strong>ia using precipitati<strong>on</strong><br />

estimates, a cloud mask, and land use data, all derived from the GOES<br />

imager data (for details see Schroeder et al., 2008b).<br />

2.3 - <strong>Fire</strong> Characterizati<strong>on</strong><br />

<strong>Fire</strong> characterizati<strong>on</strong> is required in order to understand the processes leading<br />

to and resulting from biomass burning. Currently, fire size and temperature<br />

estimates are calculated by the WF-ABBA product, whereas both WF-<br />

ABBA and TA provide estimates of <strong>Fire</strong> Radiative Power. In order to assess<br />

those parameters we used coincident data from ASTER and Landsat ETM+.

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