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

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172<br />

III - FIRE DETECTION AND FIRE MONITORING<br />

to be false detects and adding fires that the algorithms have not detected.<br />

False detects can be due to a number of c<strong>on</strong>diti<strong>on</strong>s including urban heat<br />

islands, solar specular reflecti<strong>on</strong> off water surfaces, highly reflective clouds,<br />

relatively brighter vegetated land embedded within darker areas, instrument<br />

noise, etc. <strong>Fire</strong>s not detected by the algorithms can be attributed to<br />

partial obscurati<strong>on</strong> by clouds, overhead vegetati<strong>on</strong> canopy, detected temperature<br />

that is not sufficiently hot or hotter than the surrounding area,<br />

etc. Validati<strong>on</strong> results (Schroeder et al., 2008) using 30m ASTER data found<br />

that fires added by analysts reduced the omissi<strong>on</strong> error rate compared to<br />

WFABBA and MODIS detecti<strong>on</strong>s. However, the commissi<strong>on</strong> error rate was not<br />

reduced by automated detecti<strong>on</strong>s that were deleted, with actual fires being<br />

err<strong>on</strong>eously removed. Validati<strong>on</strong> using ground based reports from Florida,<br />

M<strong>on</strong>tana, Idaho and Manitoba supported the finding of reduced omissi<strong>on</strong><br />

errors in the HMS compared to the automated <strong>on</strong>ly product (WFABBA,<br />

MODIS and FIMMA) with approximately twice as many detecti<strong>on</strong>s, although<br />

the overall detecti<strong>on</strong> rate was <strong>on</strong>ly 25-30%. The low detecti<strong>on</strong> rate is<br />

ascribed to the small size (less than 2 ha) of many of the fires as well as<br />

prohibitive cloud cover. HMS products may be accessed at<br />

www.osdpd.noaa.gov/ml/land/hms.html.<br />

2 - Smoke Detecti<strong>on</strong> and Model Transport<br />

Smoke detecti<strong>on</strong> is exclusively performed with visible imagery, primarily<br />

utilizing animated GOES data, although polar imagery is occasi<strong>on</strong>ally used.<br />

Detecti<strong>on</strong> is optimized over the c<strong>on</strong>tiguous US with GOES-West in the morning<br />

and GOES-East in the evening due to favorable solar zenith and satellite<br />

viewing angles. Analysts graphically depict the smoke extent by manually<br />

drawing polyg<strong>on</strong>s. An estimate of the vertically integrated smoke c<strong>on</strong>centrati<strong>on</strong><br />

is assigned to each polyg<strong>on</strong>. Three ranges of values (in µm/m 3 )<br />

are available for the analyst to assign to the polyg<strong>on</strong>. The automated GOES<br />

Aerosol and Smoke Product (GASP) (Knapp et al., 2005) which generates<br />

Aerosol Optical Depth (AOD) is a tool to aid analysts in this determinati<strong>on</strong>.<br />

The smoke depicted may be attached to actively burning fires or may be<br />

several days old and have drifted hundreds or thousands of km from the<br />

source.<br />

Many fires do not produce emissi<strong>on</strong>s that are detectable. Clouds obscure<br />

some smoke emissi<strong>on</strong>s while other fires may have minimal emissi<strong>on</strong>s due to<br />

the short durati<strong>on</strong> of the fire, limited biomass or the engineering of the fire<br />

in the case of agricultural/prescibe burns. For fires producing smoke that is<br />

detected the analyst provides an estimate of the initiati<strong>on</strong> and durati<strong>on</strong> of<br />

emissi<strong>on</strong>s and a coarse estimate of the fire size. The size is ideally estimated<br />

using higher (1km) resoluti<strong>on</strong> polar data with the fire close to the<br />

suborbital track. This is not always possible, especially in dynamic wildfire<br />

situati<strong>on</strong>s in the mid and lower latitudes. In these cases the analyst pro-

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