Insufficient observing assets exist with fine resolution and rapid refresh that focus on pre-fire analysis of vegetation to fully understand rate-of-spread potential just prior to and during wildland fire events. GEO and LEO satellite-based pre-fire and active fire products are important components to wildfire management, but suffer from moderate to poor spatial resolution and/or sporadic revisit times. Landsat multispectral data provides fine resolution vegetation data, but at the cost of lengthy revisit times (two weeks).
This presentation will provide a description of a unique sensing system to provide the potential for supporting pre-fire vegetation and fuels modeling along with active fire monitoring, all supporting near-RT predictive modeling of wildfire spread. MIT LL is developing the Chrisp Compact VNIR/SWIR Imaging Spectrometer (CCVIS) that provides spectral imaging from 0.4 mm to 2.5 mm (Mercury Cadmium Telluride, MCT) or 1.7 mm (InGaAs). The imaging spectrometer is mated to a MIT LL developed Digital Focal Plane Array (DFPA) to lower the noise floor to fully measure radiance for fire temperatures out to 1200 C for both day or night scenes.
A hyperspectral spectrometer will permit identification of land cover properties including vegetation or infrastructure, as well as vegetation moisture (greenness) and stress. Conceived to fly on a 12u CubeSat, the hyperspectral imager would be capable of: observing wildfire fuels and vegetation health pre-fire, characterizing fire perimeters and intensity during active fires, observing changes in land cover due to fire damage, and tracking wildfire smoke during controlled burns. A discussion of the benefits of using SWIR bands to track and measure wildfire characteristics will be given including sensitivity to fire radiative temperature and smoke obscuration. A development timeline will be provided as well as design challenges and solutions with respect to wildfire measurements.

