Paper mill fire in New Jersey
GOES-16 Near-Infrared “Snow/Ice” (1.61 µm, top), Near-Infrared “Cloud Particle Size” (2.24 µm, center) and Shortwave Infrared (3.9 µm, bottom) images, with hourly plots of surface observations [click to play animation | MP4]
The nighttime thermal signatures seen on the near-infrared 1.61 µm and 2.24 µm images (brighter white pixels) result from the fact that those two ABI spectral bands are located close to the peak emitted radiance of very hot features such as volcanic eruptions or large fires (below).
![Plots of Spectral Response Functions for ABI Bands 5, 6 and 7 [click to enlarge]](https://cimss.ssec.wisc.edu/satellite-blog/wp-content/uploads/sites/5/2018/08/ABI_Band_5_6_7_Spectral_Response_Functions_Fires.png)
Plots of Spectral Response Functions for ABI Bands 5 (1.61 µm), 6 (2.24 µm) and 7 (3.9 µm) [click to enlarge]