Northern California’s Bear Fire produces a pyrocumulonimbus cloud
![GOES-17 “Red” Visible (0.64 µm, top left), Shortwave Infrared (3.9 µm, top right), Fire Temperature RGB + GLM Flash Extent Density (bottom left) and “Clean” Infrared Window (10.35 µm, bottom right) [click to play animation | MP4]](https://cimss.ssec.wisc.edu/satellite-blog/images/2020/09/norcal_4p-20200909_104425.png)
GOES-17 “Red” Visible (0.64 µm, top left), Shortwave Infrared (3.9 µm, top right), Fire Temperature RGB + GLM Flash Extent Density (bottom left) and “Clean” Infrared Window (10.35 µm, bottom right) [click to play animation | MP4]
A comparison of Suomi NPP VIIRS Day/Night Band (0.7 µm), Shortwave Infrared (3.74 µm) and Infrared Window (11.45 µm) images (below) displayed the initial 2 pyroCb cloud pulses shortly after their formation. Side-illumination from the Moon (which was in the Waning Gibbous phase, at 59% of Full) allowed for a distinct shadow to be cast northwest of the colder/taller pyroCb pulse — and the pyroCb clouds exhibited a darker appearance than the layer of low-altitude smoke to the west, likely due to very high amounts of fresh smoke contained within the rapidly-rising cloud turrets.
![Suomi NPP VIIRS Day/Night Band (0.7 µm), Shortwave Infrared (3.74 µm) and Infrared Window (11.45 µm) images [click to enlarge]](https://cimss.ssec.wisc.edu/satellite-blog/images/2020/09/200909_1020utc_suomiNPP_viirs_infrared_dayNightBand_shortwaveInfrared_Bear_Fire_CA_pyroCb_anim.gif)
Suomi NPP VIIRS Day/Night Band (0.7 µm), Shortwave Infrared (3.74 µm) and Infrared Window (11.45 µm) images [click to enlarge]
![GOES-17 True Color RGB images [click to pay animation | MP4]](https://cimss.ssec.wisc.edu/satellite-blog/images/2020/09/GOES-17_ABI_RadC_true_color_2020253_150117Z.png)
GOES-17 True Color RGB images [click to pay animation | MP4]