STAR Joint Polar Satellite System Algorithms & Data Products website National Oceanographic & Atmospheric Administration website NOAA Center for Satellite Applications and Research website

NOAA-21 First Light Images

NOAA-21 ATMS First Light Image, 22 November 2022

STAR JPSS has produced first light imagery from the recently launched NOAA-21 satellite. The image selected shows the Channel 18 (183 Ghz) Brightness Temperature for the ascending node on November 21-22. ATMS is the first NOAA-21 instrument to be activated.

Thanks and credit: STAR ATMS SDR Team. Click images to enlarge.

NOAA-21 CrIS First Light Image, 12 Feb 2023

NOAA-21 CrIS First Light Image - The CrIS sensor provides hyperspectral infrared observations over 2,211 channels with high radiometric and spectral accuracy. The first light image in brightness temperature was captured by the NOAA-21 CrIS sensor at the 1596 cm-1 water vapor channel on February 12, 2023. This image shows the large-scale waves of upper tropospheric water vapor and clouds over the Earth�s globe.

Thanks and credit: STAR CrIS SDR Team. Click images to enlarge.

NOAA-21 VIIRS First Light Image, 6 December 2011
The STAR VIIRS SDR team has produced first light imagery from the VIIRS visible bands. The image shows true color imagery from December 5. The VIIRS visible/near infrared bands were the second instrument to be activated, with the VIIRS thermal bands, CRIS, and OMPS to follow in February.

Thanks and credit: STAR VIIRS SDR Team. Click images to enlarge.

NOAA-21 OMPS NM First Light Image, 18 February 2023

NOAA-21 OMPS NM First Light Image - The Ozone Mapping Profiler Suite (OMPS) instrument on the NOAA-21 satellite acquired its first data on February 18, 2023. This first-light image shows the radiance values for the cloud reflectivity channel on the OMPS Nadir Mapper. The highest radiances are associated with bright cloud tops. The cloud reflectivity channel is one of the five primary channels used to estimate total ozone concentration. The striping pattern is created from the slight differences in the angle of the satellite relative to the incoming energy from the sun.

Thanks and credit: STAR OMPS SDR Team. Click images to enlarge.