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IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING 1
Improving the Calibration of Suomi NPP VIIRS
Thermal Emissive Bands During Blackbody
Warm-Up/Cool-Down
Wenhui Wang , Changyong Cao, Alexander Ignatov , Xingming Liang, Zhenglong Li,
Likun Wang, Bin Zhang, Slawomir Blonski, and Jun Li
Abstract— The Suomi National Polar-orbiting Partnership
Program Visible Infrared Imaging Radiometer Suite (VIIRS)
thermal emissive bands (TEB) have been performing well during
nominal operations since launch. However, small but persistent
calibration anomalies are observed in all TEBs during the quar-
terly blackbody (BB) warm-up/cool-down (WUCD) events. As a
result, the time series of daytime sea surface temperature (SST)
(derived from bands M15–M16) show warm spikes on the order
of 0.25 K. This paper suggests that VIIRS TEB WUCD biases
are band dependent, with daily-averaged biases about -0.04 and
0.05 K for I4 and I5, and -0.05, -0.05, 0.11, 0.09, and 0.05 K
for M12–M16, respectively. Two correction methods—Ltrace
and WUCD-C—have been implemented and evaluated using
colocated observations from the Cross-track Infrared Sounder
(CrIS), radiative transfer simulations, and SST retrievals. Also an
error in the National Oceanic and Atmospheric Administration
operational processing was identified and fixed. Both correction
methods effectively minimize WUCD-induced SST anomalies.
The Ltrace method works well for I5, M12, and M14–M16,
with residual biases about 0.01 K. The WUCD-C method,
on the other hand, performs well to correct WUCD biases
in all TEBs, with residual biases also about 0.01 K. How-
ever, it introduces warm biases relative to CrIS at cold scene
temperatures, which requires further study. Applying nonequal
BB thermistor weights improves calibration at BB temperature
set points, but its impact on daily-averaged WUCD biases is
small. The proposed methodologies may also be applied to
the VIIRS onboard the follow-on Joint Polar Satellite System
satellites.
Index Terms— Blackbody (BB) warm-up/cool-down (WUCD),
radiometric calibration bias, sea surface temperature (SST)
anomaly, sensor data record (SDR), Suomi National Polar-
orbiting Partnership (S-NPP), thermal emissive bands (TEB),
Visible Infrared Imaging Radiometer Suite (VIIRS).
Manuscript received December 24, 2017; revised July 5, 2018;
accepted August 13, 2018. This work was supported by NOAA STAR
through the Joint Polar Satellite System Program. (Corresponding author:
Wenhui Wang.)
W. Wang, X. Liang, S. Blonski, and B. Zhang are with Earth Resources
Technology, Inc., Laurel, MD 20707 USA (e-mail: wenhui.wang@noaa.gov).
C. Cao and A. Ignatov are with the NOAA/Center for Satellite Applications
and Research, College Park, MD 20740 USA.
Z. Li and J. Li are with the Cooperative Institute for Meteorological Satellite
Studies, University of Wisconsin–Madison, Madison, WI 53706 USA.
L. Wang and B. Zhang are with CICS/ESSIC, University of Maryland,
College Park, MD 20740 USA.
Color versions of one or more of the figures in this paper are available
online at http://ieeexplore.ieee.org.
Digital Object Identifier 10.1109/TGRS.2018.2870328
I. I NTRODUCTION
T
HE Visible Infrared Imaging Radiometer Suite (VIIRS)
onboard the Suomi National Polar-orbiting Partner-
ship (S-NPP) satellite was successfully launched on
October 28, 2011. The National Oceanic and Atmospheric
Administration (NOAA) VIIRS sensor data records (SDRs),
produced operationally by the interface data processing seg-
ment (IDPS), became available on January 20, 2012 and
achieved validated maturity on March 19, 2014. VIIRS has
seven thermal emissive bands (TEBs), including two imagery
resolution bands (I4 and I5) and five moderate reso-
lution bands (M12–M16), covering spectral range from
3.697 to 11.845 μm. S-NPP VIIRS TEB calibration has been
performing well during nominal operations since launch. How-
ever, small but persistent calibration anomalies have been
observed in all TEBs during the quarterly blackbody (BB)
warm-up/cool-down (WUCD) events, which are performed
to characterize on-orbit calibration offset and nonlinearity
changes over time [1]–[3]. During such events, VIIRS daytime
sea surface temperature (SST) product, which uses bands
M15 and M16 as primary inputs, becomes anomalous with
warm biases shown as spikes in the SST time series on
the order of 0.25 K [4] as seen in the NOAA SST Quality
Monitor system [5]. Accurate and stable satellite SST data are
critical to numerical weather prediction, seasonal, and climate
applications. The VIIRS TEB calibration anomalies during
WUCD negatively impact the SST analysis according to the
users, and therefore need to be addressed to better support
these applications.
Cao et al. [1] analyzed the SST WUCD anomalies and
attributed them primarily to a warm bias in M15 during the
BB cooling phase of the WUCD, which is further ampli-
fied by the SST retrieval algorithm. The study suggests that
the root cause of the WUCD calibration bias is the flawed
theoretical assumption in the TEB calibration equations that
the shape of the calibration curve remains unchanged on-
orbit from that determined prelaunch. The assumption is not
working well during the WUCD events when the temperature
of BB is unstable. A localized correction method, with a
diagnostic correction term (Ltrace), was introduced to rec-
oncile the flawed assumption in the calibration algorithm
and to significantly minimize the WUCD-induced calibration
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