Weekly Report on GOES-14 PLT Science Test
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Weekly Report on
GOES-14 PLT Science Test
NOAA / NESDIS / STAR
X. Wu, G. Rancic, F. Yu, M. Grotenhuis
December 14, 2009
1
Initial Post-Launch Calibration of
GOES-14 Imager Visible Channel by Moon
Purpose:
Verify pre-launch calibration
Establish benchmark for trending
Method:
Vicarious calibration based on lunar observations.
Data:
GOES-14 lunar observations on 08/10/2009.
Analysis:
Lunar irradiances are calculated per Wu & Yu (2006).
ROLO predicted irradiances are obtained (courtesy of Dr. Tom Stone of
USGS).
2
GOES-14 observed and ROLO model
predicted lunar irradiances and their ratios
GOES-14 Lunar Calibration
GOES ROLO Ratio
0.92 1.030
3. The ratio is not constant, likely due to
0.90
angular dependence of scan mirror reflectance 1.020
Irradiance (W m^-2 um^-1) or Ratio (no unit)
that will be addressed separately.
GOES/ROLO Ratio (no unit)
0.88 1.010
2. The measured irradiance
0.86
generally follows the 1.000
predicted trend.
1. The predicted lunar
irradiance decreases
0.84 0.990
with the waning moon
0.82 0.980
20.4 20.6 20.8 21.0 21.2 21.4 21.6 21.8 22.0
Time (UTC on 10 Aug 2009)
3
Preliminary results
The GOES-14 Imager visible channel appears
~1% brighter than predicted by the ROLO model.
Well within the uncertainty of Lunar based post-
lunch calibration (>2%).
It has been observed for several AVHRR’s that
measurements are initially brighter then expected.
Further evaluation by other vicarious calibration
will follow.
4
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