HR: 0830h
AN: A21D-0995 [PDF]
TI: Calibration of TOMS Radiances From Ground Observations
AU: * Bojkov, B R
EM: bojkov@ventus.gsfc.nasa.gov
AF: Science Systems and Applications, Inc., 10210 Greenbelt Road, Suite 600, Lanham, MD 20706 United States
AU: Kowalewski, M G
EM: mattk@ventus.gsfc.nasa.gov
AF: Science Systems and Applications, Inc., 10210 Greenbelt Road, Suite 600, Lanham, MD 20706 United States
AU: Wellemeyer, C G
EM: cgw@qhearts.gsfc.nasa.gov
AF: Science Systems and Applications, Inc., 10210 Greenbelt Road, Suite 600, Lanham, MD 20706 United States
AU: Labow, G J
AF: Science Systems and Applications, Inc., 10210 Greenbelt Road, Suite 600, Lanham, MD 20706 United States
AU: Hilsenrath, E
AF: NASA Goddard Space Flight Center, NASA Goddard Space Flight Center
Code 916, Greeenbelt, MD 20771 United States
AU: Bhartia, P K
AF: NASA Goddard Space Flight Center, NASA Goddard Space Flight Center
Code 916, Greeenbelt, MD 20771 United States
AU: Ahmad, Z
AF: Science and Data Systems, 16509 Copperstrip Lane, Silver Spring, MD 20906 United States
AB:
Verification of a stratospheric ozone recovery remains a high priority for environmental research and policy definition.
Models predict an ozone recovery at a much lower rate than the measured depletion rate observed to date. Therefore improved
precision of the satellite and ground ozone observing systems are required over the long term to verify its recovery. We
show that validation of radiances from the ground can be a very effective means for correcting long term drifts of
backscatter type satellite measurements and can be used to cross calibrate all BUV instruments in orbit (TOMS, SBUV/2, GOME,
SCIAMACHY, OMI, GOME-2, OMPS). This method bypasses the retrieval algorithms used to derive ozone products from both
satellite and ground based measurements that are normally used to validate the satellite data. Radiance comparisons employ
forward models, but they are inherently more accurate than the retrieval algorithms.
This method employs very accurate comparisons between ground based zenith sky radiances and satellite nadir radiances and
employs two well established capabilities at the Goddard Space Flight Center, 1) the SSBUV calibration facilities and 2) the
radiative transfer codes used for the TOMS and SBUV/2 algorithms and their subsequent refinements. The zenith sky
observations are made by the SSBUV where its calibration is maintained to a high degree of accuracy and precision. Radiative
transfer calculations show that ground based zenith sky and satellite nadir backscatter ultraviolet comparisons can be made
very accurately under certain viewing conditions. Initial ground observations taken from Goddard Space Flight Center
compared with radiative transfer calculations has indicated the feasibility of this method. The effect of aerosols and
varying ozone amounts are considered in the model simulations and the theoretical comparisons. The radiative transfer
simulations show that the ground and satellite radiance comparisons can be made with an uncertainty of less than 1% without
the knowledge of the amount ozone viewed by either instrument on ground or in space.
To demonstrate this technique, nadir radiances from Earth Probe TOMS were compared with zenith sky observations over Goddard
Space Flight Center from 2001-2003 at three coincident wavelengths (312.5, 317.5 and 360 nm). These comparisons showed good
agreement between EP-TOMS radiances corrected by the flight diffuser and by polar ice observations.
DE: 1610 Atmosphere (0315, 0325)
SC: Atmospheric Sciences [A]
MN: 2003 Fall Meeting