579
SPECTRAL VARIABILITY EFFECTS ON THE ATMOSPHERIC CORRECTION OF
IMAGING SPECTROMETER DATA FOR SURFACE REFLECTANCE RETRIEVAL
P.M. Teillet
Canada Centre for Remote Sensing
1547 Merivale Road, Nepean, Ontario, Canada K2G 4V3
and
J.R. Irons
Biophysical Sciences Branch
NASA Goddard Space Flight Center, Greenbelt, Maryland, USA 20771
ABSTRACT
Based on apparent radiances (nadir-looking) from
the airborne Advanced Solid-State Array Spectro-
radiometer (ASAS) and measured optical depth
values, a surface reflectance spectrum was
computed by an atmospheric code run (i) monochro-
matically at band center wavelengths, (ii) for
rectangular bandpasses, and (iii) for spectral
response profiles. A comparison of the results
from these different cases indicates that
anomalous results for surface reflectance can be
obtained in the vicinity of absorption features in
the monochromatic case and that bandpass computa
tions yield better results. Even with bandpass
calculations, if there is no information available
on gaseous absorption at the time of image
acquisition and standard values are used in the
atmospheric correction of high spectral resolution
data, it is shown that the retrieved surface
reflectances can depart significantly from normal
values in spectral regions affected by absorption.
INTRODUCTION
In remote sensing, an atmospheric radiative
transfer code is used to determine surface
reflectances given image data acquired by
satellite or aircraft sensors. The more accurate
models of radiative transfer through the
atmosphere are complex and can require a lot of
computer processing time. Thus, in remote sensing
studies, such models are often run monochromati-
cally to represent a spectral band in order to
save time. With the relatively narrow bands of
imaging spectrometers, such an approach should
work well throughout most of the relevant spectral
domain. However, the narrowness of the imaging
spectrometer bands also implies greater
sensitivity to atmospheric absorption features,
which can be very spectrally selective.
The effects of these factors on atmospheric
correction of imaging spectrometer data were
examined using data from the airborne Advanced
Solid-state Array Spectroradiometer (ASAS), used
by the NASA Goddard Space Flight Center for
multiple direction reflectance observations (Irons
et al., 1989). The sensor primarily consists of
a charge injection device with a 512 by 29 silicon
photodetector array. A diffraction grating is
used to distribute the spectral information onto
the 29-array dimension, from which 29 channels are
obtained in the 465-871 nm range. For a flight
altitude of 5000 feet, the nadir pixel size is 4.5
m across track. The data acquisition strategy is
to change the pointing direction of the sensor
from 45 degrees fore to 45 degrees aft while
flying over a specific target location. In this
way, seven images are acquired at 15 degree
increments in view angle for a given target area.
Thus, ASAS is a particularly useful instrument for
studying bidirectional reflectance distribution
functions of natural surfaces.
ASAS data were acquired by NASA over Konza prairie
grass in 1987 as part of the First ISLSCP Field
Experiment (FIFE), where ISLSCP stands for the
International Satellite Land Surface Climatology
Project. Radiometric calibration coefficients
were used to convert the data recorded during the
flight to physical radiance units. An individual
radiance spectrum was extracted from a nadir image
acquired over vegetation. In the present
atmospheric correction study, attention was
focused on 9 channels encompassing the spectral
range from about 0.670 to 0.805 micrometers, with
each individual channel having a bandwidth of
0.015 micrometers. This portion of the
reflectance spectrum of vegetation includes the
chlorophyll minimum in the visible and the rise up
to the infrared plateau region. The feasibility
of retrieving surface reflectances from the
measured radiances has been investigated with the
help of the 5S atmospheric code (Tanre et al.,
1986; Teillet, 1989).
ANALYSIS AND RESULTS
Monochromatic Case
Based on the input conditions listed in Table 1
and the ASAS apparent radiances, surface
reflectances were computed by 5S monochromatically
at the band center wavelengths listed in Table 2.
However, computations in the 5S code are tied to
a wavelength grid with 0.005 micrometer spacing.
Thus, if the specified wavelength is 0.678 micro
meters, for example, the code will actually
generate results for a wavelength of 0.680 micro
meters, the nearest grid wavelength. Results from
this approach are listed in Table 2 under the
heading "5S LAMBDA GRID".
Rectangular Bandpass Case
Each individual ASAS band is not monochromatic but
rather has a bandwidth of 0.015 micrometers. A
rectangular bandpass was adopted and used in a
second series of 5S runs to approximate the
spectral response profile of each ASAS channel.
The results are presented in Table 2 under the
heading "5S BAND (RECT)".
Profile Bandpass Case
It can be argued that a rectangular bandpass of
0.015 micrometers is not very representative of