Image Standardization
(At-Sensor Reflectance and COST Correction)
Image
standardization is the process of normalizing image pixel values for
differences in sun illumination geometry, atmospheric effects and instrument
calibration. Standardizing
imagery improves the ability to mosaic adjacent imagery and compare
imagery over time (e.g. change detection).
Because some procedures involve collecting in-situ atmospheric
measurements and radiometric transfer code (RTC), they are difficult
and more costly to implement. The procedures used by this website
are image-based, requiring no additional information other than that
provided by the imagery.
This
website provides three tools that create ERDAS Imagine
TM spatial models (.gmd format).
Each tool creates a different .gmd file providing
a slightly different approach to standardization. These tools are designed for Landsat 5 TM and Landsat
7 ETM+ scenes and require, as input, the header file (*.h1) accompanying
NLAPS formatted imagery from the USGS at Eros Data Center.
1)
DN-to-Reflectance
Conversion:
This tool creates a spatial model (.gmd file) that
converts the image’s digital numbers (DN, or voltage measurements) to
at-sensor radiance and computes at-sensor reflectance while normalizing
solar elevation angle. The equation
is as follows:

Where,
rBandN = Reflectance for Band N
LbandN = Digital Number for Band N
D
= Normalized Earth-Sun Distance
EbandN = Solar Irradiance for Band N
2) COST
Atmospheric Correction:
This tool creates a spatial model (.gmd file) that
converts DN to reflectance as in tool # 1, but in addition includes
an image-based atmospheric correction procedure using the Chavez (1996)
COST method. The equation is
as follows:

Where,
rBandN = Reflectance for Band N
LbandN = Digital Number for Band N
HbandN = Digital Number representing Dark Object
for Band N
D
= Normalized Earth-Sun Distance
EbandN = Solar Irradiance for Band N
t = Atmospheric Transmittance
expressed as 
3) COST
without Tau (Dark Object Subtraction) Atmospheric Correction:
This tool creates a spatial model (.gmd file) using
the Chavez (1996) COST method, with the exception that it omits Tau
(t). The equation is as follows:

Where,
rBandN = Reflectance for Band N
LbandN = Digital Number for Band N
HbandN = Dignal Number representing Dark Object
for Band N
D
= Normalized Earth-Sun Distance
EbandN = Solar Irradiance for Band N
Frequently
Asked Questions
References:
Chavez, P.S. Jr., 1996, Image-based atmospheric corrections—revisited
and revised. Photogrammetric
Engineering and Remote Sensing 62(9): 1025-1036.
Chengquan Huang, Limin Yang, Collin Homer, Bruce
Wylie, James Vogelman and Thomas DeFelice, 2002. At-satellite reflectance: A first normalization of Landsat 7 ETM+ Images.
WWW URL: http://landcover.usgs.gov/pdf/huang2.pdf,
US Dept. of Interior, USGS.
Markam, B. L. and Barker. J. L. 1986, Landsat MSS
and TM post-calibration dynamic ranges, exoatmospheric reflectances
and at-satellite temperatures, EOSAT Landsat Technical Notes, 1: 3-8
DISCLAIMER: The
tools on this website are designed for the purposes outlined above. The RSGIS lab recommends you test the models
prior to using them. The tools
on this website are provided “as-is,” without warranty of any kind,
express or implied. The RSGIS
lab and Utah State University do not warrant that the operation of the
tools shall be error free. Users bear all risk as to the quality and performance
of the tools.
Download
.exe versions of these tools (password required)
If you have questions or comments regarding this
website, please contact jlowry@cnr.usu.edu
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