IAPRS & SIS, Vol.34, Part 7, “Resource and Environmental Monitoring”, Hyderabad, India,2002
IMPACT OF ON-BOARD HYPERSPECTRAL DATA COMPRESSION ON MINERAL
MAPPING PRODUCTS
K. Staenz ? , R. Hitchcock P , S. Qian ? , and R.A. Neville ?
? Canada Centre for Remote Sensing, Natural Resources Canada, 588 Booth Street, Ottawa, ON,
Canada K1A 0Y7 (karl.staenz Q ccrs.nrcan.gc.ca)
P Prologic Systems Ltd., 75 Albert Street, Suite 206, Ottawa, ON, Canada
(robert.hitchcock G ccrs.nrcan.gc.ca) ©) Canadian Space Agency, 6767 Route de 1’ Aéroport, St. Hubert, QC, Canada J3Y 8Y9
(Shen-en.Qian G space.gc.ca)
Commission VII, WG VII/1
KEY WORDS: Hyper spectral, Geology, Compression, Processing, Classification, Impact Analysis
ABSTRACT:
As on-board data compression is an option for future operational hyperspectral satellite systems, its impact on the data products need
to be investigated. Accordingly, the study presented in this paper investigated the impact of lossy Hierarchical Self-organizing
Cluster Vector Quantification (HSOCVQ) data compression on the identification and mapping of minerals in environments with
sparse vegetation cover. For this purpose, an Airborne Visible/Infrared Imaging Spectrometer (AVIRIS) radiance cube acquired over
the Cuprite mining district area in Nevada on June 12, 1996 was compressed by factors of 10, 20, and 40. The original data and the
de-compressed data were processed separately, applying atmospheric correction using MODTRAN4.2 and spectra post-processing
prior to automatic Iterative Error Analysis (IEA) endmember selection, and subsequent constrained spectral linear unmixing to
produce mineral (endmember) abundance maps. The results indicate that the errors between original radiance data and de-
compressed data increase with increasing compression ratio. This trend is also true for the derived mineral abundance maps. In
general, for most of the endmembers, the 10:1 and 20:1 compression ratios produced abundance maps which are spatially similar to
those extracted from the original data, when only fractions larger than 0.5 are mapped. Only these higher fractions are of interest for
exploration purposes. One endmember out of 15 was lost using the 40:1 compression ratio and, consequently, this particular
endmember could not be mapped.
1.0 INTRODUCTION
With the launch of spaceborne hyperspectral sensors, data
transmission becomes an issue due to the high data rate
required to cope with the large volumes of hyperspectral data.
This is especially true when moving towards operational
systems, as compared to technology demonstrators such as
NASA's Hyperion. In order to overcome this problem, lossy
data compression can be used to reduce the data volume while
preserving enough information for the generation of application
products in various areas, such as forestry, agriculture,
environment, coastal/inland waters, and geoscience. Suitable
data compression techniques are those which use Vector
Quantization (VQ) (Qian et al, 1997 and 2000). These
techniques are characterised by their near lossless property with
high compression ratio and relatively simple structure.
The goal of this study is to apply a VQ compression technique,
called the “Hierarchical Self-organizing Cluster Vector
Quantification” (HSOCVQ: Qian et al, 2002), to calibrated
(radiance) hyperspectral airborne data to investigate the impact
of this technique on mineral mapping products. For this
purpose, an Airborne Visible/Infrared Imaging Spectrometer
(AVIRIS: Green et al., 1998) data set acquired on June 12,
1996 over a test site near Cuprite, Nevada, U.S.A., was used.
The products retrieved from data compressed with HSOCVQ
were compared quantitatively and qualitatively with the
products extracted from the original (uncompressed) data. The
ratios used in the compression are 10:1, 20:1, and 40:1. The
subsequently de-compressed data sets were processed in the
same way as the original data. Major processing steps include
the removal of atmospheric effects, automatic extraction of
endmembers, and application of a constrained linear spectral
unmixing technique to map the minerals. These processing
steps were carried out using the Imaging Sp ectrometer Data
Analysis System (ISDAS: Staenz et al., 1998) developed at the
Canada Centre for Remote Sensing. The paper describes in
detail the aforementioned processing steps together with the
extracted results. Special emphasis is given to the analysis of
the end products (fractions of minerals) but also to the
comparison of intermediate outputs such as the endmembers.
2.0 DATA USED
A Cuprite standard Jet Propulsion Laboratory (JPL) AVIRIS
data set, collected on June 12, 1996, has been used for this
study. This sensor acquires imagery at approximately 20-m
ground resolution from an ER-2 aircraft in 224 spectral bands,
each about 10 nm wide, in the 400-nm to 2500-nm wavelength
range. Additional information for identification of endmembers
includes the USGS (2002) spectral data base.
The site selected for this study lies within the Cuprite mining
district of Nevada (37.6 °N and 117.2 ° W). This site has been
used as a test area for mineral mapping in hyperspectral remote
sensing for many years (Goetz and Srivastava, 1985; Hook and
Rast,..1990; Swayze et.31,.1992; Neville et al, 2003).
Accordingly, this site is very well characterized in terms of
mineralogy. This and the excellent exposure of alteration
minerals such as alunite, kaolinite, buddingtonite, and others
together with limited soil development and sparse vegetation