Sevilleta
National Wildlife Refuge, near Albuquerque, New Mexico
\log
12/20/97
- Date this file created. G. Shore.
10/30/01 - Added date/time fields to
APPENDIX II section. G. Shore.
\doc
##############################################################
DATA
SET CODE AND TITLE
SEV031 AVHRR Biweekly Composites (1994)
##############################################################
ABSTRACT
This dataset contains 16 separate 14-day
composited AVHRR
images for 1994 clipped approximatedly to the New Mexico
State
boundaries (plus 50 Km buffer around boundary). These were
obtained from the U.S.
Geological Survey's EROS Data Center (EDC),
National Mapping Division,
from the "CONTERMINOUS U.S. AVHRR BIWEEKLY
COMPOSITES" CD
product series.
##############################################################
KEYWORDS
SEV031
AVHRR Advanced_Very_High_Resolution_Radiometer NOAA Satellite_Imagery
Remote_Sensing USGS_EROS_Data_Center 1994
##############################################################
TABLE
OF CONTENTS
I. WHY THE DATA WERE
COLLECTED
II. WHEN THE DATA WERE
COLLECTED
III. WHO IS INVOLVED
WITH THE DATA
IV. WHERE TH DATA
WERE COLLECTED
V. HOW THE DATA
WERE COLLECTED AND PROCESSED BY THE USGS EDC
VI. HOW THE DATA WERE PROCESSED BY THE SEVILLETA IMS (SIMS)
VII. APPENDIX I - USGS EDC Metadata
VIII.
APPENDIX II - Pixel Date Attribute Table
##############################################################
I.
WHY THE DATA WERE COLLECTED
See the U.S. Geological Survey's EROS Data Center (EDC)
documentation
in APPENDIX I below.
##############################################################
II.
WHEN THE DATA WERE COLLECTED
Sixteen 14-day composites for 1994.
See the U.S. Geological
Survey's EROS Data Center (EDC)
documentation in APPENDIX I below
for specific composite periods.
##############################################################
III.
WHO IS INVOLVED WITH THE DATA
SOURCE AGENCY CONTACTS:
See the U.S. Geological Survey's EROS Data
Center (EDC) documentation
in APPENDIX I below for USGS EDC
contacts.
LOCAL SEVILLETA LTER CONTACTS:
Primary contact:
Greg Shore, Sevilleta LTER
(gshore@sevilleta.unm.edu).
Principle investigators:
Bruce Milne, Sevilleta LTER
(bmilne@sevilleta.unm.edu)
GIS/GPS specialist:
Greg Shore, Sevilleta LTER
(gshore@sevilleta.unm.edu).
Data Management
Greg Shore, Sevilleta LTER
(gshore@sevilleta.unm.edu)
##############################################################
IV.
WHERE THE DATA WERE COLLECTED
The original biweekly composited images covered the
Conterminous
United States. However, the images were
clipped
to the approximate New Mexico State boundaries (plus 50 Km
buffer
around boundary) for online access purposes, while the full
U.S.
scenes are stored offline on tape.
The clipping coordinates were
selected to perform exact clipping,
so no resampling was required.
The approximate online (NM clipped)
boundaries are:
Latitude/Longitude,
decimal degrees (Clarke 1866 spheroid)
XMIN: -109.515170 YMIN 30.759247 XMAX -102.454601 YMAX
37.817184
Lambert
Azimuthal Equal-area (see EDC document for projection info)
XMIN:
-914000 YMIN -1529000 XMAX -216000 YMAX -795000
The source and the clipped images
are in the following map projection:
Lambert
Azimuthal Equal Area projection
Parameters:
Radius of sphere 6,370,997.0 meters
Longitude of central meridian 100 00 00 West
Latitude of origin 45 00 00 North
False easting 0
False northing
0
Units of measure meters
Pixel size 1,000 meters
Each clipped image has
735 rows and 699 columns, and has a cell size
of 1000 x 1000 m.
See the U.S. Geological Survey's EROS Data
Center (EDC) documentation
in APPENDIX I below for spatial extent, projection
information, etc.,
related to the full Conterminous US scenes.
##############################################################
V.
HOW THE DATA WERE COLLECTED AND PROCESSED BY THE USGS EDC
See the U.S. Geological Survey's EROS Data
Center (EDC)
documentation in APPENDIX I below.
##############################################################
VI.
HOW THE DATA WERE PROCESSED BY THE SEVILLETA IMS (SIMS)
The general SIMS processing steps for each
biweekly composite
period were to read the 10 image bands off the source
USGS-EDC CD,
concatenate/import them into a 10-band ERDAS Imagine format
image
file, georegister to the USGS-EDC specifications, clip the
scene
to the approximate New Mexico State boundaries, move the
clipped
scene to the online SIMS archive, and write the full scene to
offline tape.
The
band order in the archived scenes is:
1- NOAA CHANNEL 1
6- NDVI
2- NOAA
CHANNEL 2 7- SATELLITE
ZENITH
3- NOAA CHANNEL
3 8- SOLAR ZENITH
4- NOAA CHANNEL 4
9- RELATIVE AZIMUTH
5- NOAA CHANNEL 5 10-
DATE
The bands are described in detail in the U.S. Geological
Survey's
EROS Data Center (EDC) documentation in APPENDIX I below. The
attribute data for the
"DATE" band is found in APPENDIX II below.
A more precise
description of the processing steps is as follows:
1. Mount AVHRR
CD
2. Read the 10 bands of information off the CD for each biweekly
composited
scene, concatenate
the 10 bands into a single file, then import as an
ERDAS Imagine 10-band image file (of
size 2889 rows x 4587 cols). This
process was automated with the C-shell script:
/db/local/imagery/bincom/avhrr_import.csh
94
NOTE: this
generates 10-band ERDAS Imagine format files, that are of
image size 2889 rows x 4587
cols, with filenames as follows:
avhrr94pPP.img
where: PP = bi-weekly growth period number
and bands in following
order::
1- NOAA
CHANNEL 1 6- NDVI
2- NOAA CHANNEL 2 7- SATELLITE ZENITH
3- NOAA CHANNEL 3 8- SOLAR ZENITH
4- NOAA
CHANNEL 4 9- RELATIVE
AZIMUTH
5- NOAA
CHANNEL 5 10- DATE
3.
Georegister the scene as follows:
Bring up ERDAS Imagine GUI, then Tools->ImageInfo tool and do:
1. File->Open->avhrr94pPP.img
2. Edit->Change Map Model:
a. Upper Left X: -2050000
b. Upper Left Y: 752000
c. Pixel Size X: 1000
d. Pixel Size Y: 1000
e. Units: meters
f. Projection: Lambert Azimuthal
Equal-area
NOTE: click OK,
then answer "Yes" to changing Map Model in all layers.
3. Edit->Add/Change Projection:
a. Spheroid Name: Sphere of Radius
6370997m
b. Datum Name:
Undefined
c. Longitude of
center of projection: 100:00:00 W
d. Latitude of center of projection: 45:00:00 N
e. False easting: 0.0 meters
f. False northing: 0.0 meters
NOTE: click OK, then answer
"Yes" to changing Map Model in all layers.
4. Edit->Change Layer Name:
a. Change bands 1 - 5 to Channel_1,
Channel_2, ..., Channel_5,respectively
b. Change band 6 to NDVI
c. Change bands 7 - 10 to SATELLITE_ZENITH, SOLAR
ZENITH,
RELATIVE_AZIMUTH, and
DATE, respectively
4. Clip full-scene to New Mexico minimum bounding
box (+50 Km buffer) with
coordinates ULx = -914000, ULy = -795000, LRx = -216000, LRy =
-1529000,
and dimensions 735
rows x 699 columns. This process was
automated with
the C-shell
scripts:
/db/local/imagery/bincom/batch_avhrr_clip2nm.csh, which calls:
/db/local/imagery/bincom/avhrr_clip2nm.csh avhrr94pPP.img
avhrr94pPPnm.img
NOTE: this generates 10-band ERDAS Imagine format files, that are
of
image size 735 rows x 699 cols, with
filenames as follows:
avhrr94pPPnm.img
5. Unix
compress the NM clipped image, make an archive directory, and move it
to the archive destination
(/db/archive/imagery/avhrr/avhrr94pPP/). This
process was automated with the C-shell scripts:
/db/local/imagery/bincom/avhrr_archive.csh
NOTE: this generates Unix compressed
files with filenames as follows:
avhrr94pPPnm.img.Z
6.
Compress (gzip) and archive the full scene image to 4mm DAT tape, then
remove from online disk:
gzip avhrr94pPP.img
mt -f /dev/rmt/0cn fsf <#>
tar cvf /dev/rmt/0cn
avhrr94pPP.img.gz
rm
avhrr94pPP.img.gz
7. Copy the most current yearly
"USGS-EDC-AVHRR Dataset README" file off CD for
inclusion in the online SIMS IAF metadata
file (avhrr94.dbf) for the images
(note, must also convert from DOS to Unix file):
dos2unix /cdrom/cdrom0/readme.1st
avhrr94readme.1st
8. Copy the "Date of Acquisition by
Pixel" attribute file off each CD, then
split by biweekly period for inclusion in GIS/RS Metadata
Abstract file
(avhrr94pPPnm.mda), and merge by year for inclusion in SIMS IAF
metadata
file
(avhrr94.dbf):
dos2unix
/cdrom/cdrom0/geom/date.att avhrr94pPP-PPdate.att
/db/local/imagery/bincom/batch_avhrr_split_dateatt.csh,
which calls:
/db/local/imagery/bincom/avhrr_split_dateatt.csh
/db/local/imagery/bincom/avhrr_concat_dates.csh 94 >
avhrr94date.att
9. Generate (this) SIMS IAF metadata file (i.e.,
avhrr94.dbf) using template
file
(avhrr_dbf.tmpl), appending readme file (avhrr94readme.1st), and date
file (avhrr94date.att).
10.
Generate GIS/RS Metadata Abstract file for each image, and put with
image in appropriate directory
(/db/archive/imagery/avhrr/avhrr94pPP/):
/db/local/imagery/bincom/get_avhrr_dates.csh 94 avhrr94.dbf
97 \
> avhrr94periods.txt
/db/local/imagery/bincom/batch_make_avhrr_abstract.csh
avhrr94periods.txt
which calls:
/db/local/imagery/bincom/make_avhrr_abstract.csh
##############################################################
VII. APPENDIX I - USGS EDC Metadata
THE 1994 CONTERMINOUS U.S. AVHRR
BIWEEKLY COMPOSITES
TABLE OF CONTENTS
Page
Preface.
. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1
Introduction . . . . . . . . . . . .
. . . . . . . . . . . . . . . . . .
1
Data Set Characteristics . . . . . . . . . . . . . . . . . . . .
. . . . .2
Procedures . . . . . . . . . . . . . . . . . . . . . . . . . .
. . . . . .5
Scene Selection . .
. . . . . . . . . . . . . . . . . . . . . . . . . .5
Satellite and Solar Viewing Geometry. . . .
. . . . . . . . . . . . . .6
Radiometric Calibration . . . . . . . . . . . . . . . . . . . . . . .
.7
Normalized Difference
Vegetation Index. . . . . . . . . . . . . . . . .9
Date of Acquisition . . . . . . . . . . . .
. . . . . . . . . . . . . 10
Geometric Registration. . . . . . . . . . . . . . . . . . . . . . . .
10
Compositing . . . . . . . . .
. . . . . . . . . . . . . . . . . . . . 13
Miscellaneous Data. . . . . . . . . . . . . . . . . . . . . . .
. . . 15
CD-ROM Organization. . . . . . . . . . . . . . . . . . . . . . .
. . . . 20
References . . . . . . . . . . . . . . . . . . . . . . . . . .
. . . . . 26
THE 1994 CONTERMINOUS U.S. AVHRR BIWEEKLY COMPOSITES
PREFACE
The
conterminous U.S. Advanced Very High Resolution Radiometer (AVHRR)
biweekly
composites data set provided in the past have been developed as
annual
data sets, with a single biweekly composite for January and February, a
continuous
series of biweekly composites for the months from March through
October,
and biweekly composites for the months of November and December. The
biweekly composites are produced
from afternoon acquisitions of NOAA-11 data.
Unfortunately, on September
13, 1994 the operational AVHRR sensor on board
NOAA-11 failed. Consequently, the 1994 conterminous U.S. AVHRR
biweekly data
set will be for the period of January through September 15,
1994.
INTRODUCTION
In 1987, the U.S.
Geological Survey's EROS Data Center (EDC), in Sioux Falls,
South Dakota,
began receiving Advanced Very High Resolution Radiometer (AVHRR)
data from
NOAA polar-orbiting satellites. The
central location of the EDC in
the United States enables direct reception
of all AVHRR overpasses of the
lower 48 States, as well as much of Canada
and Mexico. Early in the 1990
growing
season the EDC started acquiring NOAA-11 AVHRR 1-km resolution daily
observations
to produce weekly and biweekly maximum normalized difference
vegetation
index (NDVI) composites of the conterminous United States
(Eidenshink,
1992). The objective of the vegetation
mapping program is to
compile, annually, a comprehensive series of
calibrated, georegistered, daily
observations, and biweekly maximum NDVI
composites. These data are being
published
on CD-ROM for distribution of the data set.
These data sets can be
used in environmental monitoring and global
climate change studies.
The vegetation diversity of the conterminous
United States provides
opportunities for using both AVHRR data and the
NDVI for monitoring vegetation
condition in several different ecosystems,
including forests, agricultural
crops, and grasslands. The data set provides a comprehensive
growing season
profile of these ecosystems, is extremely useful for
assessing seasonal
variations in vegetation conditions, and provides a
foundation for studying
long-term changes resulting from human or natural
factors.
DATA SET CHARACTERISTICS
The data set is composed of sixteen 14-day
maximum NDVI composites, created
from nearly 300 NOAA-11 images. The sixteen core composite periods
represent
a continuous period from March 4, 1994, to September 15,
1994. The first two
(periods 1 and
2) composites represent a 2-week period each for January and
February. The 1994 data set is available as a set of
four CD-ROM's. Each of
the four
discs has four biweekly composites, miscellaneous data, and that are
described later in this
file. Each disc also contains the NDVI
statistics of
all counties in the conterminous United States for each
composite period.
Each
daily observation includes nine bands of information: AVHRR channels 1-5,
NDVI,
satellite zenith, solar zenith, and relative azimuth. The daily
observations have been calibrated to reflectance,
scaled to byte data, and
geometrically registered to the Lambert Azimuthal
Equal Area map projection.
Each 14-day composite includes 10 bands
of information, the 9 bands described
above for each daily observation and
a 10th band, which is a pointer to
identify the date of the source daily
observation scene. The data for
each
pixel in the composite are extracted from the daily observation scene
on the
basis of the maximum NDVI compositing process.
The
14-day composite periods for 1994 were:
____________________________________________________
Period Date of coverage Julian day
____________________________________________________
1
01/07 - 01/20/1994 007
- 020
2 02/11 - 02/24/1994 042 - 055
3
03/04 - 03/17/1994 063
- 076
4 03/18 - 03/31/1994 077 - 090
5
04/01 - 04/14/1994 091
- 104
6 04/15 - 04/28/1994 105 - 118
7
04/29 - 05/12/1994 119
- 132
8 05/13 - 05/26/1994 133 - 146
9
05/27 - 06/09/1994 147
- 160
10 06/10 - 06/23/1994 161 - 174
11
06/24 - 07/07/1994 175
- 188
12 07/08 - 07/21/1994 189 - 202
13
07/22 - 08/04/1994 203
- 216
14 08/05 - 08/18/1994 217 - 230
15
08/19 - 09/01/1994 231
- 244
16 09/02 - 09/15/1994 245 - 258
____________________________________________________
The
image dimensions of each band are 2,889 lines and 4,587 samples (13
megabytes).
NOTE: Prior to the 1994 image
compositing the format of the Land Analysis
System (LAS) files contained a
512 byte header record followed by data blocked
into 512 byte segments for
each line. As a result the dimension
increased to
4,608 samples. The
LAS software package no longer has this criteria. Actual
image data is processed and reported as 2,889 lines
by 4,587 samples.
PROCEDURES
The sections that
follow describe the data processing flow that was used at
the EDC to
create a composite data set. All image
processing was conducted
using Land Analysis System (Ailts and others,
1990) software.
Scene Selection
Cloud-free AVHRR observations
of the land surface are necessary for monitoring
the vegetation
conditions. A single AVHRR overpass is
seldom completely cloud
free.
Holben (1986) showed that compositing AVHRR data acquired over
several
days produces spatially continuous cloud-free images over large
areas with
sufficient temporal resolution to study green vegetation
dynamics. The
duration of
consecutive daily observations is called the compositing period.
On a
daily basis during a composite period, each observation of NOAA-11 data
over
the conterminous United States was evaluated for cloud cover. Typically,
there are two satellite
overpasses per day, one over the eastern portion of
North America and a
second pass over the western part of the continent. Every
image that provided a clear observation of a large
ground surface area at
reasonable nadir viewing angles is included in the
composite. On an average,
18 daily
observations per biweekly period are included in the composite.
Satellite
and Solar Viewing Geometry
The availability of the viewing geometry
information allows studies on the
effects of off-nadir viewing and the
investigation of potential data
correction techniques. The solar zenith angle is used during the
calibration
process to correct the solar illumination variability along an
orbit.
The computation of the solar and satellite geometry is a
process that derives
the satellite zenith, solar zenith, and relative
azimuth angle for each image
pixel.
The relative azimuth is the absolute difference between the
satellite
and solar azimuth angles.
The computed angles do not exceed 180 degrees. A
separate image band is created for each of these three
angle computations.
The
satellite zenith angle is computed in degrees, in which nadir is
represented
as 90 degrees. Therefore, values less
than 90 degrees represent
view angles in the backscattered (easterly)
direction and values greater than
90 represent the forward scatter
(westerly) direction. Note that
the
effective field of view of the satellite is approximately 55 degrees
each side
of nadir, but computed satellite zenith angles can exceed 55
degrees because
of the curvature of the Earth.
The relative
azimuth angle is computed as the absolute difference between the
solar
azimuth and the satellite azimuth angles.
The computed values are in
the 0 - 180 range. The relative azimuth angle is computed
instead of separate
azimuth angles because only the absolute difference
between the azimuth angles
is required for atmospheric correction
algorithms. Also, saving only the
computed
relative azimuth angle requires only one band in a daily observation
and
composite image instead of two, which reduces the image storage
requirements
on CD-ROM.
Radiometric
Calibration
Radiometric calibration of the AVHRR visible and near-infrared
channels
(channels 1 and 2) is an important consideration because there is
poor
preflight calibration, no onboard calibration, and difficulty with
inflight
calibration. Preflight
calibration coefficients can change while the
instrument is in storage, or
after launch, because of the space environment.
Degradation of AVHRR
sensors after launch has been well documented (Rao, 1987;
Price, 1987;
Holben and others, 1990). Several
studies have used stable sites
such as homogeneous desert targets to
monitor the degradation of the sensors
after the satellite had been
launched. Corrections are made for
sensor
degradation by using coefficients developed from a study by Teillet
and Holben
(1992) [unpublished report].
Their calculation takes into account the desert
calibration
approach (Holben and others, 1990) to develop a set of
time-dependent
calibration coefficients for the AVHRR sensor on NOAA-11. The
time-dependent coefficients are
based on a piecewise linear fit of the desert
results. Piecewise linear fits are recommended for
operational use because,
unlike polynomial fits, they will not change
retroactively when new data are
added to the end of the time series.
In addition to radiometric
calibration, the solar illumination variability,
which occurs in the
north/south direction within an orbit, was corrected using
the cosine of
the solar zenith angle. The calibration
and solar illumination
correction of channels 1 and 2 was completed using
the following formula:
R = (d*d/z)*kb(c-C)
where:
R is reflectance,
d is the mean earth-sun distance in astronomical
units,
z is the cosine
of the solar zenith angle,
k is the mean solar flux,
b is the gain coefficient,
c is the digital count, and
C is the deep space digital
counts.
Reflectance values for channels 1 and 2 were converted to
byte data, where the
range 0 - 254 represents 0 to 63.5 percent
reflectance (0.25 percent per bin)
and the value 255 is a grouping of
reflectance values greater than 63.5
percent. Any feature with greater than 63 percent reflectance is a
cloud,
snow, or other bright nonvegetated surface.
The
calibration coefficients for AVHRR thermal channels 3, 4, and 5 are
derived
onboard the satellite using a view of a stable blackbody and deep
space as
a reference (Kidwell, 1991). The
calibration process converts raw
data values to energy
(milliwatts/m2-steradian-cm-1) using the following
formula:
E=a+bc
where:
E is energy,
a is the intercept,
b is the gain coefficient,
and
c is the digital
count.
Energy is converted to brightness temperature using the
inverse of Planck's
radiation function.
The brightness temperatures are represented in Kelvin
units. A scaling factor was used to convert the
brightness temperatures to
byte data.
A scaling factor of 202.5 is subtracted from the brightness
temperature
value and the difference is multiplied by 2 to maintain one half
percent
accuracy (i.e., a brightness temperature of 280 becomes 155).
Normalized Difference Vegetation
Index (NDVI)
The NDVI is the difference of near-infrared (channel 2) and
visible
(channel 1) reflectance values normalized over the sum of channels
1 and 2
(NIR-VIS)/(NIR+VIS). The
NDVI equation produces values in the range of -1.0
to 1.0, where
increasing positive values indicate increasing green vegetation
and
negative values indicate nonvegetated surface features such as water,
barren,
ice, snow, or clouds. The NDVI can be
derived at several points in
the processing flow. To retain the most precision, the NDVI is
derived after
calibration of channels 1 and 2, prior to scaling to byte
range. Computation
of the NDVI
must precede geometric registration and resampling to maintain
precision
in this calculation.
To
scale the computed NDVI results to byte data range, the NDVI computed
value,
which ranges from -1.0 to 1.0, is scaled to the range of 0 to 200,
where
computed -1.0 equals 0, computed 0 equals 100, and computed 1.0 equals
200. As a result, NDVI values less than 100 now
represent clouds, snow,
water, and other nonvegetative surfaces and values
equal to or greater than
100 represent vegetative surfaces.
Date of Acquisition
The
date of acquisition images are provided to allow a user to identify the
specific
daily observation used for each pixel.
The date images for each
composite identify each daily image as a
unique value. The unique value is
linked
to an inventory of the daily observations.
A complete list of daily
observations used in each composite period
is on this CD-ROM under the \GEOM
directory in file DATE.ATT.
Geometric
Registration
The process of compositing daily observations for each
biweekly period
required each daily overpass to be registered to a common
map projection to
ensure that, from day to day, each 1-km pixel
represented the same ground
location.
The map projection chosen for the data is the Lambert Azimuthal
Equal
Area. This projection is appropriate
for the North American Continent
because of its visual presentation and
equal area characteristic, which allows
easy measurement of area
throughout the data set.
To perform the image-to-image registration
of the data a base image was
developed as a reference. Tests have shown that the best way to
prepare the
base image is to register individual daily orbits to an
accurate base map.
The map base used is the hydrography layer of the U.S.
Geological Survey
1:2,000,000-scale digital line graph (DLG). The features in the DLG data,
such as
water bodies, rivers, and streams, are identifiable features in the
AVHRR
1-km data. The DLG data are rasterized
to 1-km cells and registered to
the Lambert Azimuthal Equal Area
projection before being used as the map base
for the data.
Approximately 20 near-nadir
cloud-free segments of NOAA-11 channel 2 daily
observations from the 1989
and 1990 growing season are manually registered to
the DLG data. Each segment is verified for accuracy
(root-mean-square error
less than 1 pixel). The segments are digitally mosaicked to produce a single
base
image of the conterminous United States for registering the 1994 growing
season
data. The accuracy of this base image
is verified with a
root-mean-square error less than 1 pixel. Table 1 provides details on
projection
parameters.
Table 1. Lambert Azimuthal Equal Area (LAZEA) projection
_______________________________________________________________
Parameters:
Radius of sphere 6,370,997.0 meters
Longitude of central meridian
100 00 00 West
Latitude
of origin 45 00 00
North
False easting 0
False northing
0
Units of measure meters
Pixel size 1,000 meters
For the conterminous United
States (1994)
Center of pixel
(1,1) ( -2050000, 752000 )
Number of lines
2,889
Number of
samples 4,587
LAZEA minimum bounding rectangle:
In projection meters:
Lower left ( -2050500, -2136500 )
Upper left ( -2050500,
752500 )
Upper
right ( 2536500,
752500 )
Lower
right ( 2536500, -2136500 )
In decimal degrees of longitude and
latitude:
Lower left ( -119.9722899
23.5837576 )
Upper left ( -128.5300591
48.4030555 )
Upper
right ( -65.3946489
46.7048989 )
Lower
right ( -75.4163527
22.4793919 )
In degrees, minutes, and seconds of longitude and latitude:
Lower left ( -119 58 20
23 35 02 )
Upper
left ( -128 31
48 48 24 11 )
Upper right ( -65 23 41
46 42 18 )
Lower
right ( -75 24 59 22 28 46 )
________________________________________________________________
Each daily observation for the 1994 growing season is registered to
the base
image using image-to-image correlation. To improve overall registration
accuracy, 150 samples are
eliminated from each edge of the raw data image.
The 150 samples
represent the most extreme off-nadir pixels and are often the
source of
error in the image correlation process.
Then, the channel 2 data
for each daily observation are transformed
using the satellite orbit model.
Next, correlation of the original image
to the reference image is performed
using a set of 255 selected ground
control points. If most of the
ground
control points are cloud covered in the daily observation, no
correlation is
defined and the image is rejected. Otherwise, the correlation is
determined
and the satellite transformation coefficients from the orbital
model are
revised. Then the raw
data (channels 1 - 5), NDVI, and satellite geometry
data are transformed
using the revised coefficients and nearest neighbor
resampling.
Compositing
The method for
determining the portion of each overpass to be included in the
composite
image was to retain pixels having the highest NDVI values. The NDVI
was examined pixel by pixel
for each overpass within the biweekly compositing
period to determine the
maximum value.
The retention of the highest NDVI value reduces the
number of
cloud-contaminated pixels because values for clouds and cloud
shadows are
generally less than 100 (in the byte-scaled data) and clear
day observations
of vegetated surfaces are equal to or greater than 100
(in the byte-scaled
data). The
result is a near cloud-free image that depicts the maximum
vegetative
greenness for the compositing period.
The product of the compositing
process was a 10-band image that included the
maximum NDVI value for each
pixel during the composite period, the channels
1-5 and satellite viewing
geometry data from the chosen daily observations,
and a pointer value that
identified the satellite overpass from which that
pixel was taken. Table 2 lists the data included in each of
the 10 bands.
Table 2. Band description of composite images
__________________________________________________________________
Band
Description | Band
Description
__________________________________________________________________
1
AVHRR channel 1 | 6
NDVI
2 AVHRR channel 2 |
7 Satellite zenith
3
AVHRR channel 3 | 8
Solar zenith
4 AVHRR channel 4 |
9 Relative azimuth
5
AVHRR channel 5 | 10
Date
__________________________________________________________________
The
date of acquisition pointer is provided to allow a user to identify the
specific
AVHRR daily observation (satellite scene number) used for each pixel.
To
determine the date and scene number, first identify the date pointer
value
for the pixel within a composite period, then use the reference
table in file
DATE.ATT to determine the scene number.
Miscellaneous Data
When
displaying large areas with AVHRR data, an overlay or mask of familiar
linework,
such as county boundaries, can be used as a location aid. Several
images are included in the
\MISC directory to provide location information.
All of the linework
images represent lines in raster format as 1-km cells.
These data sets
include climatic division boundaries (CDLINES), major land
resource areas
boundaries (LRALINES), county boundaries (CTYLINES), and water
bodies
(WATERMSK). The climatic division lines
were digitized from NOAA base
maps.
The county lines are a modified version of the 1:2,000,000-scale
DLG
data. The major land resource
area boundaries were digitized from the U.S.
Department of Agriculture,
Soil Conservation Service (1981) maps.
The linework in the CDLINES
and LRALINES images is coded at the byte value
255. In the CTYLINES image, the county boundaries
identified by the coasts
and international borders are at value 253, the
county borders that are
coincident with State borders are at value 254,
and other county boundaries
are at value 255. This variable coding provides the capability to display
coastal,
State, or county boundaries from the same image. The water bodies
image has two unique identifiers. Water has a 0 value and land has a
value
of 1.
Also
included are three raster polygon images that can be used in an overlay
process
where histograms or descriptive statistics could be computed for the
NDVI
values within a polygon. These images
include counties (CTYPOLY), major
land resource areas (LRAPOLY), and
climatic divisions (CDPOLY).
Each
polygon is in raster format and has a unique numeric identifier. Images
that include more than 256
unique polygons are stored in I*2 integer (16 bit)
format.
The attribute information that
identifies or characterizes each polygon is
included under the \MISC
directory. The attributes for the major
land
resource area polygons are in LRAPOLY.ATT. The fields in the file are
polyid -- the unique polygon identification number
mlra -- the major land resource area
(MLRA) identification code used by
the Soil Conservation Service
lratext -- text description of the MLRA
used by the Soil Conservation
Service
The unique polygon identification
number for the climatic division polygons
can be parsed into the State and
climatic division number within that State.
For example, climatic
district one in Arizona is polygon number 401.
The 4 is
the Federal Information Processing Standard (FIPS) State
identification number
for Arizona, and the 01 identifies the polygon as
division one. Climatic
district
one in Oklahoma is polygon number 4001, where 40 is the FIPS State
code
and 01 is division one.
The attributes for the county polygons
are in CTYPOLY.ATT. The fields in
the
file are
cntyid
-- the unique polygon identification number
npixels -- the number of pixels in each county
FIPS -- the FIPS State and county code
for each county
cname -- the
county name
sname -- the
State name
One of the standard products calculated from the
conterminous U.S. AVHRR data
set is a statistical summary of the NDVI, by
county, for each composite
period.
The statistical summaries for all 1994 compositing periods are
available
on each of the discs. The statistical
summary can be imported to a
spreadsheet and a graph can be created to
show seasonal NDVI profiles. The
statistical
summary is linked to the CTYPOLY image by the key attribute CNTYID
that is
included in the CTYPOLY.ATT. This
summary can be merged with the
CTYPOLY image for representation in image
form.
The statistical summary for each composite period is stored in
separate tables
with a standard naming convention (CNTYP01.DAT is the table
for period 1,
CNTYP02.DAT for period 2, and so on). These tables are 80-character ASCII
files
with the following attributes and format:
___________________________________________________________________________
Col #
Fortran stmt. Description Definition
___________________________________________________________________________
1- 4 i4
CNTYID Unique identifier
for
each county polygon
5-10 1x,i5
FIPS FIPS code
11-18
1x,f7.2 MEAN Mean NDVI (with clouds,
water, negative NDVI not
counted)
19-22
1x,i3 %USED The portion of all pixels
in county which are counted.
23-30 1x,f7.3 SD Standard deviation
31-34 1x,i3 MIN
Minimum value in county
35-38 1x,i3 MAX Maximum value in county
39-46
1x,f7.2 MEDIAN Median value
47-50
1x,i3 MODE Mode value
51-54
1x,i3 PERIOD # Composite period number
___________________________________________________________________________
The
NDVI statistics are calculated for each county after clouded pixels,
water
bodies, and negative NDVI values (the 0 - 100 range of the scaled
NDVI) are
masked out. The cloud
screening is done independently (and is not applied to
image data on the
CD-ROM) by using a threshold value of 240 for the sum of
channels 1 and 2
(values greater than 240 are considered clouds). The cloud-
screening technique includes an added indicator,
the attribute %USED. The
attribute
%USED represents the proportion of the pixels in a county (excluding
water
bodies) that were counted in the computation.
A low value in this
attribute can indicate cloud
contamination.
Added to the miscellaneous image file was the surface
water bodies mask.
These water bodies were separated using channel 2 from
daily AVHRR scenes.
Cloud-free scenes were selected through a visual
quality assessment of the
images.
After a threshold between land and water values was identified, a
binary
mask was computed and the water bodies data was added to a land
characteristic
data base. Approximately 50 AVHRR
scenes were used to create
the mask.
Unique numeric identifiers were used in the raster formatted
polygons
- water has the value of 0 and land has the value of 1.
Table
3. A list of miscellaneous image file
characteristics
__________________________________________________________
Name Type
Bands Lines Samples
__________________________________________________________
LRAPOLY I*2 1 2,889
4,587
LRALINES Byte 1 2,889
4,587
CDPOLY I*2 1 2,889 4,587
CDLINES Byte
1 2,889 4,587
CTYPOLY I*2 1 2,889 4,587
CTYLINES Byte 1 2,889 4,587
WATERMSK
Byte 1 2,889
4,587
__________________________________________________________
CD-ROM
ORGANIZATION
A large volume of data was generated during the
construction of this data
base.
The data stored on each CD-ROM required ten 6,250-bpi magnetic tapes.
The data are organized in a directory structure that logically separates
the
data components. This
structure is:
README.1ST
\AVHRR
README \LABELS \IMAGES
\NDVI
README
\LABELS \IMAGES
\GEOM
README
\LABELS \IMAGES
\MISC
README
\LABELS \IMAGES \STATS
\DEMO
README
\SOFTWARE
README
Each directory on
the disc contains data that are similar in type. Each
directory also contains an ASCII text file (README)
that details the contents
of the directory.
The data files and LAS header files (files with name
extensions .DDR) are in
the \IMAGES subdirectories, and the image label
files are in the \LABELS
subdirectories.
To get a quick start looking at the image files, label files
for
each image are included in the \LABELS directory using the same file name
as
the image file it describes in the \IMAGES subdirectory. These label files
were designed for use
by the public domain MS-DOS personal computer IMDISP
image display
software developed by NASA's Jet Propulsion Laboratory in
Pasadena,
California. IMDISP users can access the
images on this CD-ROM by
selecting the image name in the \LABELS
subdirectory, which automatically
accesses the header information required
by the software to retrieve the image
data. The data dimensions of each band are 2,889 lines and 4,587
samples (13
megabytes).
The \AVHRR directory contains the five
channels of AVHRR data associated with
the four biweekly composites on
each CD-ROM. Each band of each biweekly
composite
file is uniquely named using the convention
P01CH1.IMG
where P01 identifies composite period 1
and CH1 identifies the image as
channel 1. The daily observations on the sixth disc are named using the
same
convention, with D01 referring to the first daily observation. The image
files are stored in the
\IMAGES subdirectory.
The
\NDVI directory contains the single band computed NDVI for the biweekly
AVHRR
composite data sets and is named using the convention:
P01NDVI.IMG
where P01
identifies composite period 1 and NDVI identifies the image as a
vegetation
index image. The image files are stored
in the \IMAGES
subdirectory.
The \GEOM directory contains the
satellite and solar zenith and relative
azimuth information for each pixel
in the AVHRR composite images.
This
directory also contains the date images for each of the
composites, as well as
the DATE.ATT attribute file.
The \MISC
directory contains the political (CTYLINES, CTYPOLY), climatic
divisions
(CDLINES, CDPOLY), and land resource area (LRALINES, LRAPOLY) raster
line
and polygon images, which are useful for display or in digital analysis
procedures. Attribute files related to these are
included as files
CTYPOLY.ATT and LRAPOLY.ATT. Each MISC directory also has a subdirectory,
STATS, which
contains the NDVI statistics of all counties for each composite
period.
The
\DEMO directory contains a batch job that runs under DOS and uses the
display
program, IMDISP. This program displays
images from the 1990
Conterminous U.S.
AVHRR Biweekly Composites set.
The display files are
compressed samples of these images. To initiate the demo program, enter
"DEMO"
at the DOS prompt.
The
\SOFTWARE directory contains programs to allow the PC-DOS user to display
and
interact with the digital images on the CD's.
These public domain
programs include
IMDISP -
An image display program developed by NASA's Jet Propulsion
Laboratory. The most recent version is included on this
disc. See
the IMDISP documentation file
IMDISP.DOC, located in the \SOFTWARE
directory, and use the IMDISP help command for further
details.
CONVERT - A conversion program included with IMDISP
that allows the
conversion of a raster image to integer, byte, nibble, or binary
format.
COPIM -
A copy program that allows copying all or portions of a raster
image and puts IMDISP compatible
label records at the front of the
image.
COMBINE - A utility for combining
two or more images as a single new image.
This utility has options to:
1. Combine up to three separate
images into a single new
black-and-white image and also create a customized color
palette of up to 255 colors that,
along with the new combined
image, allows a color simulation of a 3-band false color
composite image suitable for
display on an 8-bit PC color
monitor; these colors are a very close approximation of how the
image would appear on a 24-bit color display.
2. Automatically "stretch"
or brighten an existing palette.
3. Embed one image (such as raster linework) within
a second image.
The resultant images and palettes created by the
COMBINE
utility are
compatible with the IMDISP display program.
It takes approximately 4 minutes to process a 512
lines
by 512 samples,
3-image false color composite when the
input and output images are on hard disk. To run this
utility type COMBINE and respond to the prompts
requesting the input image names,
output image name, and
output palette name.
LL2LAM
- Converts latitude and
longitude coordinates to Lambert Azimuthal
Equal Area projection coordinates.
LAM2LL -
Converts Lambert Azimuthal Equal Area projection coordinates to
latitude and longitude
coordinates.
LL2LS -
Converts latitude and longitude to line and sample coordinates in
the Conterminous U.S.
AVHRR data set. This data set is
in the
Lambert
Azimuthal Equal Area projection.
LS2LL - Converts line and sample coordinates in
the Conterminous U.S.
AVHRR data set to latitude and longitude.
There are no restrictions on
making copies of IMDISP or any of the other
public domain programs for use
on other PC's or with other raster images.
* NOTE: Prior to displaying any of the following
images with IMDISP, the
command "SET SWAP" must be run to reset the display for
16-bit
integer data. This command must be run after the image has
been
selected with the
IMDISP "FILES" command.
CTYPOLY.LBL - County polygon data
CDPOLY.LBL - Climatic polygon data
LRAPOLY.LBL - LRA polygon data
DEM.LBL - Digital elevation data
For more information
please contact Customer Services, EROS Data Center, U.S.
Geological
Survey, Sioux Falls, SD 57198, (605)594-6151, FAX (605)594-6589.
REFERENCES
Ailts, B.,
Akkerman, D., Quirk, B., and Steinwand, D., 1990, LAS 5.0 -- an
image processing system for research and
production environments:
American Society for Photogrammetry and Remote Sensing-American
Congress
on Surveying and
Mapping Annual Convention, Denver, Colorado,
March 18-23, 1990, Proceedings, v. 4, p. 1-12.
Eidenshink,
J.C., 1992, The 1990 conterminous U.S. AVHRR data set:
Photogrammetric Engineering and Remote Sensing, vol. 58, no.
6,
pp. 809-813.
Holben,
B.N., 1986, Characteristics of maximum-value composite images from
temporal AVHRR data: The International
Journal of Remote Sensing, v. 7,
no. 11, p. 1417.
Holben, B.N., Kaufman, Y.J., and Kendall,
J.D., 1990, NOAA-11 AVHRR visible
and near-IR inflight calibration: The International Journal of
Remote
Sensing, v. 11, no. 8,
p. 1511.
Kidwell, K.B., 1991, NOAA Polar Orbiter Data Users' Guide:
National Oceanic
and
Atmospheric Administration, World Weather Building, Room 100,
Washington, D.C.
Price, John
C., 1987, Calibration of satellite radiometers and the comparison
of vegetation indices: Remote Sensing of the Environment, v. 21,
no.
15, pp. 15-27.
Rao,
Nagaraja C. R., 1987, Pre-launch calibration of channels 1 and 2 of
Advanced Very High Resolution
Radiometer: NOAA Technical Report
NESDIS
36, Satellite Research
Laboratory, National Environmental Satellite,
Data, and Information Service, Washington, D.C., 62 p.
Teillet,
P.M. and Holben, B.N., 1994, Towards operational radiometric
calibration of NOAA-AVHRR imagery in the
visible and infrared channels:
Canadian Journal of Remote Sensing, v.20, no.1, pp 1-10.
U.S.
Department of Agriculture, Soil Conservation Service, 1981, Land resource
regions and major land resource areas of
the United States: Agricultural
Handbook 296, 156 p.
Acknowledgments
A number of individuals contributed to the
successful completion of the AVHRR
Conterminous U.S. composite data,
including various operations staff and
digital data production scientists. Jesslyn F. Brown and Richard A.
McKinney
provided excellent technical reviews.
Jeffery C. Eidenshink
Mary C.
Weinheimer
Michael E. Madigan
##############################################################
VIII.
APPENDIX II - Pixel Date Attribute Table
PERIOD INDEX
SCENEID Date GMT
------ -----
---------------- ------- --------
01 1 ah11010794231507 01-07-94 23:15:07
2 ah11010894230229
01-08-94 23:02:29
3 ah11010894212135
01-08-94 21:21:35
4 ah11010994224953
01-09-94 22:49:53
5 ah11011094223733
01-10-94 22:37:33
6 ah11011194222500
01-11-94 22:25:00
7 ah11011294235637
01-12-94 23:56:37
8 ah11011394234339
01-13-94 23:43:39
9 ah11010994210941
01-09-94 21:09:41
10 ah11011494233043
01-14-94 23:30:43
11 ah11011494214810
01-14-94 21:48:10
12 ah11011594213612
01-15-94 21:36:12
13 ah11011794225305
01-17-94 22:53:05
14 ah11011894224013
01-18-94 22:40:13
15 ah11011994204833
01-19-94 20:48:33
16 ah11012094235935
01-20-94 23:59:35
02
101 ah11021194224810 02-11-94
22:48:10
102 ah11021294223535 02-12-94 22:35:35
103 ah11021394222316
02-13-94 22:23:16
104 ah11021494235434 02-14-94 23:54:34
105
ah11021594215844 02-15-94 21:58:44
106
ah11021694214645 02-16-94 21:46:45
107
ah11021994211040 02-19-94 21:10:40
108
ah11022294203519 02-22-94 20:35:19
109 ah11022394234414 02-23-94
23:44:14
110 ah11022494233128 02-24-94 23:31:28
03
1 ah11030494233407 03-04-94
23:34:07
2 ah11030494215153 03-04-94 21:51:53
3 ah11030594232112
03-05-94 23:21:12
4 ah11030594213939 03-05-94
21:39:39
5 ah11030694230834 03-06-94 23:08:34
7 ah11030794225556
03-07-94 22:55:56
8 ah11030994223100
03-09-94 22:31:00
9 ah11031094221842
03-10-94 22:18:42
101 ah11031194234937
03-11-94 23:49:37
102 ah11031194220625
03-11-94 22:06:25
103 ah11031294233640
03-12-94 23:36:40
104 ah11031294215425
03-12-94 21:54:25
105 ah11031394232345 03-13-94 23:23:45
106
ah11031494231106 03-14-94 23:11:06
107
ah11031594225828 03-15-94 22:58:28
108
ah11031694210621 03-16-94 21:06:21
109
ah11031494213013 03-14-94 21:30:13
110 ah11031594211816 03-15-94
21:18:16
111 ah11031694224606 03-16-94 22:46:06
112 ah11031794223332
03-17-94 22:33:32
04
1 ah11031894222113 03-18-94
22:21:13
3 ah11031994235210 03-19-94 23:52:10
4
ah11032194214441 03-21-94 21:44:41
5
ah11032194232527 03-21-94 23:25:27
6
ah11032094233912 03-20-94 23:39:12
7
ah11032294213321 03-22-94 21:33:21
8
ah11032294231416 03-22-94 23:14:16
9
ah11032394212126 03-23-94 21:21:26
10
ah11032494224919 03-24-94 22:49:19
101
ah11032794235527 03-27-94 23:55:27
102
ah11032894234231 03-28-94 23:42:31
103
ah11032994232951 03-29-94 23:29:51
104
ah11032994214758 03-29-94 21:47:58
105
ah11033094213600 03-30-94 21:36:00
106
ah11033094231657 03-30-94 23:16:57
107
ah11033194212405 03-31-94 21:24:05
108 ah11033194230420 03-31-94
23:04:20
5 1
ah11040194211211 04-01-94 21:12:11
3
ah11040294210018 04-02-94 21:00:18
4
ah11040394222707 04-03-94 22:27:07
5
ah11040494235823 04-04-94 23:58:23
6 ah11040494221451 04-04-94 22:14:51
7 ah11040594234527
04-05-94 23:45:27
9 ah11040694233232
04-06-94 23:32:32
10 ah11040794213840
04-07-94 21:38:40
101 ah11040894212629
04-08-94 21:26:29
102 ah11040994225440
04-09-94 22:54:40
103 ah11041094224206
04-10-94 22:42:06
104 ah11041194222948
04-11-94 22:29:48
105 ah11041394234808
04-13-94 23:48:08
106 ah11041394220516
04-13-94 22:05:16
107 ah11041494233513
04-14-94 23:35:13
108 ah11041494215317
04-14-94 21:53:17
6
1 ah11041594232234 04-15-94
23:22:34
2 ah11041694230957 04-16-94 23:09:57
3 ah11041794225721
04-17-94 22:57:21
5 ah11041894224447
04-18-94 22:44:47
6 ah11041894210521
04-18-94 21:05:21
7 ah11041994223109
04-19-94 22:31:09
8 ah11042094001524
04-20-94 00:15:24
10
ah11042194220634 04-21-94 22:06:34
11
ah11042194234925 04-21-94 23:49:25
12
ah11042094221851 04-20-94 22:18:51
101
ah11042294215434 04-22-94 21:54:34
102
ah11042394214235 04-23-94 21:42:35
103
ah11042494213022 04-24-94 21:30:22
105
ah11042594225831 04-25-94 22:58:31
106
ah11042594211826 04-25-94 21:18:26
107
ah11042694224556 04-26-94 22:45:56
108
ah11042694210647 04-26-94 21:06:47
110
al11042994000224 04-29-94 00:02:24
7 1 ah11042994235154 04-29-94 23:51:54
2 ah11042994220901
04-29-94 22:09:01
3 ah11043094233857
04-30-94 23:38:57
4 ah11050194232616
05-01-94 23:26:16
5 ah11050294213249
05-02-94 21:32:49
6 ah11050294231337
05-02-94 23:13:37
8 ah11050494224823
05-04-94 22:48:23
10 ah11050594223603
05-05-94 22:36:03
11
ah11050694002035 05-06-94 00:20:35
101
ah11050994232843 05-09-94 23:28:43
102
ah11050994214712 05-09-94 21:47:12
104
ah11050794221127 05-07-94 22:11:27
105
ah11050794235421 05-07-94 23:54:21
107
ah11050894234124 05-08-94 23:41:24
108
ah11051094213514 05-10-94 21:35:14
109
ah11051094231603 05-10-94 23:16:03
110
ah11051194212317 05-11-94 21:23:17
111
ah11051194230325 05-11-94 23:03:25
112
ah11051294211122 05-12-94 21:11:22
8 1 ah11051394205944 05-13-94 20:59:44
2 ah11051494204752
05-14-94 20:47:52
3 ah11051494222712
05-14-94 22:27:12
4
ah11051594221352 05-15-94
22:13:52
5 ah11051594235647 05-15-94 23:56:47
6 ah11051694220152
05-16-94 22:01:52
7 ah11051694234350
05-16-94 23:43:50
8 ah11051794214936
05-17-94 21:49:36
9 ah11051794233108 05-17-94
23:31:08
10 ah11051994212541 05-19-94 21:25:41
102 ah11052094225313
05-20-94 22:53:13
103 ah11052194210152
05-21-94 21:01:52
104 ah11052194224053 05-21-94 22:40:53
106
ah11052294222834 05-22-94 22:28:34
107
ah11052394001236 05-23-94 00:12:36
108
ah11052394221616 05-23-94 22:16:16
109
ah11052494220414 05-24-94 22:04:14
110 ah11052294002551 05-22-94
00:25:51
111 ah11052594215159 05-25-94 21:51:59
112 ah11052594233331
05-25-94 23:33:31
113 ah11052694214000
05-26-94 21:40:00
114 ah11052694232051
05-26-94 23:20:51
9
1 ah11052794212803 05-27-94
21:28:03
2 ah11052794230813 05-27-94 23:08:13
3 ah11052894211607
05-28-94 21:16:07
4 ah11052894225535
05-28-94 22:55:35
5 ah11052994210413
05-29-94 21:04:13
6 ah11052994224315
05-29-94 22:43:15
7 ah11053094002813
05-30-94 00:28:13
8 ah11053094205235
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#################### END
DOC SECTION #########################
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