Sevilleta
National Wildlife Refuge, near Albuquerque, New Mexico
\log
12/03/97
- Date this file created. G. Shore.
12/20/97 - Updated documentation. 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 (1993)
##############################################################
ABSTRACT
This dataset contains 21 separate 14-day
composited AVHRR
images for 1993 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 1993
##############################################################
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
Twenty-one 14-day composites for 1993.
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 21
NULL bytes onto the last line of each band, 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
93
NOTE: this
generates 10-band ERDAS Imagine format files, that are of
image size 2889 rows x 4587
cols, with filenames as follows:
avhrr93pPP.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->avhrr93pPP.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 avhrr93pPP.img
avhrr93pPPnm.img
NOTE: this generates 10-band ERDAS Imagine format files, that are
of
image size 735
rows x 699 cols, with filenames as follows:
avhrr93pPPnm.img
5. Unix compress the NM clipped image, make
an archive directory, and move it
to the archive destination (/db/archive/imagery/avhrr/avhrr93pPP/).
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:
avhrr93pPPnm.img.Z
6.
Compress (gzip) and archive the full scene image to 4mm DAT tape, then
remove from online disk:
gzip avhrr93pPP.img
mt -f /dev/rmt/0cn fsf <#>
tar cvf /dev/rmt/0cn
avhrr93pPP.img.gz
rm avhrr93pPP.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 (avhrr93.dbf) for the images
(note, must also convert from DOS to Unix
file):
dos2unix
/cdrom/cdrom0/readme.1st avhrr93readme.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
(avhrr93pPPnm.mda), and merge by year for inclusion in SIMS IAF
metadata
file (avhrr93.dbf):
dos2unix /cdrom/cdrom0/geom/date.att
avhrr93pPP-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
93 > avhrr93date.att
9. Generate (this) SIMS IAF metadata file
(i.e., avhrr93.dbf) using template
file (avhrr_dbf.tmpl), appending readme file (avhrr93readme.1st), and
date
file
(avhrr93date.att).
10. Generate GIS/RS Metadata Abstract file for
each image, and put with
image
in appropriate directory (/db/archive/imagery/avhrr/avhrr93pPP/):
/db/local/imagery/bincom/get_avhrr_dates.csh 93 avhrr93.dbf 97 \
> avhrr93periods.txt
/db/local/imagery/bincom/batch_make_avhrr_abstract.csh
avhrr93periods.txt
which calls:
/db/local/imagery/bincom/make_avhrr_abstract.csh
##############################################################
VII. APPENDIX I - USGS EDC Metadata
THE 1993 CONTERMINOUS U.S. AVHRR BIWEEKLY
COMPOSITES
TABLE OF CONTENTS
Page
Introduction . . . . . . . . . . . . . . . . . . . . . . . . .
. . . . . . . 1
Data Set Characteristics . . . . . . . . . . . . . .
. . . . . . . . . . . . 2
Procedures . . . . . . . . . . . . . . . .
. . . . . . . . . . . . . . . . . 4
Scene Selection . . . . . . . . . . . . . . . . . . . . . . . . . . . .
. 4
Satellite and Solar Viewing
Geometry. . . . . . . . . . . . . . . . . . . 5
Radiometric Calibration . . . . . . . . . . . . . . . . . . . .
. . . . . 6
Normalized
Difference Vegetation Index. . . . . . . . . . . . . . . . . . 9
Date of Acquisition . . . . . . . . . . . .
. . . . . . . . . . . . . . .10
Geometric Registration. . . . . . . . . . . . . . . . . . . . . . . . .
.10
Compositing . . . . . . . .
. . . . . . . . . . . . . . . . . . . . . . .13
Miscellaneous Data. . . . . . . . . . . . . . . . . . . . . . .
. . . . .15
CD-ROM Organization. . . . . . . . . . . . . . . . . . .
. . . . . . . . . .20
References . . . . . . . . . . . . . . . . . .
. . . . . . . . . . . . . . .26
THE 1993
CONTERMINOUS U.S. AVHRR BIWEEKLY COMPOSITES
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 twenty-one 14-day maximum NDVI composites,
created
from nearly 400 NOAA-11 images, and 3 single date images. The 17 core
composite periods represent
a continuous period from March 5, 1993, to October
28, 1993. The first two (periods 1 and 2) and last two
(periods 20 and 21)
composites represent a 2-week period each for January,
February, November, and
December.
The 1993 data set is available as a set of six CD-ROM's. Each of
the first five discs has four
biweekly composites and miscellaneous data that
are described later in
this file. The sixth disc of the 1993
CD-ROM series
contains the December 2-week composite, two daily
observation AVHRR scenes
depicting the Mississippi River region of the
United States. These observations
were chosen to represent the change that
occurred from the 1993 Mississippi
River flooding. One observation is of July 17, 1992 before
the flooding and
the other observation is of July 12, 1993 showing the
flooding. These two
daily
observations only have channels 1 and 2.
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 1993 were:
____________________________________________________
Period Date of coverage Julian day
____________________________________________________
1
01/08 - 01/21/1993 008
- 021
2 02/12 - 02/25/1993 043 - 056
3
03/05 - 03/18/1993 064
- 077
4 03/19 - 04/01/1993 078 - 091
5
04/02 - 04/15/1993 092
- 105
6 04/16 - 04/29/1993 106 - 119
7
04/30 - 05/13/1993 120
- 133
8 05/14 - 05/27/1993 134 - 147
9
05/28 - 06/10/1993 148
- 161
10 06/11 - 06/24/1993 162 - 175
11
06/25 - 07/08/1993 176
- 189
12 07/09 - 07/22/1993 190 - 203
13
07/23 - 08/05/1993 204
- 217
14 08/06 - 08/19/1993 218 - 231
15
08/20 - 09/02/1993 232
- 245
16 09/03 - 09/16/1993 246 - 259
17
09/17 - 09/30/1993 260
- 273
18 10/01 - 10/14/1993 274 - 287
19
10/15 - 10/28/1993 288
- 301
20 11/12 - 11/25/1993 316 - 329
21
12/10 - 12/23/1993 344
- 357
____________________________________________________
The image
dimensions of each band are 2,889 lines and 4,608 samples (13
megabytes).
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
(in press). 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 1993 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
(1993)
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 1993 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 1993
compositing periods are
available on the sixth disc. 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
4,608
LRALINES Byte 1 2,889
4,608
CDPOLY I*2 1 2,889 4,608
CDLINES Byte 1 2,889 4,608
CTYPOLY I*2 1 2,889 4,608
CTYLINES Byte 1 2,889 4,608
WATERMSK
Byte 1 2,889
4,608
__________________________________________________________
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
\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.
The binary image files were put on the CD-ROM with a 512-byte
header
record. This header record is used by
the LAS image processing system.
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 actual data
dimensions of each band are 2,889 lines and 4,587 samples (13
megabytes),
but the images are stored as 2,889 lines and 4,608 samples to
accommodate
LAS software. The last 21 samples of
each line are blank (zero)
to make each line a multiple of 512 as required
by the LAS, with the exception
of the last line. The images were generated on a UNIX-based system. On UNIX
systems, the portion of the
last block does not exist; therefore, lines
1-2,888 contain 4,608 samples
and line 2,889 has 4,587 samples. The
formula
to calculate the number of disc blocks for an image in a UNIX
environment is
#image_bytes_line
= #samps * #bytes_samp
#bytes_file_line = INT(((#image_bytes_line - 1) / 512) + 1) * 512
#bytes_file = (#lines * #bytes_file_line *
#nbands) -
(#bytes_file_line -
#image_bytes_line) + 512
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 sixth disc contains the December 2-week
composite
period P21NDVI and the three daily observations D01 - D03. 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), water bodies
(WATERMSK), 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.
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., in press, Towards operational radiometric
calibration of NOAA AVHRR imagery in the
visible and infrared channels:
Canadian Journal of Remote Sensing.
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
Michael E. Madigan
Mary C.
Weinheimer
##############################################################
VIII.
APPENDIX II - Pixel Date Attribute Table
PERIOD INDEX
SCENEID Date GMT
------ -----
---------------- ------- --------
1 1 ah11011093211530 01-10-93
21:15:30
2 ah11010993212737 01-09-93 21:27:37
3 ah11011193224549
01-11-93 22:45:49
4 ah11011293205140
01-12-93 20:51:40
5 ah11011293223324
01-12-93 22:33:24
6
ah11011593201607 01-15-93 20:16:07
7
ah11011593215603 01-15-93 21:56:03
8
ah11011693200424 01-16-93 20:04:24
9
ah11011693214353 01-16-93 21:43:53
10
ah11011793195242 01-17-93 19:52:42
11
ah11011793213130 01-17-93 21:31:30
12
ah11011893194116 01-18-93 19:41:16
13
ah11011993192937 01-19-93 19:29:37
14
ah11011993210718 01-19-93 21:07:18
15
ah11011993225000 01-19-93 22:50:00
16
ah11012093191829 01-20-93 19:18:29
17
ah11012093205529 01-20-93 20:55:29
18
ah11012093223715 01-20-93 22:37:15
19
ah11011093225835 01-10-93 22:58:35
20 ah11012193222446 01-21-93
22:24:46
2 1 ah11021793215909 02-17-93 21:59:09
2 ah11021893200731
02-18-93 20:07:31
3 ah11021893214700
02-18-93 21:47:00
4 ah11021993213436
02-19-93 21:34:36
5
ah11022093212229 02-20-93 21:22:29
6
ah11022393204632 02-23-93 20:46:32
7
ah11022493203445 02-24-93 20:34:45
8
ah11022193225305 02-21-93 22:53:05
9
ah11021293211842 02-12-93 21:18:42
10
ah11021393224901 02-13-93 22:49:01
11
ah11022493221524 02-24-93 22:15:24
12
ah11022593202300 02-25-93 20:23:00
13
ah11022593220258 02-25-93 22:02:58
3 2 ah11030693234025 03-06-93
23:40:25
3 ah11030593220645 03-05-93 22:06:45
4 ah11030693215435
03-06-93 21:54:35
5 ah11030693201501
03-06-93 20:15:01
6 ah11030793232649
03-07-93 23:26:49
7
ah11030793214226 03-07-93
21:42:26
8 ah11030793200318 03-07-93 20:03:18
9 ah11030893231346
03-08-93 23:13:46
10 ah11030893213003
03-08-93 21:30:03
12 ah11030993230058
03-09-93 23:00:58
13 ah11030993211757 03-09-93
21:17:57
14 ah11031093224813 03-10-93 22:48:13
15 ah11031093210608
03-10-93 21:06:08
16 ah11031193223528
03-11-93 22:35:28
17 ah11031193205404 03-11-93 20:54:04
101
ah11031293222300 03-12-93 22:23:00
102
ah11031293204217 03-12-93 20:42:17
103
ah11031393221048 03-13-93 22:10:48
104
ah11031493201831 03-14-93 20:18:31
105 ah11031493215823 03-14-93
21:58:23
106 ah11031593233054 03-15-93 23:30:54
107 ah11031593214613
03-15-93 21:46:13
108 ah11031593200703
03-15-93 20:07:03
109 ah11031693231750
03-16-93 23:17:50
110 ah11031693213350
03-16-93 21:33:50
111 ah11031693195521
03-16-93 19:55:21
112 ah11031793230447
03-17-93 23:04:47
113 ah11031793212143
03-17-93 21:21:43
114 ah11031893225201
03-18-93 22:52:01
115 ah11031893210954
03-18-93 21:09:54
116 ah11031893193217
03-18-93 19:32:17
4 1 ah11031993223932
03-19-93 22:39:32
2 ah11032093222703
03-20-93 22:27:03
3 ah11032193221436 03-21-93 22:14:36
4
ah11032293220210 03-22-93 22:02:10
5
ah11032393215001 03-23-93 21:50:01
6
ah11032493213737 03-24-93 21:37:37
7
ah11032493232140 03-24-93 23:21:40
8 ah11032593230852 03-25-93
23:08:52
9 ah11032593212530 03-25-93 21:25:30
10 ah11032093204548
03-20-93 20:45:48
11 ah11032193203401
03-21-93 20:34:01
12 ah11032293202217
03-22-93 20:22:17
101 ah11032693225605
03-26-93 22:56:05
102 ah11032693211326
03-26-93 21:13:26
103 ah11032793224320
03-27-93 22:43:20
104 ah11032793210136
03-27-93 21:01:36
105 ah11032893223052
03-28-93 22:30:52
106 ah11032693193601
03-26-93 19:36:01
107 ah11032993221824
03-29-93 22:18:24
108 ah11032993203747
03-29-93 20:37:47
109 ah11033093220558
03-30-93 22:05:58
110 ah11033093202602 03-30-93 20:26:02
111
ah11033193215348 03-31-93 21:53:48
112
ah11033193201418 03-31-93 20:14:18
113
ah11040193232544 04-01-93 23:25:44
114
ah11040193214125 04-01-93 21:41:25
115 ah11040193200236 04-01-93
20:02:36
5 1 ah11040293212917 04-02-93 21:29:17
3 ah11040393211712
04-03-93 21:17:12
4 ah11040493210523
04-04-93 21:05:23
5 ah11040493224709
04-04-93 22:47:09
6
ah11040593223305 04-05-93 22:33:05
7
ah11040593205132 04-05-93 20:51:32
11
ah11040893201604 04-08-93 20:16:04
13
ah11040793220802 04-07-93 22:08:02
14
ah11040793202752 04-07-93 20:27:52
101
ah11040993214320 04-09-93 21:43:20
102
ah11041093231503 04-10-93 23:15:03
103
ah11041093213108 04-10-93 21:31:08
104
ah11041193230156 04-11-93 23:01:56
105
ah11041193211858 04-11-93 21:18:58
106
ah11041293224920 04-12-93 22:49:20
107
ah11041293210704 04-12-93 21:07:04
108
ah11041393223632 04-13-93 22:36:32
109
ah11041393205457 04-13-93 20:54:57
110 ah11041493222359 04-14-93
22:23:59
111 ah11041493204306 04-14-93 20:43:06
112 ah11041593221128
04-15-93 22:11:28
6 1 ah11041693215858
04-16-93 21:58:58
3 ah11041793214645
04-17-93 21:46:45
4
ah11041893231829 04-18-93 23:18:29
5
ah11041893213432 04-18-93 21:34:32
6
ah11041893195609 04-18-93 19:56:09
7
ah11041993230536 04-19-93 23:05:36
8
ah11041993212221 04-19-93 21:22:21
9
ah11041993194440 04-19-93 19:44:40
10
ah11042093225247 04-20-93 22:52:47
11
ah11042193223958 04-21-93 22:39:58
12
ah11042093211014 04-20-93 21:10:14
13
ah11042193205821 04-21-93 20:58:21
14
ah11042293204629 04-22-93 20:46:29
102
ah11042493220238 04-24-93 22:02:38
104
ah11042593215010 04-25-93 21:50:10
107
ah11042793194749 04-27-93 19:47:49
108 ah11042793230904 04-27-93
23:09:04
109 ah11042793212547 04-27-93 21:25:47
110 ah11042893225613
04-28-93 22:56:13
111 ah11042893211337
04-28-93 21:13:37
112 ah11042993210144
04-29-93 21:01:44
113
ah11042993224338 04-29-93 22:43:38
114
ah11042693232211 04-26-93 23:22:11
115
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110
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113
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102
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115
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116
ah11121993220430 12-19-93 22:04:30
117
ah11122093233511 12-20-93 23:35:11
118
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21:40:17
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####################
END DOC SECTION #########################
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