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Long Term Acquisition Plan Files
The Long Term Acquisition Plan (LTAP) is used to direct the acquisition
by Landsat 7 of Worldwide Reference System (WRS) scenes around the
world for archiving in the U.S. EROS Data Center. The contents of
the following files represent the underpinnings of the LTAP:
- seasonality file - Formats available:
ASCII text file. (900 KB)
- WRS land data base, Rev. 3.0, October, 2002- Formats available:
Excel file.
(1.5
MB)
- nominal cloud cover file - Formats available: Word
text file. (5.7 MB)
- nominal cloud cover daylight additions file - Formats available:
Word
text file. (5.7 MB)
- nominal gain settings file - Formats available: ASCII
text file. (4.7 MB)
- maximum solar zenith angle
1. The seasonality
file specifies which WRS scenes are to be acquired during which
periods of time (request period), and the frequency of acquisition
during those periods. This file covers the year 2001 and includes
both daytime and nighttime imaging. Frequency of acquisition is
defined as either "once" during the request period, or
"all" opportunities during the request period. The results
of ingesting this file into the scheduler and developing the daily
schedule are posted daily on the web, at this
server location.
Here is the warning label associated with the seasonality file:
The scheduler has many resources and priorities that it juggles
during consideration of requests for scheduling, including:
- predicted cloud cover as compared to the nominal
- number of missed opportunities for this request since it was
opened
- how good the cloud cover assessment score was for the last
acquisition
- nearness to end of the request period
- availability of resources including duty cycle, onboard recorder
space, and station contact time
The result of this juggling is that scenes marked with an "all"
opportunities frequency are usually acquired every 4-5 cycles (64-80
days) instead of every cycle (16 days). Another outcome of this
is that scenes marked with a "once" frequency may be acquired multiple
times within the request period in an attempt to better the cloud
cover results, should the first acquisition's cloud cover be considerably
worse than the nominal. So please treat the frequency assignment
in the seasonality as a guide, not a rule.
The column headings for the seasonality file are:
- first date of request period (yyyy-mm-dd)
- last date of request period (yyyy-mm-dd)
- path/row (note that rows 246-248 will be sorted to the end of
the path)
- acquisition frequency (once, all)
- base priority of the request
- maximum solar zenith angle (only for night scenes, is set to
90)
2. The
WRS land data base identifies those WRS scenes containing land
or shallow water which will be imaged at least once every year.
At the end of the file are separate tables for the niche communities
and special interests. These include: EOS validation sites, glaciers,
MODIS fire validation sites, political (disputed sites), volcanoes,
global oceanic islands. A comprehensive reef list is a future addition.
3. and 4. The nominal
cloud cover file reports the average cloud cover for each WRS
scene for each month of the year. The file spans one year and addresses
the descending rows only.The
nominal cloud cover daylight additions file adds those ascending
rows which will be in daylight during some part of the year and
therefore may be imaged. The average cloud cover is derived from
the International Satellite Cloud Climatology Project D2 data set,
years 1989-1993. As subsequent years are processed, this file will
be updated.
The columns in the nominal cloud cover files are: first day of
month|last day of month|path|row|cloud cover value all cloud cover
values for row 1 across all paths are given, then for row 2, etc.
5. The nominal
gain settings file identifies the gain settings that will be
used as defaults for each WRS scene for each day of the year. This
file spans one year. The scheduler uses the DOY value. The DD-MMM
values that are included in the file are for a leap year and are
guidance for those who don't easily equate a DOY value of 177 with
the date 25-JUN. The file addresses both descending and ascending
rows of interest to the U.S. archive. The settings are given as
H for high gain or L for low gain. The order in which they are specified
for each scene is bands 123456678, where band 6 is repeated twice,
once for format 1 and once for format 2, and band 8 is the panchromatic
band. You will notice that bands 66 are constant at LH and band
8 is constant at L. The other bands are changed in groupings, with
bands 123 changed together, band 4 changed on its own merits, and
bands 57 changed together. When we do night imaging, we use the
following default settings: HHHHLLHLL. The file only contains
entries showing when the default gain setting has changed from its
previous setting. The default gain settings are generated using
rules that take land cover type and sun angle into account.
To understand these rules, read the file "gain
setting rules". Other files referenced by this document
are:
6. The maximum solar zenith angle is a single value for
all scenes at all times of the year. Daylight imaging will not be
scheduled if the angle is 85 degrees or more (same as 5 degrees
or less in elevation from the earth's surface).
Back to Chapter 5
Last Update: November 7, 2002
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