|
CHAPTER 11 SECTIONS > Level 0R Product | Level 1R Product | Level 1G Product | Level 1 Differences
11.3
Level 1G Product
The 1G product available to users from EROS is a radiometrically
and geometrically corrected Level 0R image.
The correction algorithms employed model the spacecraft and sensor using
data generated by onboard computers during imaging events. Primary inputs
are the PCD, which includes the attitude and ephemeris profiles, the definitive
ephemeris (if available) and the MSCD. Refined parameters from the
CPF, ground control points and a digital elevation model are also
used to improve the overall geometric fidelity of the standard level-one
terrain-corrected (L1T) product.
The L1T correction process utilizes both ground control points (GCP)
and digital elevation models (DEM) to attain absolute geodetic accuracy.
The WGS84 ellipsoid is employed as the Earth model for the Universal Transverse
Mercator (UTM) coordinate transformation. Associated with the UTM projection
is a unique set of projection parameters that flow
from the USGS General Cartographic Transformation Package. The
end result is a geometrically rectified product free from distortions
related to the sensor (e.g. jitter, view angle effects), satellite (e.g.
attitude deviations from nominal), and Earth (e.g. rotation, curvature,
relief).
Geodetic
accuracy of the L1T product depends on the accuracy of the GCPs
and the resolution of the DEM used*. The 2005 Global Land Survey is used
as the source for GCPs while the primary terrain data is the Shuttle
Radar Topographic Mission DEM. Scenes that have a quality
scores of 99 and less than 40 percent cloud cover are automatically processed,
and any archived scene, regardless of cloud cover, can be ordered through
one of two EROS web portals (Product
Ordering.)
| Table 11.1 Landsat 7 1G
Projection Parameters |
| |
Required Parameters |
| Projection Name |
1 |
2 |
3 |
4 |
5 |
6 |
7 |
8 |
9 |
10 |
11 |
12 |
13 |
| Universal Transvere Mercator (UTM) |
SMajor |
SMinor |
Zone |
|
|
|
|
|
|
|
|
|
|
| Lambert Conformal Conic |
SMajor |
SMinor |
STDPR1 |
STDPR2 |
CentMer |
OriginLat |
FE |
FN |
|
|
|
|
|
| Polyconic |
SMajor |
SMinor |
|
|
CentMer |
OriginLat |
FE |
FN |
|
|
|
|
|
| Transverse Mercator |
SMajor |
SMinor |
Factor |
|
CentMer |
OriginLat |
FE |
FN |
|
|
|
|
|
| Polar Stereographic |
SMajor |
SMinor |
|
|
LonPol |
TrueScale |
FE |
FN |
|
|
|
|
|
| Hotine Oblique Mercator A |
SMajor |
SMinor |
Factor |
|
|
OriginLat |
FE |
FN |
Long1 |
Lat1 |
Long2 |
Lat2 |
zero |
| Hotine Oblique Mercator B |
SMajor |
SMinor |
Factor |
AziAng |
AzmthPt |
OriginLat |
FE |
FN |
|
|
|
|
one |
| Space Oblique Mercator B |
SMajor |
SMinor |
Satnum |
Path |
|
|
FE |
FN |
|
|
|
|
one |
| Projection Parameter
Definitions |
| AziAng |
azimuth angle east of north for center projection line |
| AzmthPt |
longitude of point on central meridian where AziAng occurs.
|
| CentMer |
Longitude of the projection's central meridian |
| Factor |
scale factor at the central meridian (transverse mercator) or center of projection (Oblique Mercator)
|
| FE |
false easting in the same units as the semi-major axis |
| FN |
false northing in the same units as the semi-major axis |
| Lat1 |
latitude of first point on the projection's center line |
| Lat2 |
latitude of second point on the projection's center line |
| Long1 |
longitude of first point on the projection's center line |
| Long2 |
longitude of second point on the projection's center line |
| LongPol |
longitude down below pole of map |
| OriginLat |
latitude of the projection origin |
| Path |
path number for Landsat 7 using the World Reference System #2 |
| Satnum |
number of the Landsat satellite (i.e. 7) |
| SMajor |
semi-major axis of the projection's ellipsoid |
| SMinor |
semi-minor axis of the projection's ellipsoid |
| STDPR1 |
latitude of the first standard parallel |
| STDPR2 |
latitude of the second standard parallel |
| TrueScale |
latitude of the true scale |
The Landsat 7 level 1G product projection parameters are listed in Table 12.1. Most projections do not require 13 parameters as evidenced by the empty table cells. Parameter definitions are listed in Table 12.2.
During L1T processing the 0R image data undergoes two-dimensional resampling
according to the following set of parameters:
- Correction level - L1T*
- Pixel Size - 15, 30, 60 meters for panchromatic, VNIR/SWIR, and thermal
- Resampling kernel - Cubic
Convolution (CC)
- Map projection - UTM
with Polar Stereographic projection used for Antarctica scenes
- Ellipsoid - WGS84
- Image orientation
- north up
- Output format - GeoTIFF
- File transfer protocol (FTP) download only
* While most scenes are processed to L1T, some lack GCPs and/or
DEMs required for precision and terrain correction processing.
In these cases, the best level of correction will be applied -
Level 1GT-systematic terrain (GCPs absent) or Level 1G-systematic
(DEMs and GCPs absent). |
 Figure 11.3 - Landsat 7 Resampling Kernel (CC) Versus Other Methods
The Landsat 7 level 1G product projection parameters are listed in Table 12.1. Most projections do not require 13 parameters as evidenced by the empty table cells. Parameter definitions are listed in Table 12.2.
During 1G product rendering image pixels are converted to units of absolute
radiance using 32 bit floating point calculations. Pixel values are then
scaled to byte values prior to media output. The following equation is
used to convert DN's in a 1G product back to radiance units:
Lλ = Grescale * QCAL + Brescale
which is also expressed as:
Lλ = ((LMAXλ - LMINλ)/(QCALMAX-QCALMIN))
* (QCAL-QCALMIN) + LMINλ
| where: |
Lλ |
= Spectral Radiance at the sensor's aperture in watts/(meter
squared * ster * μm) |
|
Grescale |
= Rescaled gain (the data product "gain" contained in the Level
1 product header or ancillary data record) in watts/(meter
squared * ster * μm)/DN |
| |
Brescale |
= Rescaled bias (the data product "offset" contained in the Level
1 product header or ancillary data record ) in watts/(meter
squared * ster * μm) |
| |
QCAL |
= the quantized calibrated pixel value in DN |
| |
LMINλ |
= the spectral radiance that is scaled to QCALMIN in watts/(meter
squared * ster * μm) |
| |
LMAXλ |
= the spectral radiance that is scaled to QCALMAX in watts/(meter
squared * ster * μm) |
| |
QCALMIN |
= the minimum quantized calibrated pixel value (corresponding
to LMINλ) in DN
= 1 for LPGS products
= 1 for
NLAPS products processed after 4/4/2004
= 0 for NLAPS products processed before 4/5/2004 |
| |
QCALMAX |
= the maximum quantized calibrated pixel value (corresponding
to LMAXλ) in DN
= 255 |
The LMINs and LMAXs are the spectral
radiances for each band at digital numbers 0 or 1 and 255 (i.e QCALMIN,
QCALMAX), respectively. LPGS used 1 for QCALMIN while
NLAPS used 0 for QCALMIN for data products processed
before April 5, 2004. NLAPS from that date now uses 1 for the QCALMIN
value. Other product differences exist as well. One LMIN/LMAX set exists for each gain state. These values
will change slowly over time as the ETM+ detectors lose responsivity.
Table 11.2 lists two sets of LMINs and LMAXs. The first set should be
used for both LPGS and NLAPS 1G products created before July
1, 2000 and the second set for 1G products created after July
1, 2000. Please note the distinction between acquisition and processing
dates.
Use of the appropriate LMINs and LMAXs will ensure accurate conversion
to radiance units. Note for band 6: A bias was found in the
pre-launch calibration by a team of independent investigators post
launch. This was
corrected for in the LPGS processing system beginning Dec 20, 2000. For
data processed before this, the image radiances given by the
above transform are 0.31 w/m2 ster um too high. See the official announcement for more details. Note for the Multispectral Scanner (MSS),
Thematic Mapper (TM), and Advanced Land Imager (ALI) sensors: the
required radiometry constants are tabulated in this PDF file.
Table 11.2 ETM+ Spectral Radiance Range
watts/(meter squared * ster * μm) |
| Band Number |
Processed Before July 1, 2000 |
Proccessed After July 1, 2000 |
| Low Gain |
High Gain |
Low Gain |
High Gain |
| LMIN |
LMAX |
LMIN |
LMAX |
LMIN |
LMAX |
LMIN |
LMAX |
| 1 |
-6.2 |
297.5 |
-6.2 |
194.3 |
-6.2 |
293.7 |
-6.2 |
191.6 |
| 2 |
-6.0 |
303.4 |
-6.0 |
202.4 |
-6.4 |
300.9 |
-6.4 |
196.5 |
| 3 |
-4.5 |
235.5 |
-4.5 |
158.6 |
-5.0 |
234.4 |
-5.0 |
152.9 |
| 4 |
-4.5 |
235.0 |
-4.5 |
157.5 |
-5.1 |
241.1 |
-5.1 |
157.4 |
| 5 |
-1.0 |
47.70 |
-1.0 |
31.76 |
-1.0 |
47.57 |
-1.0 |
31.06 |
| 6 |
0.0 |
17.04 |
3.2 |
12.65 |
0.0 |
17.04 |
3.2 |
12.65 |
| 7 |
-0.35 |
16.60 |
-0.35 |
10.932 |
-0.35 |
16.54 |
-0.35 |
10.80 |
| 8 |
-5.0 |
244.00 |
-5.0 |
158.40 |
-4.7 |
243.1 |
-4.7 |
158.3 |
For relatively clear Landsat scenes, a reduction in between-scene variability
can be achieved through a normalization for solar irradiance by converting
spectral radiance, as calculated above, to planetary reflectance or albedo.
This combined surface and atmospheric reflectance of the Earth is computed
with the following formula:
| Where: |
|
 |
= Unitless planetary reflectance |
 |
= Spectral radiance at the sensor's aperture |
 |
= Earth-Sun distance in astronomical units from an Excel
file
or interpolated from values listed in Table 11.4 |
 |
= Mean solar exoatmospheric irradiances from
Table 11.3 |
 |
= Solar zenith angle in degrees |
Table 11.3 ETM+ Solar Spectral
Irradiances
(generated using the Thuillier solar
spectrum) |
| Band |
watts/(meter squared * μm) |
| 1 |
1997 |
| 2 |
1812 |
| 3 |
1533 |
| 4 |
1039 |
| 5 |
230.8 |
| 7 |
84.90 |
| 8 |
1362. |
| Table 11.4 Earth-Sun Distance
in Astronomical Units
|
| Day of Year |
Distance |
Day of Year |
Distance |
Day of Year |
Distance |
Day of Year |
Distance |
Day of Year |
Distance |
| 1 |
.98331 |
74 |
.99446 |
152 |
1.01403 |
227 |
1.01281 |
305 |
.99253 |
| 15 |
.98365 |
91 |
.99926 |
166 |
1.01577 |
242 |
1.00969 |
319 |
.98916 |
| 32 |
.98536 |
106 |
1.00353 |
182 |
1.01667 |
258 |
1.00566 |
335 |
.98608 |
| 46 |
.98774 |
121 |
1.00756 |
196 |
1.01646 |
274 |
1.00119 |
349 |
.98426 |
| 60 |
.99084 |
135 |
1.01087 |
213 |
1.01497 |
288 |
.99718 |
365 |
.98333 |
ETM+ Band 6 imagery can also be converted from spectral radiance (as described
above) to a more physically useful variable. This is the effective at-satellite
temperatures of the viewed Earth-atmosphere system under an assumption
of unity emmissivity and using pre-launch calibration constants listed
in Table 11.5. The conversion formula is:
| Where: |
|
| T |
= Effective at-satellite temperature in Kelvin |
| K2 |
= Calibration constant 2 from Table 11.5 |
| K1 |
= Calibration constant 1 from Table 11.5 |
| L |
= Spectral radiance in watts/(meter squared
* ster * µm) |
| Table 11.5 ETM+ and TM Thermal
Band Calibration Constants |
| |
Constant 1- K1
watts/(meter squared * ster * μm) |
Constant 2 - K2
Kelvin |
| Landsat 7 |
666.09 |
1282.71 |
| Landsat 5 |
607.76 |
1260.56 |
The same two 1R options exist for users when defining the size or spatial
extent of a Landsat level 1G product ordered from the LP-DAAC.
- Standard Worldwide Reference System (WRS) Scene. The standard
WRS scene, as defined above for the 0R product, can be ordered in 1G
form. Partial scenes that may exist at the beginning and end of subintervals
may be also be ordered.
- Partial Subinterval. A partial subinterval can also be ordered
in 1G form. Unlike the 0R product the 1G is limited to a maximum of
3 WRS scenes in size. The variably sized 1G product can float or be
positioned at any scan line starting point within a subinterval. Alternatively,
the product can be defined by up to three contiguous WRS locations.
The 1G product ordered from the LP-DAAC consists of the corrected image
files and descriptive metadata. All other ancillary files delivered with
the 0R and 1R products are not included. A user may order a subset of
the available bands which affects the actual file count in a 1G product.
The 1G product can be packaged into one of following user-specified output
formats:
- Hierarchical Data Format. The HDF packaging format used for the 0R and 1R products
is also used for structuring the 1G. The design employs external elements
for the band files and metadata. These are standalone files that are
referenced via tags and pointers residing in an HDF directory. External
elements provide users with two processing options - exploit the NCSA
HDF libraries for data access or process the data files directly using
homegrown code.
The number of files comprising an HDF-formatted 1G product will
vary according to the number of bands ordered. A product with a full
band complement has 11 files - the HDF directory, a metadata file,
and a separate file for each band. The HDF directory and metadata
files are always present regardless of bands ordered. Please refer
to the Landsat 7 0R Distribution
Product Data Format Control Book, Volume 5 (PDF) for details regarding
band file specifics. The 1R metadata file description can be found
in the ESDIS Level
1 Product Generation System Output Files DFCB (PDF).
The HDF format can be specified for any type of 1G product ordered
from the LP-DAAC.
- Fast. The Fast Format was originally developed by EOSAT as
a means for quickly accessing Landsat 4 and 5 image data. Its structure
is straightforwardly simple. Each band is self contained in its own
file (i.e external element style). A header file containing three records
accompanies the image data. The three records in order of appearance
are labeled administrative, radiometric, and geometric respectively.
Sensor specific information is placed in the administrative record,
gains and biases can be found in the radiometric record while projection
information and image coordinates are stored in the geometric record.
A single header file along with the image files constitute the Fast
product.
A derivative of the Fast Format (Fast-L7) used by EOSAT for Landsat
(FAST-B) and Indian Remote Sensing products (Fast-C) was created for
Landsat 7. Several differences are worth noting. File names are now
included in the administrative record which allows for direct file
access. A separate header file now accompanies the panchromatic, thermal
and VNIR/SWIR band groups for Landsat 7. For Fast-B and Fast-C all
bands were resampled to a common grid cell size thus permitting a
single header file. In all likelihood each of the band groups for
Landsat 7 will be resampled to a common resolution (i.e. 15, 30, &
60 meters) thus requiring a distinct header file for each.
All critical fields required for product ingest were left unchanged
in the Fast L-7A Format. As a consequence Heritage Fast readers residing
on user systems can be used for the Landsat 7 Fast formatted product.
A full layout of the Fast L-7A Format can be found in the ESDIS Level 1 Product Generation system Output Files DFCB.
The Fast-L7 format supports all variations of the 1G product.
- GeoTIFF. Geographic tagged image file format (GeoTIFF) is based
on Adobe's TIFF - a self-describing format developed to exchange raster
images such as clipart, logotypes, and scanned images between applications
and computer platforms. Today, the TIFF image file format is used to
store and transfer digital satellite imagery, scanned aerial photos,
elevation models, and output from digital cameras. TIFF is the only
full-featured format in the public domain, capable of supporting compression,
tiling, and extension to include geographic metadata.
The TIFF file consists of a number of label (tags) which describe
certain properties of the file (such as gray levels, color table,
byte format, compression size). After the initial tags comes the image
data which may be interrupted by more descriptive tags. GeoTIFF refers
to TIFF files which have geographic (or cartographic) data embedded
as tags within the TIFF file. The geographic data can then be used
to position the image in the correct location and geometry on the
screen of a geographic information display.
Baseline TIFF image types can be bilevel, greyscale, palette color,
and full color (24 bit). For simplicity's sake the grayscale model
was implemented for the Landsat 7 GeoTIFF product. Under this implementation
each ordered band is delivered as its own 8 bit greyscale GeoTIFF
image. A standard WRS scene possessing the full band complement would
thus be comprised of nine separate GeoTIFF images or files. No other
files accompany the product. For detailed information regarding the
Landsat 7 GeoTIFF implementation please refer to the ESDIS Level 1 Product Generation system Output Files DFCB (PDF).
For GeoTIFF details, please download the GeoTIFF Format Specification (PDF) or visit this web
site.
At the present time GeoTIFF format cannot be used for the Space
Oblique Mercator and Oblique Mercator projections. Products projected
into these reference systems must be formatted using HDF or Fast-L7.
An instrument malfunction occurred onboard Landsat 7 on May 31, 2003.
The problem was caused by failure of the Scan Line Corrector (SLC), which
compensates for the forward motion of the satellite. Subsequent efforts
to recover the SLC have not been successful, and the problem is
permanent.
The Landsat 7 Enhanced Thematic Mapper Plus (ETM+) is still capable
of acquiring useful image data with the SLC turned off, particularly
within the central portion of any given scene. Landsat 7 ETM+ will therefore
continue to acquire image data in the "SLC-off" mode.
EDC has recently released several Landsat 7 ETM+ SLC-off
data products. The first, a gap-present product became available on
October 22, 2003. This product release includes all image data acquired
by Landsat
7 in
SLC-off
mode
from July
14, 2003
to present, excluding a 2-week interval from 9/3/03 to 9/17/03.
The center of a gap-present SLC-off data product is very similar
in quality to previous Landsat 7 data. However, the scene's edges will
contain
alternating
scan lines of missing data (Level 1G) or duplicated data (Level 0Rp or
L1R). The precise location of the affected scan lines will vary from
scene to scene, and these gaps will not be visible on the browse image
preview when ordering SLC-off data. A preliminary report regarding the
utility of Landsat 7 SLC-off data is available in PDF form.
This report includes input from scientists affiliated with the USGS,
NASA, and the Landsat 7 Science Team.
The gap-present SLC-off data product is available as a single scene
entity in Level 1G terrain corrected (L1T) form.
As of November, 2008, the USGS offers all archived
Landsat scenes to the public at no charge. Newly acquired Landsat 7 ETM+
SLC-off and Landsat 5 TM images with less than 40 percent cloud cover
are automatically processed and made freely available for immediate download.
SLC-off data products can be searched and ordered via the Earth
Explorer, and Global
Visualization L7 Image Browser.
The second product now being offered (as of May 10, 2004) is in 1G form
and has the gap areas filled with Landsat 7 data acquired at a similar
time of year and prior to the SLC failure. The two scenes are geometrically
registered, and a histogram matching technique is applied to the fill
pixels which provides the best-expected radiance values for the missing
data.
Figure 11.4 - Top image: pre-SLC anomaly, middle of image. Middle
image: scene after SLC anomaly. Bottom image: scene after SLC anomaly
with data gaps filled.
The USGS, in conjunction with NASA, is continuing to research other
methods of providing merged data products and will continue to provide
information resulting from this work as it becomes available. Various
methodoligies have been examined to fill the data gaps with observations
acquired during prior or later than the target scene of interest. An
exampled of a gap-filled product is illustrated in Figure 11.4.
If available, the Landsat 7 definitive ephemeris is used for geometrically
correcting ETM+ data. Definitive ephemeris substantially improves
the positional accuracy of the Level 1G product over predicted ephemeris.
An ephemeris is a set of data that provides the assigned places
of a celestial body (including a manmade satellite) for regular
intervals. In the context of Landsat 7, ephemeris data shows the
position and velocity of the spacecraft at the time imagery is collected.
The position and velocity information are used during product generation.
The Landsat 7 Mission Operations Center receives tracking data
on a daily basis that shows the position and velocity of the Landsat
7 spacecraft. This information comes from the three US operated
ground-receiving stations and is augmented by similar data from
NASA's Tracking and Data Relay Satellites. The Flight Operations
Team processes this information to produce a refined or "definitive"
ephemeris that shows the position and velocity of Landsat 7 in one
minute intervals. Tracking data are used to compute the actual spacecraft
position and velocity for the last 61 hours and to predict these
values for the next 72 hours. The predicted ephemeris data are uploaded
to the spacecraft daily. On-board software interpolates from this
data to generate the positional information contained in the Payload
Correction Data (PCD).
Engineers with the Landsat Program have completed a predicted versus
definitive ephemeris analysis. Comparisons to ground control points
demonstrate the definitive ephemeris is, in fact, reliably more
accurate than the predicted ephemeris. Geometric accuracy on the
order of 30-50 (1 sigma) meters, excluding terrain effects, can
be achieved when the definitive ephemeris is used to process the
data. Level 1G products produced after March 29, 2000 use definitive
ephemeris if available. The .MTL field "ephemeris_type" in the product
metadata files identifies whether a product was created with definitive
or predicted ephemeris. Daily definitive ephemeris profiles have
been archived since June 29, 1999 and are available for downloading.
11.3.8 Radiometric Scaling Parameters for Landsat 7 ETM+ Level 1G Products |
Back to Top |
The LMIN's and LMAX's are a representation of how
the output Landsat ETM+ Level 1G data products are scaled in radiance
units. The LMIN corresponds to the radiance at the minimum quantized
and calibrated data digital number (QCALMIN), which is typically
"1" or "0" and LMAX corresponds to the radiance at the maximum quantized
and calibrated data digital number(QCALMAX), typically "255".
Reflective bands:
The LMIN's are set so that a "zero radiance" scene
will still be on scale in the 8 bit output product, even with sensor
noise included. LMIN should result in "zero " radiance being about
5 DN in low gain and 7.5 DN in high gain. The LMAX's are set so
that LMAX corresponds to slightly less than the saturation radiance
of the most sensitive detector. This is done so that in the output
product all "pixels" saturate at the same radiance. Currently the
LMAX is set to be 0.99 of the pre-launch saturation radiance of
the most sensitive detector in each band.
Normally, there is no need to change the LMIN's or
LMAX's, unless something changes drastically on the instrument.
If the sensitivity of the instrument increases, which is not expected,
there is no need to change the LMIN and LMAX values. If the sensitivity
decreases, the LMAX values can be increased which in turn increases
the usable dynamic range of the product (this will not occur unless
the change is large). The changes that have taken place to date
have been mostly due to the adoption of "improved" pre-launch gains
for the instrument that have, in effect, "increased" its sensitivity.
The Landsat Project Science Office also detected a few errors in
the original numbers, which were corrected.
|