ASTER
(Advanced Spaceborne Thermal Emission and Reflection Radiometer) is an imaging
instrument flying on Terra, a satellite launched in December 1999 as part of
NASA's Earth Observing System (EOS). ASTER is a cooperative effort between
NASA,
The following analysis was done using software from Wimsoft (http://wimsoft.com).
Table 1. ASTER
bands
Band |
Bandwidth (nm)
|
Pixel Size (m)
|
Remarks |
VNIR = visible near-infrared |
|||
1 |
520 - 600 |
15 |
|
2 |
630 - 690 |
15 |
|
3N |
760 - 860 |
15 |
N = normal |
3B |
760 - 860 |
15 |
B = backward looking
at 26.7˚ |
SWIR = shortwave infrared |
|||
4 |
1600 - 1700 |
30 |
|
5 |
2145 - 2185 |
30 |
|
6 |
2185 - 2225 |
30 |
|
7 |
2235 - 2285 |
30 |
|
8 |
2295 - 2365 |
30 |
|
9 |
2360 - 2430 |
30 |
|
TIR = thermal infrared |
|||
10 |
8125 - 8475 |
90 |
|
11 |
8475 - 8825 |
90 |
|
12 |
8925 - 9275 |
90 |
|
13 |
1025 - 1095 |
90 |
|
14 |
1095 - 1165 |
90 |
|
Detailed instructions for ordering and processing ASTER data are given in Exercises_ASTER.pdf. A few examples are shown below.
The RGB composite was created from ASTER VNIR
bands 1, 2 and 3N. ASTER does not have a real blue band and therefore the
created RGB image does not look like a true-color image. Below is a small
subset of a RGB image of the
.
The full image as well as images from other dates are available at http://spg.ucsd.edu/Satellite_Data/Venice.
A WAM utility wam_turbidity_aster
calculates relative turbidity by subtracting ASTER band 2 from band 1. Itis
convenient to represent turbidity as a grayscale image with turbid areas dark
(black) and clear areas light (white). Note the high turbidity cloud south of
A RGB composite from ASTER
bands 1, 2 and 3N of the
Outflow from the Los Buenos
creek, affected by the Mexican sewage treatment plant can be seen on this image. Increased turbidity in the outflow plume is
shown below.
Aster images are suitable
for visualization with Google Earth (http://earth.google.com/download-earth.html).
After you have installed Google Earth, you can create a KML file for your ASTER
(it is easy to create, see Exercises_ASTER.pdf)
and then just clicking on the KML file starts Google
Earth that would load your specified image. The ASTER PNG file will overlay the
original Google Earth image of the area. The PNG file is about 27-30 MB in size
and may take a while to download. In the screen shot example below, the Google
earth data is in the top part and the overlaid ASTER data below it. As you can
see, the navigation of the ASTER data is excellent and the two parts match very
well. This way you can read, for example, the place
names from Google Earth.
You can try to load the
full ASTER image of the San Diego area into Google Earth with the following KML file and the Venice image with the
following KML file.
It should be noted that ASTER
was designed for land applications and therefore the sensitivity of its VNIR
bands is not sufficient to see much structure in the open ocean. However, in near-shore
turbid environments ASTER data can be useful.
ASTER, RGB of channels 1-2-3N, 2005-March-22 (click on the image to view a larger version)
A comparison of ASTER and MODIS data is shown here.
![]() |
View this image in Google Earth |