UPPER COLCA ARCHAEOLOGICAL
RESEARCH PROJECT
Arequipa, Peru
SEASONALITY IN THE COLCA VALLEY
Precipitation
in the Colca Valley
is seasonal and it
greatly influences the scheduling of irrigation agriculture and grazing
activities in the region (Guillet and Mitchell 1991). The Colca is located at the edge of the tropics at a latitude of 15.6° South, and is in a semi-arid environment. Two ASTER satellite images are
presented below that demonstrate the seasonality of precipitation in a part of the Colca Valley
where the river is at an altitude of
approximately 3600 meters above sea level (masl) or about 11,800'.
About this imagery
These ASTER images are composed of Very
Near Infra Red (VNIR) bands. In this data the band 3 (displayed as
red) is of a slightly longer wavelength than the visual red band and
therefore highly photosynthesizing plants appear as a brilliant red
in these images. More information about ASTER is available online.
Sept 28, 2000 scene
The dry winter season was nearly over when the first image
was recorded on Sept 28, 2000 by the ASTER sensor. Note that the
well-watered marshlands on eastern side of this subset are at over
4500 masl but are quite lush.
May 1, 2001 scene
The second scene is from May 1 which is well after the end of the rainy
season and is the austral autumn. Higher elevation crops that grow more slowly may not yet been
harvested. The vegetation in non-irrigated areas is considerably
more vibrant than in the September scene.
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The dry season
-- 28 September 2000

Click
image to view full scene
The end of the wet season
-- 1 May 2001

Click
image to view full scene
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Click here to view
a scanned 1:100,000 scale topographic map of the same coverage
region (140k file). |
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A procedure called
Normalized Difference Vegetation Index (NDVI) can be used to
quantify photosynthesis and vegetative mass with some multispectral
imagery. The NDVI method was used with bands 2 and 3n of the
Sept 28 2000 ASTER scene in Erdas Imagine 8.4. A
modified version of the Landsat TM NDVI script was used in the
calculation, the function is as follows:
ASTER NDVI = (B3n — B2) / (B3n + B2)
In the resulting image the
vegetation with high photosynthesis rates, which will absorbs most of the visual band light,
is displayed as dark green. The sparse, dry, or unhealthy vegetation
that fails to absorb visual spectra light, and therefore reflects it
back at the satellite sensor, is displayed as dark
brown.

Click image to view higher resolution PDF file.
The higher altitude marshlands and irrigated grazing
areas stand out in the NDVI image as having high values (Dark
Green), as do the irrigated and yet unharvested crops in the valley bottom. The high altitude puna
grassland is relatively low productivity vegetation. The lowest NDVI
values are derived from the rhyolitic boulder fields on the 5000m
high Ancachita volcano, on the right side of the image. These rocky
slopes have
extremely low vegetative growth and therefore the Near IR and Visual
bands reflect back in roughly equal amounts.
ASTER visual band spectral information
| ASTER Band |
Visual Color |
Spectral
wavelength |
| Band 1 (Visual) |
Blue |
0.52
- 0.60 mm |
| Band 2
(Visual) |
Green |
0.63
- 0.69 mm |
| Band 3 (Visual -
Near IR) |
Red |
0.78
- 0.86 mm |
- Guillet, David W., & Mitchell, William (editors)
- 1991. Irrigation at high altitudes: the social organization of irrigation in the Andes. American Anthropological Association, Washington, D.C.
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