IRIAN JAYA, INDONESIA, and NEW ZEALAND
IRIAN JAYA, INDONESIA, and NEW ZEALAND
IRIAN JAYA, INDONESIA, and NEW ZEALAND
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Imaging of Glaciers<br />
Aerial Photography<br />
The first known sequences of vertical aerial photographs in New<br />
Zeal<strong>and</strong> were taken around 1937 <strong>and</strong> 1938 by New Zeal<strong>and</strong> Aerial Map<br />
ping, Ltd., but these were mainly of lowl<strong>and</strong> areas. A set of vertical<br />
aerial photographs was taken over the Franz Josef, Fox, Tasman, <strong>and</strong><br />
Hooker Glaciers in 1953, followed by a most useful set of oblique aerial<br />
photographs taken by the Royal New Zeal<strong>and</strong> Air Force along both sides<br />
of the Southern Alps in autumn 1955. These surveys were made just<br />
prior to the first of the systematic vertical aerial photographic flights<br />
made over the Southern Alps as part of a nationwide aerial photo-<br />
grammetric mapping program. By the end of the 1960's all of the<br />
glacierized areas were photographed, <strong>and</strong> many areas have been re-<br />
photographed since.<br />
Satellite Imagery<br />
All of New Zeal<strong>and</strong>'s glacierized areas are included in existing L<strong>and</strong>sat<br />
images, but not all of the images are usable for glacial observations<br />
(fig. 8). The two requisites for an optimum usable image are no cloud<br />
cover <strong>and</strong> an image acquired at the time of minimum snow cover (late<br />
summer). Many of the better images of the glacierized areas have glacial<br />
features obscured by seasonal snow. The coding for each of the nominal<br />
scene centers shown on figure 8 refers primarily to the amount of cloud<br />
cover over the glacierized regions. Table 1 provides additional informa<br />
tion on each image, including remarks about amount of snow cover.<br />
Table 1 lists the known usable images of the New Zeal<strong>and</strong> glaciers.<br />
Many additional images exist, but these are generally unacceptable be<br />
cause of excessive cloud cover or because of snow cover on winter<br />
scenes. Unfortunately, the L<strong>and</strong>sat satellite paths <strong>and</strong> image rows do<br />
not coincide well with the configuration of the glacierized areas. This<br />
results in images of the more important glacerized regions appearing at<br />
the margins of the images. The best available image of the Mount Cook<br />
area is the larger scale (1:500,000) L<strong>and</strong>sat 3RBV image (30324-21342,<br />
subscene A), corresponding to the northwest quadrant of Path 79, Row<br />
91, but this image lacks relief detail in the snowfields (Ferrigno <strong>and</strong><br />
Williams, 1983).<br />
L<strong>and</strong>sat images are more appropriate for the larger glaciers, because<br />
the spatial resolution of the image is inadequate for identifying details of<br />
small glaciers less than about 1 or 2 km2 in area. On a l:l,000,000-scale<br />
L<strong>and</strong>sat MSS image 1 km equals 1 mm, so a 1-km2 glacier would<br />
measure 1 mm2 on the image. Even on a 1:500,000-scale L<strong>and</strong>sat 3 RBV<br />
image, a 1-km2 glacier would only be 4 mm2 . Unfortunately the rapid<br />
changes in small, steep, <strong>and</strong> very active glaciers, such as the one shown<br />
in figure 9, are difficult to monitor by satellite imagery. On some small<br />
glaciers the snowline has recently risen beyond the upper limits of the<br />
glacier, thereby leaving the entire glacier in the ablation zone (fig. 10).<br />
H36 SATELLITE IMAGE ATLAS OF GLACIERS OF THE WORLD