Planned stereo pairs have suitable stereo convergence angles and illumination by design.
In addition to planned stereo pairs, the Pairendipity software can identify overlapping
HiRISE images that are serendipitously suitable for stereo processing and find stereo
pairs within the CTX dataset.
Planned HiRISE stereo pairs are listed in the “Stereo Pair List (CSV)” link below.
Since this list is based on produced stereo anaglyphs it also contains a few serendipitous
pairs that underwent special processing. Most serendipitous HiRISE stereo pairs are listed
in the “Pairendipity Stereo” link, while CTX stereo pairs are listed
in “Pairendipity CTX Stereo”.
Images taken close together in time minimize illumination and frost differences and are
especially useful (see the Delta-Days column in the Pairendipity files or difference
the orbit numbers in the image IDs in the Stereo Pair List file). Stereo pairs
with both images planned within the same 14-day (168-orbit) operations cycle are known as SPORCs.
| Ancient Clays near the Hellas Basin: ESP_093165_1555 ESP_093600_1555 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.3 | 45.7 | -7.4 | 24.85 | 35.8 | 32.7 |
| Ice Margin of Lobate Debris Apron: ESP_092504_1370 ESP_092715_1370 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -42.8 | 97.1 | -1.2 | -21.8 | 42.3 | 42.1 |
| Troughs overlying South Polar Layered Deposit: ESP_092416_0905 ESP_083622_0905 (Interval in Earth days: 685) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -89.3 | 8.90 | 28.4 | 26.90 | 64.8 | 64.9 |
| Channel Leading to Crater in Terra Cimmeria: ESP_092594_1695 ESP_092805_1695 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -10.5 | 154. | 0.42 | -22.8 | 43.9 | 43.2 |
| Hillslope Morphologies near Eberswalde Crater: ESP_092601_1550 ESP_092812_1550 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.7 | 325. | -4.5 | -25.4 | 40.5 | 39.9 |
| Potential Compound Dune in USGS Dune Database 1687-642: ESP_092317_1155 ESP_092383_1155 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -64.2 | 168. | 0.25 | -14.7 | 52.1 | 52.5 |
| Streamlined Shapes South of Harmakhis Vallis: ESP_092425_1385 ESP_092636_1385 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -41.0 | 93.9 | 2.97 | -20.3 | 42.5 | 42.2 |
| South Polar Glacier Crevasses: ESP_092682_0915 ESP_092589_0915 (Interval in Earth days: 8) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.6 | 323. | 22.6 | 26.11 | 64.9 | 64.3 |
| Triangular Scars on Hillslopes: ESP_092549_1335 ESP_092325_1335 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -46.2 | 308. | 3.67 | -16.2 | 42.4 | 46.3 |
| Holden Crater Sedimentary Fan: ESP_092456_1525 ESP_092667_1525 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.9 | 325. | 0.76 | -25.0 | 41.6 | 41.2 |
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