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.
| Exposure of South Polar Layered Deposits: ESP_031942_0875 ESP_040660_0875 (Interval in Earth days: 679) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.5 | 71.2 | 8.44 | 24.55 | 76.9 | 75.5 |
| Small Crater on South Polar Layered Deposits: ESP_031994_0920 ESP_032111_0920 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.8 | 48.7 | 6.86 | 18.71 | 76.3 | 76.4 |
| Exposure of South Polar Layered Deposits: ESP_032098_0875 ESP_040483_0925 (Interval in Earth days: 653) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.6 | 132. | 8.52 | 6.282 | 79.2 | 71.4 |
| Southern Hemisphere Dune Changes: ESP_031882_1135 ESP_031895_1135 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -66.2 | 151. | -7.7 | 18.93 | 56.4 | 55.2 |
| Exposure of South Polar Layered Deposits: ESP_031929_0925 ESP_032231_0925 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.4 | 31.1 | 1.24 | 7.938 | 75.8 | 79.0 |
| Exposure of South Polar Layered Deposits: ESP_031827_0940 ESP_031775_0940 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -85.8 | 236. | 8.00 | -7.60 | 71.0 | 71.7 |
| Fresh Shallow Valleys: ESP_031789_1380 ESP_049881_1380 (Interval in Earth days: 1410) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -41.5 | 162. | 5.59 | -8.59 | 38.0 | 42.9 |
| Rough Terrain and Albedo Boundary on South Polar Layered Deposits: ESP_032059_0925 ESP_032216_0925 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.4 | 82.3 | 1.27 | 8.289 | 77.8 | 78.9 |
| Noctis Labyrinthus Bedform Changes: ESP_031838_1685 ESP_032115_1685 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.1 | 261. | -2.5 | -20.9 | 32.8 | 33.7 |
| Youthful Crater Superimposed on Volcanic Plain: ESP_031974_1855 ESP_039873_1855 (Interval in Earth days: 616) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.304 | 146. | 4.53 | 16.53 | 37.3 | 48.5 |
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