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.
| Olivine-Rich Terrain in Yuty Crater: ESP_016579_2025 ESP_017647_2025 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.08 | 325. | 1.00 | 18.99 | 40.6 | 42.1 |
| Terrain South of Newcomb Crater: ESP_016736_1520 ESP_068970_1525 (Interval in Earth days: 4070) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.6 | 5.59 | 4.65 | -7.50 | 65.7 | 63.9 |
| Small Volcano in Northern Syria Planum: ESP_016318_1710 ESP_016951_1710 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.76 | 254. | 6.70 | -9.92 | 48.9 | 55.9 |
| Layered Walls of Impact Crater in Mawrth Vallis Outcrops: ESP_016895_2045 ESP_017040_2045 (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 | 23.95 | 339. | -3.5 | 8.322 | 41.6 | 41.0 |
| Deposits on the Floor of Palos Crater: ESP_016943_1775 ESP_017721_1775 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.67 | 111. | 5.57 | -9.88 | 51.3 | 55.9 |
| Candidate Landing Site in a Possible Salt Playa: ESP_016288_1745 ESP_016433_1745 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.64 | 353. | 0.58 | 17.63 | 47.4 | 47.7 |
| Well-Preserved Impact Crater: ESP_015905_2235 ESP_016182_2235 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 42.91 | 3.36 | 3.72 | -15.9 | 45.9 | 45.8 |
| Gullied Crater Wall: ESP_015950_1395 ESP_016451_1395 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -40.3 | 225. | 4.65 | 25.21 | 64.5 | 70.3 |
| Livny Crater: ESP_016223_1525 ESP_050956_1525 (Interval in Earth days: 2707) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.1 | 330. | 2.51 | -21.4 | 59.3 | 51.0 |
| Cerberus Fossae Cutting Hill: ESP_016229_1895 ESP_016862_1895 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.130 | 162. | 4.10 | -9.74 | 40.9 | 46.1 |
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