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.
| North Polar Layered Deposits: ESP_018910_2625 ESP_018870_2625 (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 | 82.36 | 34.0 | -16. | -0.48 | 65.6 | 64.2 |
| Small Cut Crater in Capri Chasma: ESP_018940_1680 ESP_025599_1680 (Interval in Earth days: 519) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.7 | 311. | -8.4 | 2.74 | 60.7 | 54.3 |
| Slope Streaks on Dunes Change Detection: ESP_018839_2635 ESP_019143_2635 (Interval in Earth days: 24) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 83.47 | 118. | 29.2 | 17.73 | 63.9 | 67.4 |
| Small Cone in Hydraotes Chaos: ESP_019124_1805 ESP_019269_1805 (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 | 0.248 | 326. | -4.3 | 11.07 | 54.5 | 53.4 |
| Utopia Planitia Crater: ESP_018894_2115 ESP_019316_2115 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 30.96 | 121. | 1.64 | -11.7 | 46.5 | 51.1 |
| High-Latitude Exposure of North Polar Layered Deposits: ESP_019178_2675 ESP_028067_2675 (Interval in Earth days: 693) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.66 | 228. | -7.9 | -19.4 | 71.9 | 73.2 |
| Possible MSL Rover Landing Site Holden Crater: ESP_019045_1530 ESP_019322_1530 (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 | -26.6 | 325. | 8.87 | -19.8 | 67.8 | 68.0 |
| Layered Terrain in Aeolis Planum: ESP_018959_1730 ESP_019025_1730 (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 | -6.90 | 150. | 4.52 | -18.8 | 57.2 | 58.8 |
| Possible MSL Landing Site in Gale Crater: ESP_018854_1755 ESP_018920_1755 (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 | -4.58 | 137. | 5.54 | -18.0 | 56.2 | 57.8 |
| Syrtis Major Planum Channel and Depression: ESP_018988_1980 ESP_042882_1980 (Interval in Earth days: 1861) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.54 | 76.5 | 0 | -26.9 | 48.6 | 42.2 |
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