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.
| Gullies in Resistant Layers of Crater Wall: ESP_023289_1335 ESP_022999_1335 (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 | -46.1 | 18.9 | 26.3 | -0.21 | 42.6 | 41.0 |
| Gully Change Detection: ESP_023111_1330 ESP_023032_1330 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -46.3 | 197. | 29.0 | 2.043 | 40.3 | 41.2 |
| Layers on Hellas Planitia Rim and Proposed Site for Future Exploration: ESP_023195_1505 ESP_023340_1505 (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 | -29.1 | 66.7 | -12. | 6.662 | 35.1 | 34.9 |
| Crater with Rugged Floor in THEMIS V26860010: ESP_023396_1490 ESP_024319_1490 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -30.8 | 338. | 2.17 | 16.49 | 36.5 | 49.0 |
| Polar Layers Exposed on Promethei Lingula Surface: ESP_023102_0980 ESP_022983_0980 (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 | -82.0 | 111. | -8.0 | 6.991 | 70.0 | 67.3 |
| Bedrock Exposed in Rim and Terraces of Crater in Molesworth Crater: ESP_023126_1520 ESP_023627_1520 (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 | -27.4 | 149. | -7.8 | 15.53 | 33.7 | 36.6 |
| Proposed MSR Landing Site in Mawrth Vallis: ESP_023132_2050 ESP_023409_2050 (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 | 24.73 | 338. | -1.9 | -22.7 | 50.0 | 47.8 |
| Lateral Dunes: ESP_023270_1120 ESP_023349_1120 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -67.6 | 185. | 2.54 | 19.45 | 59.8 | 60.1 |
| Crater with Depression in Central Peak: ESP_023381_1205 ESP_031240_1205 (Interval in Earth days: 612) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -59.0 | 37.2 | -26. | -4.83 | 56.5 | 45.9 |
| Proposed MSR Landing Site in Jezero Crater: ESP_023102_1985 ESP_023168_1985 (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 | 18.34 | 77.7 | 8.20 | -11.8 | 45.2 | 45.6 |
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