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.
| Small Feature on South Polar Layered Deposits: ESP_041111_0925 ESP_041004_0925 (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 | -87.2 | 244. | 7.47 | 28.48 | 80.0 | 76.6 |
| Ridges and Light-Toned Outcrops North of Atlantis Chaos: ESP_041151_1500 ESP_047309_1500 (Interval in Earth days: 480) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -29.7 | 181. | -8.0 | 2.323 | 39.6 | 50.5 |
| Light-Toned Hydrated Materials Inside Ius Chasma: ESP_041121_1725 ESP_048136_1725 (Interval in Earth days: 547) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.24 | 276. | 1.18 | 20.39 | 33.8 | 43.6 |
| Candidate Landing Site for 2020 Mission in Hypanis Valles Delta: ESP_041436_1920 ESP_041858_1920 (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 | 12.02 | 314. | -0.1 | -24.4 | 37.7 | 39.3 |
| Possible Degraded Crater on South Polar Layered Deposits: ESP_041218_0925 ESP_041309_0925 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.6 | 243. | 3.20 | 9.973 | 83.4 | 83.5 |
| Protonilus Region Terraces: ESP_041129_2210 ESP_041406_2210 (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 | 40.73 | 51.7 | 5.59 | -14.1 | 57.6 | 55.0 |
| Gigas Sulci: ESP_040661_1890 ESP_041149_1890 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.091 | 233. | 7.06 | -29.4 | 41.8 | 40.3 |
| Icy Scarp: ESP_040772_1215 ESP_041062_1215 (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 | -58.0 | 93.6 | -4.8 | 13.05 | 51.8 | 55.0 |
| Well-Preserved Gullied 15-Kilometer Impact Crater: ESP_040964_1305 ESP_057856_1305 (Interval in Earth days: 1316) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -49.1 | 249. | -4.2 | 5.903 | 48.2 | 38.7 |
| Layering on Floor of Orson Welles Crater: ESP_040790_1805 ESP_056996_1805 (Interval in Earth days: 1263) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.309 | 314. | -20. | 5.758 | 38.3 | 48.2 |
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