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.
| Layered Material and Proposed Site for Future Exploration: ESP_024553_1500 ESP_024843_1500 (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 | -29.8 | 71.8 | -7.0 | 15.99 | 53.5 | 56.6 |
| Dune Composition: ESP_025042_1375 ESP_024976_1375 (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 | -42.3 | 42.0 | 0.35 | 18.39 | 69.4 | 67.5 |
| Meanders and Tributaries in Ridge Form in the Zephyria Region: ESP_024484_1750 ESP_024985_1750 (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 | -5.09 | 151. | 4.43 | 19.16 | 38.5 | 43.0 |
| Lava Coating, Flood-Carved Kasei Valles: ESP_024202_2010 ESP_024703_2010 (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 | 20.84 | 287. | -2.9 | 19.15 | 38.0 | 35.7 |
| The Eastern Floor of Aram Chaos: ESP_024266_1830 ESP_023910_1830 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.112 | 340. | 24.6 | 9.188 | 33.0 | 32.9 |
| MSL Landing Site in Gale Crater: ESP_023957_1755 ESP_024023_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 | -4.55 | 137. | 15.1 | -6.86 | 32.6 | 34.9 |
| Valleys on Western Hecates Tholus: ESP_024207_2130 ESP_024352_2130 (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 | 32.52 | 149. | -0.4 | 16.28 | 43.3 | 41.0 |
| Dunes: ESP_024060_1205 ESP_023928_1205 (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 | -59.1 | 218. | -18. | 5.39 | 67.4 | 63.9 |
| Remnant of Unconformable Deposit in Electris: ESP_023929_1425 ESP_024074_1425 (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 | -37.0 | 189. | -20. | -5.72 | 49.1 | 50.5 |
| Harmakhis Vallis Terrain Sample: ESP_024249_1405 ESP_024394_1405 (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 | -39.2 | 92.0 | -1.1 | 16.31 | 54.7 | 56.2 |
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