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.
| Monitor Seasonal Changes at South Polar Cracked and Gullied Site: ESP_031213_0980 ESP_031266_0980 (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 | -81.6 | 66.2 | 6.48 | -6.79 | 61.2 | 62.4 |
| Sediments in Valleys Upslope of Ladon Valles Basin: ESP_030939_1600 ESP_031796_1600 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.9 | 327. | -2.4 | 17.48 | 38.4 | 30.6 |
| Ancient Rocks of the Isidis Basin: PSP_002756_1830 PSP_002822_1830 (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 | 3.174 | 84.9 | 2.98 | -19.6 | 55.7 | 57.7 |
| A Sinuous Ridge in Gale Crater: ESP_030814_1750 ESP_030748_1750 (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 | -4.72 | 138. | 4.50 | 28.32 | 44.8 | 43.7 |
| Gully Monitoring: ESP_030874_1315 ESP_030584_1315 (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 | -47.9 | 303. | 24.6 | 6.268 | 39.3 | 43.6 |
| Gullies on Hills in Center of Hale Crater: ESP_030715_1440 ESP_030570_1440 (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 | -35.6 | 323. | 25.9 | 11.37 | 37.7 | 40.8 |
| Central Uplift of a 30-Kilometer Diameter Crater in Noachis Terra: ESP_030808_1535 ESP_031230_1535 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.0 | 303. | 18.0 | 0.342 | 37.3 | 34.4 |
| South Polar Layered Deposit Spiral Troughs During Katabatic Wind Season: ESP_030612_0945 ESP_030639_0945 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -85.4 | 289. | 5.81 | -8.39 | 64.1 | 65.3 |
| Curved Ridges in THEMIS Images I09636004 and I16687004 and I16712004: ESP_030831_1335 ESP_031108_1335 (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 | -46.2 | 37.9 | 21.4 | -3.99 | 39.4 | 39.4 |
| Patterned Ground on Channel Floor: ESP_030698_1180 ESP_030632_1180 (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 | -61.6 | 79.0 | -22. | -12.1 | 50.4 | 50.3 |
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