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.
| Valley along Noctis Labrynthus Floor: ESP_017465_1730 ESP_017966_1730 (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 | -7.16 | 261. | -10. | 10.24 | 57.8 | 57.8 |
| Pit Craters in North Polar Layered Deposit: ESP_017376_2645 ESP_018918_2645 (Interval in Earth days: 120) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.39 | 134. | 0.70 | 16.29 | 60.4 | 65.5 |
| Possible Kieserite Deposit on Flanks of Hebes Mensa: ESP_017319_1785 ESP_017385_1785 (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 | -1.24 | 284. | 10.7 | -13.0 | 52.2 | 54.2 |
| Well-Preserved 1-Kilometer Diameter Impact Crater on Northern Plains: ESP_017480_2355 ESP_017968_2355 (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 | 55.21 | 200. | 6.86 | -14.0 | 44.1 | 46.3 |
| Central Uplift of a Northern Plains Impact Crater: ESP_017453_2315 ESP_024969_2315 (Interval in Earth days: 586) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 51 | 220. | -6.6 | 9.417 | 43.9 | 46.9 |
| Southern Gale Crater Strata with Possible Sulfates and Clays: ESP_017364_1745 ESP_017509_1745 (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 | -5.59 | 138. | -8.2 | 6.376 | 56.3 | 55.9 |
| Cone with Lobate Flows in Hydraotes Chaos: ESP_017634_1800 ESP_025493_1800 (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 | -0.10 | 326. | -12. | -26.9 | 54.3 | 49.1 |
| Western Half of Fresh Crater on Alba Patera: ESP_017571_2235 ESP_017861_2235 (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 | 43.05 | 240. | -9.5 | 10.32 | 42.5 | 41.3 |
| Thermally-Anomalous Crater on Hrad Vallis Flow: ESP_017601_2145 ESP_018023_2145 (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 | 34.20 | 141. | 6.74 | -6.84 | 40.9 | 43.0 |
| Western Rim Well-Preserved 25-Kilometer Diameter Crater in Acidalia Region: ESP_017370_2170 ESP_017871_2170 (Interval in Earth days: 40) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.52 | 329. | -8.4 | 6.007 | 41.9 | 41.5 |
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