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.
| Interesting Landslide Morphology and Phyllosilicate Detections : ESP_044871_1740 ESP_043961_1740 (Interval in Earth days: 71) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.17 | 137. | 7.69 | 21.68 | 54.3 | 53.3 |
| Pasted-on Material on Crater Ejecta : ESP_044720_1890 ESP_045353_1890 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.847 | 299. | -8.8 | 8.465 | 47.6 | 46.2 |
| Pits Fissures and Channels East of Olympus Mons : ESP_044841_1960 ESP_044907_1960 (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 | 15.86 | 233. | 6.54 | -11.9 | 43.6 | 45.1 |
| Candidate ExoMars Landing Site in Oxia Palus : ESP_044824_1985 ESP_062481_1985 (Interval in Earth days: 1376) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.08 | 336. | 23.1 | 5.898 | 41.5 | 45.8 |
| Double-Terraced Crater in Arcadia Planitia : ESP_044724_2270 ESP_044869_2270 (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 | 46.75 | 183. | 5.44 | 19.31 | 41.4 | 40.8 |
| Possible Phyllosilicates in Knobs within Depression on Dichotomy Boundary : ESP_044995_2165 ESP_052023_2165 (Interval in Earth days: 548) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.32 | 347. | 7.00 | 27.66 | 41.0 | 36.1 |
| Southwestern Elysium Planitia : ESP_044963_1815 ESP_045385_1815 (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 | 1.457 | 146. | -1.1 | 12.18 | 50.5 | 48.9 |
| Fractured Surface Near Athabasca Valles Lava : ESP_044831_1825 ESP_053560_1825 (Interval in Earth days: 680) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.431 | 148. | 3.35 | 17.54 | 49.8 | 49.5 |
| North Polar Layered Deposits 160-Meter Diameter Crater Monitoring : ESP_044810_2620 ESP_044784_2620 (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 | 81.84 | 333. | 7.95 | -6.74 | 59.0 | 59.6 |
| Meridiani Planum : ESP_044718_1780 ESP_046274_1780 (Interval in Earth days: 122) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.19 | 354. | 2.37 | 19.53 | 52.6 | 49.7 |
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