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.
| 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 |
| Unusual Structures in North Polar Layered Deposits : ESP_044794_2620 ESP_045308_2620 (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 | 81.91 | 60.4 | -8.8 | 5.241 | 59.7 | 63.2 |
| Lyot Crater Ejecta : ESP_044743_2290 ESP_044888_2290 (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 | 48.48 | 26.1 | -7.7 | 6.254 | 43.1 | 42.6 |
| 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 |
| Channels on Alba Mons : ESP_044814_2270 ESP_045157_2270 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 46.47 | 246. | 6.41 | -14.1 | 41.6 | 45.4 |
| Fractures and Exposed Bedrock in Lyot Crater : ESP_044756_2300 ESP_045099_2300 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 49.56 | 28.7 | 8.24 | -10.8 | 42.1 | 45.7 |
| 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 |
| Unusual Crater in Amazonis Planitia : ESP_044855_2090 ESP_044921_2090 (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 | 28.72 | 210. | 3.03 | -12.8 | 41.0 | 42.5 |
| Transverse Aeolian Ridges in Scandia Cavi : ESP_044722_2570 ESP_044405_2570 (Interval in Earth days: 25) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 76.93 | 226. | 2.31 | 28.96 | 55.5 | 52.8 |
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