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.
| Northwestern Ejecta Feature of Noord Crater: ESP_061017_1605 ESP_060951_1605 (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 | -19.3 | 348. | -5.9 | 14.29 | 60.8 | 59.1 |
| Modification of Fresh Crater at High-Latitudes: ESP_061047_2485 ESP_061060_2485 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 68.13 | 234. | -1.3 | 18.05 | 51.6 | 50.2 |
| Candidate Landing Site for 2020 Mission in Jezero Crater: ESP_061185_1985 ESP_060908_1985 (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 | 18.43 | 77.0 | 2.38 | 19.53 | 41.4 | 38.7 |
| Crater with Exit Breach: ESP_061037_1375 ESP_061103_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 | 164. | 4.61 | -11.8 | 77.3 | 78.8 |
| Candidate Landing Site for SpaceX Starship Near Arcadia Planitia: ESP_061128_2190 ESP_061194_2190 (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 | 38.63 | 190. | 2.81 | -11.6 | 39.5 | 40.8 |
| Candidate Landing Site for SpaceX Starship in Arcadia Region: ESP_061141_2195 ESP_061075_2195 (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 | 39.17 | 195. | -0.9 | 13.20 | 39.9 | 38.6 |
| Peace Vallis Channel: ESP_061117_1755 ESP_063530_1755 (Interval in Earth days: 188) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.23 | 137. | -10. | 2.574 | 52.3 | 56.5 |
| Eastern Exposure of Hargraves Crater Ejecta: ESP_061040_2010 ESP_069442_2010 (Interval in Earth days: 655) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 20.61 | 76.7 | -16. | 7.667 | 41.8 | 47.9 |
| Faulted and Embayed Low Shield East of Pavonis Mons: ESP_060783_1800 ESP_061139_1800 (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 | 0.196 | 253. | -5.6 | 17.40 | 46.9 | 48.0 |
| Candidate Landing Site for 2020 Mission in Jezero Crater: ESP_060829_1985 ESP_062161_1985 (Interval in Earth days: 104) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.45 | 77.0 | -19. | -28.8 | 41.5 | 47.5 |
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