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.
| Small Crater with Central Pit at High Latitudes: ESP_061667_2485 ESP_061746_2485 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 68.47 | 232. | -8.3 | 5.476 | 50.3 | 49.3 |
| Candidate Landing Site for 2020 and Sample Return Missions at Jezero Crater: ESP_061739_1985 ESP_061673_1985 (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 | 18.39 | 76.9 | -26. | -10.5 | 46.0 | 44.3 |
| Sinuous Ridge in Tempe Terra: ESP_061771_2245 ESP_061916_2245 (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 | 44.33 | 276. | 3.99 | 18.81 | 40.7 | 39.7 |
| Phlegra Montes: ESP_061762_2190 ESP_062118_2190 (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 | 38.63 | 164. | -1.8 | 13.72 | 40.7 | 40.3 |
| Fresh Exit Breach in Crater: ESP_061782_1480 ESP_061848_1480 (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 | -31.8 | 347. | -1.1 | -18.3 | 74.0 | 75.2 |
| East Ganges Chasma Dunes Interaction: ESP_061638_1725 ESP_061572_1725 (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 | -7.50 | 314. | -1.9 | 17.63 | 56.7 | 55.1 |
| Down in Chukhung Crater: ESP_060953_2185 ESP_060676_2185 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 38.36 | 287. | -0.4 | 14.28 | 39.7 | 38.7 |
| 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 |
| Glacial Features within Crater in Arabia Terra: ESP_061187_2155 ESP_087786_2155 (Interval in Earth days: 2072) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.14 | 19.9 | 4.85 | 25.65 | 39.1 | 40.0 |
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