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.
| Pitted Terrain in Ultima Lingula Region: ESP_040058_1020 ESP_040150_1020 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -77.8 | 154. | 2.49 | 23.68 | 58.9 | 58.2 |
| Crater on South Polar Layered Deposits: ESP_040228_0975 ESP_040254_0975 (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 | -82.2 | 198. | 4.92 | 22.36 | 63.3 | 62.5 |
| Degraded Cratered Cone between Isidis Planitia and Utopia Planitia: ESP_039941_2040 ESP_040152_2040 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.56 | 88.6 | 4.17 | -7.04 | 60.7 | 58.8 |
| Candidate ExoMars Landing Site in Oxia Palus Region: ESP_040182_1870 ESP_040815_1870 (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 | 7.026 | 349. | 16.0 | -4.22 | 45.8 | 39.9 |
| Spider Evolution: ESP_040285_0930 ESP_040205_0930 (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 | -87.0 | 98.7 | 14.5 | 28.16 | 67.3 | 65.5 |
| Candidate Landing Site for ExoMars Near Hypanis Valles: ESP_040091_1925 ESP_047884_1925 (Interval in Earth days: 607) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 12.47 | 314. | 2.78 | 22.11 | 51.3 | 55.0 |
| Candidate Landing Site for 2020 Mission in Mclaughlin Crater: ESP_040222_2020 ESP_040367_2020 (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 | 21.90 | 337. | -6.3 | 8.942 | 56.7 | 53.9 |
| Sinuous Ridge in Argyre Region: ESP_039933_1240 ESP_048860_1240 (Interval in Earth days: 695) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -55.8 | 318. | 2.08 | -7.99 | 44.6 | 43.1 |
| Slopes of Layered Deposits: ESP_040078_1715 ESP_048372_1715 (Interval in Earth days: 646) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.43 | 313. | -11. | 13.46 | 40.9 | 41.3 |
| Crater on South Polar Layered Deposits: ESP_040269_0970 ESP_040519_0970 (Interval in Earth days: 19) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -82.9 | 176. | -17. | 4.772 | 66.0 | 67.1 |
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