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.
| Exposure of North Polar Layered Deposits: ESP_035567_2650 ESP_035909_2650 (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 | 84.92 | 294. | 0.21 | 15.65 | 60.1 | 60.9 |
| Landform Transition from Chaos Terrain to Outflow Channel: ESP_035475_1830 ESP_036042_1830 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.839 | 323. | -6.8 | 6.109 | 53.2 | 53.2 |
| Crater on Wall in Mamers Valles: ESP_035341_2195 ESP_035631_2195 (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 | 39.35 | 16.4 | 3.18 | 25.38 | 41.5 | 40.2 |
| Faulted Layered Deposits in West Candor Chasma: ESP_035582_1745 ESP_036070_1745 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.66 | 283. | -3.0 | -27.7 | 58.0 | 60.2 |
| Cratered Cones in Western Elysium Planitia: ESP_035521_1825 ESP_043987_1825 (Interval in Earth days: 659) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.375 | 146. | 8.82 | 22.29 | 52.4 | 48.1 |
| Exposure of North Polar Layered Deposits: ESP_035530_2665 ESP_044841_2665 (Interval in Earth days: 725) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 86.61 | 200. | 0.27 | -9.62 | 61.5 | 63.4 |
| Wall of Orson Welles Crater: ESP_035594_1790 ESP_071042_1790 (Interval in Earth days: 2761) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.76 | 314. | 0 | 19.68 | 54.9 | 57.3 |
| Filled Crater Near Marte Vallis: ESP_035058_2025 ESP_035348_2025 (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 | 22.27 | 185. | -1.7 | 23.87 | 43.4 | 41.9 |
| InSight Mission Candidate Landing Site: ESP_035284_1835 ESP_035218_1835 (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 | 3.302 | 137. | 4.62 | 25.88 | 51.6 | 49.7 |
| Domoni Crater Secondaries: ESP_034990_2335 ESP_035425_2335 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 53.10 | 236. | 2.93 | 25.72 | 43.7 | 41.8 |
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