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 Future Landing Site in Aram Chaos: ESP_032178_1820 ESP_032468_1820 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.186 | 339. | -7.4 | 14.63 | 35.4 | 32.8 |
| Light-Toned Materials Exposed along Ladon Valles Floor: ESP_032218_1625 ESP_040539_1625 (Interval in Earth days: 649) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -17.4 | 328. | 7.83 | -3.22 | 32.1 | 34.1 |
| South Polar Residual Cap in Summer: ESP_032390_0925 ESP_032521_0925 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.3 | 5.67 | 8.59 | 19.38 | 81.5 | 82.7 |
| Gullies with Light-Toned Apron Material Near Atlantis Chaos: ESP_032408_1425 ESP_049168_1425 (Interval in Earth days: 1306) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.0 | 183. | -0.8 | 12.53 | 43.0 | 32.7 |
| Dark Outcrops on South Polar Layered Deposits: ESP_032202_0905 ESP_041078_0905 (Interval in Earth days: 692) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -89.3 | 94.5 | 28.3 | 24.91 | 78.6 | 80.0 |
| Margin of Pedestal Crater in Malea Planum: ESP_032440_1225 ESP_032572_1225 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -56.9 | 32.9 | 5.48 | -22.0 | 57.2 | 61.0 |
| Exposure of South Polar Layered Deposits: ESP_032253_0920 ESP_040457_0920 (Interval in Earth days: 639) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.8 | 119. | 24.1 | 8.824 | 78.4 | 70.9 |
| Gullied Crater Walls: ESP_032356_1465 ESP_023943_1465 (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 | -32.9 | 164. | -21. | -4.37 | 41.4 | 45.6 |
| Lava Flow in Syria Planum: ESP_032326_1605 ESP_032827_1605 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.1 | 259. | 7.00 | 25.67 | 33.4 | 37.6 |
| Dark V-Shaped Feature Cutting across Layers or Bands on a Slope: ESP_032227_2040 ESP_040271_2040 (Interval in Earth days: 627) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.62 | 78.8 | -8.7 | 3.583 | 46.4 | 56.7 |
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