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.
| Sinuous Troughs and Ridges near the Sirenum Fossae: ESP_017784_1425 ESP_026276_1425 (Interval in Earth days: 661) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.2 | 193. | 11.4 | -12.5 | 78.5 | 77.9 |
| Intact Stratigraphy in Crater Central Peak in Thaumasia Planum: ESP_018044_1540 ESP_018466_1540 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -25.7 | 295. | -3.9 | -17.4 | 71.1 | 71.3 |
| Flow Into Breached Crater in Central Elysium Planitia: ESP_018062_1810 ESP_018484_1810 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.837 | 160. | -8.0 | -21.3 | 54.3 | 55.6 |
| Small Channel in Elysium Planitia: ESP_017838_1865 ESP_017983_1865 (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 | 6.589 | 155. | -4.2 | 10.54 | 50.7 | 49.9 |
| Disrupted Blocky Outcrop in Cerberus Palus: ESP_018036_1880 ESP_043710_1880 (Interval in Earth days: 2001) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.089 | 149. | -6.4 | 6.703 | 50.5 | 45.5 |
| Central Uplift of Impact Crater in Tyrrhena Terra: ESP_017748_1665 ESP_026108_1665 (Interval in Earth days: 651) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.3 | 93.8 | 8.34 | 24.74 | 61.6 | 57.7 |
| Ridges and Flow-Like Forms: ESP_017734_2075 ESP_071880_2075 (Interval in Earth days: 4219) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 27.32 | 111. | -1.2 | 16.1 | 42.7 | 47.9 |
| Very Well-Preserved 10-Kilometer Diameter Impact Crater: ESP_017901_2375 ESP_017980_2375 (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 | 57.35 | 225. | 8.89 | 25.25 | 44.9 | 43.6 |
| Well-Preserved Oblique Impact Crater in Acidalia Planitia: ESP_017792_2285 ESP_018425_2285 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 47.90 | 323. | 9.53 | -4.67 | 42.0 | 45.6 |
| Cones at Edge of North Polar Layered Deposits: ESP_017885_2595 ESP_018004_2595 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.12 | 285. | 13.2 | -3.67 | 55.5 | 56.7 |
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