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.
| Intersecting Flow Fronts and Channels: ESP_084101_1845 ESP_084391_1845 (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 | 4.307 | 194. | 1.77 | 11.16 | 48.0 | 43.8 |
| Resistant Material in Olympus Mons Aureole Ridges: ESP_084192_2110 ESP_075502_2110 (Interval in Earth days: 677) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 30.57 | 226. | 3.71 | -6.18 | 64.8 | 63.6 |
| Small Delta or Fan: ESP_084359_2125 ESP_075524_2125 (Interval in Earth days: 688) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 32.17 | 345. | 4.69 | -7.02 | 63.9 | 64.7 |
| Inverted Channel in Noachis Terra: ESP_084385_1585 ESP_084451_1585 (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 | -21.1 | 2.82 | 0.76 | -22.6 | 35.6 | 37.2 |
| Fluvially Incised Terrain Northeast of Syrtis Major Planum: ESP_084369_2100 ESP_084514_2100 (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 | 29.56 | 73.9 | -5.8 | 4.318 | 62.3 | 59.8 |
| Recent Crater: ESP_084414_1385 ESP_084770_1385 (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 | -41.2 | 293. | 7.28 | -8.40 | 38.5 | 41.5 |
| Landforms above Subsurface Radar Observations of South Polar Cap: ESP_084325_1000 ESP_084562_1000 (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 | -80.0 | 222. | -6.3 | 13.65 | 62.6 | 64.0 |
| Gullied Slope: ESP_084477_1275 ESP_084411_1275 (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 | -51.9 | 16.5 | -8.1 | 8.426 | 44.9 | 43.5 |
| North Branch of Kasei Valles East of Labeatis Mensa: ESP_084493_2060 ESP_084058_2060 (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 | 25.76 | 287. | 8.43 | -6.75 | 57.0 | 63.3 |
| Sinuous Ridge Feeding Possible Lake Deposits: ESP_084101_1495 ESP_084325_1495 (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 | -30.0 | 199. | -4.7 | 26.25 | 37.7 | 34.0 |
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