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.
| Equatorial-Facing Trough Exposure of North Polar Layered Deposits: ESP_071522_2665 ESP_071048_2665 (Interval in Earth days: 37) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 86.53 | 124. | -1.3 | -11.6 | 64.9 | 62.6 |
| Plates in Utopia Planitia: ESP_071551_2125 ESP_071986_2125 (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 | 32.11 | 95.3 | 1.52 | 25.72 | 47.6 | 47.6 |
| Dune Monitoring near Northeast Syrtis Major Region: ESP_071499_1975 ESP_071565_1975 (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 | 17.40 | 77.7 | -6.6 | -26.4 | 50.8 | 52.6 |
| East Candor Chasma Wall: ESP_071478_1730 ESP_071623_1730 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.79 | 294. | -8.1 | 7.154 | 61.3 | 59.7 |
| Mounds and Ridge in Oxia Colles: ESP_071595_2060 ESP_069736_2060 (Interval in Earth days: 145) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.65 | 333. | 16.6 | -7.16 | 47.1 | 49.6 |
| Hills in Phlegra Montes: ESP_071509_2165 ESP_071944_2165 (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 | 36.25 | 161. | -1.5 | 22.93 | 47.6 | 47.8 |
| West Flank of Chasma Boreale Barchan and Linear Dunes: ESP_070975_2645 ESP_071014_2645 (Interval in Earth days: 3) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.20 | 323. | -8.5 | 6.328 | 60.8 | 60.1 |
| Scarps in Milankovic Crater: ESP_071006_2345 ESP_071085_2345 (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 | 54.14 | 212. | -1.0 | 17.95 | 48.0 | 46.5 |
| Possible Layers in Korolev Crater: ESP_071047_2535 ESP_071034_2535 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 73.14 | 163. | 8.1 | -7.01 | 54.1 | 55.3 |
| Icy Scarp Monitoring: ESP_070807_2390 ESP_070886_2390 (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 | 58.59 | 244. | -1.6 | 14.96 | 48.9 | 47.5 |
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